This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0
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 22.1055 2461093.6055 10.33 09:08:54.45 -24:08:34.9
251.42062 15.78006 galactic Pyx Second-epoch detections are separated by 1.1" 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 | ATO J137.2131-24.1385 | 09:08:53.79 -24:08:41.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8V 1988MSS...C04....0H HD 78674
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 J137.2131-24.1385,2461093.6055,10.33,0.05,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 J137.2131-24.1385 20260222.1055 10.33CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:54.45 -24:08:34.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.41 09:10:28.13 -23:17:23.2
250.98299 16.60415 galactic Pyx Second-epoch detections are separated by 5.4" 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 5651786914083002752 | 09:10:27.58 -23:17:28.8 (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 5651786914083002752,2461093.6055,10.41,0.05,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
Gaia DR3 5651786914083002752 20260222.1055 10.41CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:28.13 -23:17:23.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.54 09:08:48.30 -26:25:20.0
253.20057 14.28328 galactic Pyx Second-epoch detections are separated by 0.1" 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 5650051094460772352 | 09:08:47.90 -26:25:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1V 1982MSS...C03....0H HD 78703
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 5650051094460772352,2461093.6055,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5650051094460772352 20260222.1055 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:48.30 -26:25:20.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.76 09:08:47.12 -25:21:12.4
252.35866 14.97516 galactic Pyx Second-epoch detections are separated by 0.8" 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 5650280303978961792 | 09:08:46.64 -25:21:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6V 1988MSS...C04....0H HD 78675
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 5650280303978961792,2461093.6055,10.76,0.05,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 5650280303978961792 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:47.12 -25:21:12.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.85 09:09:45.66 -27:00:52.5
253.80688 14.05767 galactic Pyx Second-epoch detections are separated by 2.9" 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 5648287134215084288 | 09:09:45.21 -27:01:00.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6V 1982MSS...C03....0H HD 78877
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 5648287134215084288,2461093.6055,10.85,0.05,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 5648287134215084288 20260222.1055 10.85CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:45.66 -27:00:52.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.84 09:06:10.27 -30:59:27.2
256.35238 10.85605 galactic Pyx Second-epoch detections are separated by 1.6" 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 5635145530722466176 | 09:06:09.81 -30:59:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1982MSS...C03....0H HD 78222
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 5635145530722466176,2461093.6055,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635145530722466176 20260222.1055 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:10.27 -30:59:27.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.09 09:11:49.74 -22:13:56.6
250.35062 17.52661 galactic Hya Second-epoch detections are separated by 3.6" 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 | ATO J137.9637-22.2305 | 09:11:49.30 -22:14:03.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J137.9637-22.2305,2461093.6055,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J137.9637-22.2305 20260222.1055 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:49.74 -22:13:56.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.92 09:08:59.86 -30:23:58.2
256.30725 11.70279 galactic Pyx Second-epoch detections are separated by 0.7" 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 5635280186535545472 | 09:08:59.39 -30:23:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1925PASP...37...97V HD 78753
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 5635280186535545472,2461093.6055,10.92,0.05,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
Gaia DR3 5635280186535545472 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:59.86 -30:23:58.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.86 09:07:47.54 -29:57:09.4
255.78868 11.80186 galactic Pyx Second-epoch detections are separated by 3.9" 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 5635355743599911040 | 09:07:46.68 -29:57:14.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3V 1982MSS...C03....0H HD 78521
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 5635355743599911040,2461093.6055,10.86,0.05,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 5635355743599911040 20260222.1055 10.86CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:47.54 -29:57:09.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.74 09:06:48.27 -30:36:46.3
256.15309 11.20696 galactic Pyx Second-epoch detections are separated by 8.9" and 3.4 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 5635191980788033408 | 09:06:47.80 -30:36:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 1954AnCap..17.....J CD-30 7196
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 5635191980788033408,2461093.6055,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635191980788033408 20260222.1055 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:48.27 -30:36:46.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5651752515687994368,2461093.6055,11.18,0.05,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
Gaia DR3 5651752515687994368 20260222.1055 11.18CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:19.54 -23:32:20.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.13 09:11:47.17 -24:43:28.8
252.32270 15.90044 galactic Pyx Second-epoch detections are separated by 0.1" 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 5650699320987501952 | 09:11:46.72 -24:43:30.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1919AnHar..94.....C HD 79167
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 5650699320987501952,2461093.6055,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5650699320987501952 20260222.1055 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:47.17 -24:43:28.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.35 08:40:58.30 -23:27:03.0
246.79279 11.19032 galactic Pyx Second-epoch detections are separated by 0.7" and 3.5 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 5701750715316821248 | 08:40:58.67 -23:27:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3.5 1985ApJS...59..197B LTT 3215
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 5701750715316821248,2461093.6055,11.35,0.05,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
Gaia DR3 5701750715316821248 20260222.1055 11.35CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:58.30 -23:27:03.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5651592261868504320,2461093.6055,11.30,0.05,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 5651592261868504320 20260222.1055 11.30CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:50.09 -23:28:10.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.15 09:11:28.93 -30:14:13.7
256.54693 12.21158 galactic Pyx Second-epoch detections are separated by 1.7" and 4.2 pix
The object was found in VSX11" ASAS J091129-3014.4
Type: MISC
# Max. Min./Amp. JD0 Period
11.130 V Y 0.410 V 2454706.90000 1267.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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
ASAS J091129-3014.4,2461093.6055,11.15,0.05,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
ASAS J091129-3014.4 20260222.1055 11.15CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:28.93 -30:14:13.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.38 08:15:13.73 -30:25:32.3
249.21944 2.49015 galactic Pup Second-epoch detections are separated by 0.4" and 3.3 pix
The object was found in VSX 6" ASAS J081514-3025.6
Type: M
# Max. Min./Amp. JD0 Period
10.900 V 15.700 V 2452972.00000 287.000000000000 M6
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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
ASAS J081514-3025.6,2461093.6055,11.38,0.05,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
ASAS J081514-3025.6 20260222.1055 11.38CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:15:13.73 -30:25:32.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASAS J090032-2543.2,2461093.6055,11.42,0.05,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
ASAS J090032-2543.2 20260222.1055 11.42CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:00:31.59 -25:43:16.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
S Pyx,2461093.6055,9.30,0.05,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
S Pyx 20260222.1055 9.30CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:04.25 -25:05:21.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.13 08:33:37.49 -30:16:49.5
251.37865 5.82668 galactic Pyx Second-epoch detections are separated by 0.3" and 3.4 pix
The object was found in VSX 2" ASAS J083337-3016.8
Type: MISC
# Max. Min./Amp. JD0 Period
10.810 V Y 0.770 V 2452998.80000 164.200000000000 M5
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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
ASAS J083337-3016.8,2461093.6055,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J083337-3016.8 20260222.1055 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:33:37.49 -30:16:49.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
V0561 Pup,2461093.6055,9.81,0.05,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
V0561 Pup 20260222.1055 9.81CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:24:25.94 -24:21:25.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5655151385303917440,2461093.6055,13.85,0.05,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 5655151385303917440 20260222.1055 13.85CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:39.67 -22:12:42.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.52 09:08:17.56 -22:33:32.5
250.06259 16.69052 galactic Pyx Second-epoch detections are separated by 2.7" 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 5654974634513149056 | 09:08:17.00 -22:33:36.3 (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 5654974634513149056,2461093.6055,13.52,0.05,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 5654974634513149056 20260222.1055 13.52CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:17.56 -22:33:32.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.14 09:03:32.72 -30:43:56.1
255.77820 10.59881 galactic Pyx Second-epoch detections are separated by 3.1" 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 5635218854405392000 | 09:03:31.94 -30:43:54.7 (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 Lite
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 5635218854405392000,2461093.6055,13.14,0.05,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 5635218854405392000 20260222.1055 13.14CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:32.72 -30:43:56.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.29 08:03:08.94 -30:12:59.6
247.62694 0.41534 galactic Pup Second-epoch detections are separated by 3.6" and 2.7 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 5596276312914337792 | 08:03:09.45 -30:13:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.881+/-0.404 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 5596276312914337792,2461093.6055,13.29,0.05,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
Gaia DR3 5596276312914337792 20260222.1055 13.29CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:03:08.94 -30:12:59.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.18 09:03:25.60 -21:34:00.1
248.51622 16.44773 galactic Pyx Second-epoch detections are separated by 3.9" 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 5655236730598393216 | 09:03:25.39 -21:34:09.4 (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 5655236730598393216,2461093.6055,13.18,0.05,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
Gaia DR3 5655236730598393216 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:25.60 -21:34:00.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.09 09:03:16.09 -22:25:07.6
249.18178 15.88314 galactic Pyx Second-epoch detections are separated by 7.7" 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 5655124034952808960 | 09:03:15.75 -22:25:14.5 (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 5655124034952808960,2461093.6055,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655124034952808960 20260222.1055 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:16.09 -22:25:07.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.05 09:08:53.27 -27:49:48.4
254.31017 13.37681 galactic Pyx Second-epoch detections are separated by 5.6" 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 5648219960927196928 | 09:08:52.87 -27:49:51.0 (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 5648219960927196928,2461093.6055,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5648219960927196928 20260222.1055 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:53.27 -27:49:48.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.30 09:05:39.81 -22:50:17.9
249.88352 16.04540 galactic Pyx Second-epoch detections are separated by 6.8" 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 | ATO J136.4128-22.8373 | 09:05:39.73 -22:50:24.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J136.4128-22.8373,2461093.6055,13.30,0.05,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
ATO J136.4128-22.8373 20260222.1055 13.30CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:39.81 -22:50:17.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.26 09:08:24.57 -25:08:46.7
252.13835 15.04478 galactic Pyx Second-epoch detections are separated by 4.6" 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 5651034435812855424 | 09:08:24.45 -25:08:52.4 (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 5651034435812855424,2461093.6055,13.26,0.05,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 5651034435812855424 20260222.1055 13.26CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:24.57 -25:08:46.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.75 09:08:51.21 -24:26:52.8
251.65407 15.57356 galactic Pyx Second-epoch detections are separated by 2.9" 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 5651141054080778496 | 09:08:51.48 -24:26:45.2 (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 5651141054080778496,2461093.6055,12.75,0.05,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 5651141054080778496 20260222.1055 12.75CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:51.21 -24:26:52.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.56 09:06:56.51 -26:03:54.9
252.64058 14.19756 galactic Pyx Second-epoch detections are separated by 0.5" 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 5650124551284082944 | 09:06:56.99 -26:03:54.8 (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 5650124551284082944,2461093.6055,12.56,0.05,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 5650124551284082944 20260222.1055 12.56CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:56.51 -26:03:54.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.40 09:05:03.04 -30:24:57.1
255.74914 11.05077 galactic Pyx Second-epoch detections are separated by 6.0" 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 5635253111065005440 | 09:05:01.96 -30:24:57.4 (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 Lite
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 5635253111065005440,2461093.6055,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635253111065005440 20260222.1055 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:03.04 -30:24:57.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.61 09:04:41.48 -21:29:06.2
248.64301 16.72774 galactic Pyx Second-epoch detections are separated by 2.1" 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 5655334831946968576 | 09:04:41.21 -21:29:15.1 (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 5655334831946968576,2461093.6055,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655334831946968576 20260222.1055 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:41.48 -21:29:06.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.47 08:49:02.67 -26:34:04.2
250.44883 10.76856 galactic Pyx Second-epoch detections are separated by 4.5" and 3.0 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 | ATO J132.2611-26.5681 | 08:49:02.13 -26:34:02.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.390+/-0.078 (G)
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 J132.2611-26.5681,2461093.6055,12.47,0.05,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 J132.2611-26.5681 20260222.1055 12.47CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:49:02.67 -26:34:04.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.51 08:51:35.56 -30:05:21.3
253.60660 9.02541 galactic Pyx Second-epoch detections are separated by 4.2" 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 | ATO J132.9047-30.0895 | 08:51:35.10 -30:05:10.8 (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 Lite
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 J132.9047-30.0895,2461093.6055,12.51,0.05,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
ATO J132.9047-30.0895 20260222.1055 12.51CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:51:35.56 -30:05:21.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.23 09:04:00.80 -22:04:46.7
249.02094 16.23078 galactic Pyx Second-epoch detections are separated by 6.5" 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 5655157119083630976 | 09:04:00.47 -22:04:52.2 (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 5655157119083630976,2461093.6055,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655157119083630976 20260222.1055 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:00.80 -22:04:46.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.93 09:03:43.39 -26:39:29.7
252.62840 13.26411 galactic Pyx Second-epoch detections are separated by 8.6" and 3.1 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 5648588121225504000 | 09:03:43.01 -26:39:33.0 (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 5648588121225504000,2461093.6055,11.93,0.05,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 5648588121225504000 20260222.1055 11.93CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:43.39 -26:39:29.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5656006010779929600,2461093.6055,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5656006010779929600 20260222.1055 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:02:27.14 -21:22:11.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.36 09:08:50.98 -23:43:44.3
251.08284 16.03714 galactic Pyx Second-epoch detections are separated by 0.3" 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 5651746300872851840 | 09:08:50.46 -23:43:50.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A9V 1988MSS...C04....0H HD 78673
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 5651746300872851840,2461093.6055,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651746300872851840 20260222.1055 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:50.98 -23:43:44.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.43 09:06:24.33 -21:29:19.7
248.90923 17.03453 galactic Pyx Second-epoch detections are separated by 2.4" 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 5655307511659063424 | 09:06:23.86 -21:29:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0m:A2-F0: 1988MSS...C04....0H HD 78199
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 5655307511659063424,2461093.6055,10.43,0.05,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 5655307511659063424 20260222.1055 10.43CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:24.33 -21:29:19.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.59 09:10:53.24 -21:44:08.1
249.80438 17.67954 galactic Hya Second-epoch detections are separated by 2.0" 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 | Large-amplitude variable Gaia DR2 5679059337935950592 | 09:10:52.80 -21:44:12.0 (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: F3/5IV 1988MSS...C04....0H HD 79014
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 5679059337935950592,2461093.6055,10.59,0.05,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
Large-amplitude variable Gaia DR2 5679059337935950592 20260222.1055 10.59CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:53.24 -21:44:08.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.58 09:08:48.77 -26:25:21.9
253.20217 14.28426 galactic Pyx Second-epoch detections are separated by 1.2" 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 5650051094460772352 | 09:08:47.90 -26:25:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1V 1982MSS...C03....0H HD 78703
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 5650051094460772352,2461093.6055,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5650051094460772352 20260222.1055 10.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:48.77 -26:25:21.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.64 09:03:58.06 -29:46:09.4
255.09362 11.29444 galactic Pyx Second-epoch detections are separated by 3.2" 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 | Gaia DR3 5635478369207335168 | 09:03:57.10 -29:46:08.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0V 1982MSS...C03....0H HD 77842
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 5635478369207335168,2461093.6055,10.64,0.05,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 5635478369207335168 20260222.1055 10.64CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:58.06 -29:46:09.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.90 09:05:53.23 -24:45:40.8
251.45222 14.85603 galactic Pyx Second-epoch detections are separated by 2.3" and 3.5 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 5651027701304144000 | 09:05:52.81 -24:45:44.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5IV: 1988MSS...C04....0H HD 78144
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 5651027701304144000,2461093.6055,10.90,0.05,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 5651027701304144000 20260222.1055 10.90CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:53.23 -24:45:40.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASAS J091026-2941.2,2461093.6055,10.78,0.05,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
ASAS J091026-2941.2 20260222.1055 10.78CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:25.71 -29:41:27.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5655090293689021440,2461093.6055,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655090293689021440 20260222.1055 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:48.78 -21:42:07.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 10.94 09:09:46.25 -27:00:56.4
253.80920 14.05862 galactic Pyx Second-epoch detections are separated by 3.4" 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 5648287134215084288 | 09:09:45.21 -27:01:00.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6V 1982MSS...C03....0H HD 78877
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 5648287134215084288,2461093.6055,10.94,0.05,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 5648287134215084288 20260222.1055 10.94CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:46.25 -27:00:56.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J091206.39-282903.2,2461093.6055,10.90,0.05,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
ASASSN-V J091206.39-282903.2 20260222.1055 10.90CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:05.90 -28:29:09.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.07 09:08:56.41 -22:23:23.5
250.02693 16.91373 galactic Pyx Second-epoch detections are separated by 2.6" 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 5654986389840447104 | 09:08:55.91 -22:23:29.4 (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 5654986389840447104,2461093.6055,11.07,0.05,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
Gaia DR3 5654986389840447104 20260222.1055 11.07CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:56.41 -22:23:23.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.09 09:10:14.41 -26:31:16.2
253.49454 14.46174 galactic Pyx Second-epoch detections are separated by 1.7" 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 5649852941850830976 | 09:10:13.47 -26:31:23.6 (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 5649852941850830976,2461093.6055,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5649852941850830976 20260222.1055 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:14.41 -26:31:16.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASAS J091032-2943.8,2461093.6055,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J091032-2943.8 20260222.1055 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:31.78 -29:44:06.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.01 09:10:51.23 -29:40:12.2
256.02069 12.48699 galactic Pyx Second-epoch detections are separated by 3.6" 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 5635713050520644736 | 09:10:51.42 -29:39:57.7 (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 5635713050520644736,2461093.6055,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635713050520644736 20260222.1055 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:51.23 -29:40:12.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.22 09:09:20.14 -23:46:23.0
251.19255 16.09368 galactic Pyx Second-epoch detections are separated by 0.4" 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 5651557352374511616 | 09:09:19.45 -23:46:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5651557352374511616,2461093.6055,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651557352374511616 20260222.1055 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:20.14 -23:46:23.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5636130143383954816,2461093.6055,11.10,0.05,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
Gaia DR3 5636130143383954816 20260222.1055 11.10CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:08.45 -28:14:18.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.24 09:12:16.59 -23:52:49.5
251.73225 16.53590 galactic Hya Second-epoch detections are separated by 1.0" 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 5651514677579463936 | 09:12:15.93 -23:52:55.0 (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 5651514677579463936,2461093.6055,11.24,0.05,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 5651514677579463936 20260222.1055 11.24CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:16.59 -23:52:49.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.12 09:11:31.31 -28:08:30.1
254.94511 13.60922 galactic Pyx Second-epoch detections are separated by 3.7" 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 | ATO J137.8844-28.1411 | 09:11:30.40 -28:08:28.5 (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 J137.8844-28.1411,2461093.6055,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J137.8844-28.1411 20260222.1055 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:31.31 -28:08:30.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.31 09:06:38.77 -22:21:59.1
249.65452 16.52058 galactic Pyx Second-epoch detections are separated by 3.2" 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 | ATO J136.6693-22.3655 | 09:06:38.17 -22:22:07.5 (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 J136.6693-22.3655,2461093.6055,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J136.6693-22.3655 20260222.1055 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:38.77 -22:21:59.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.46 09:10:35.80 -22:32:49.8
250.41012 17.10590 galactic Pyx Second-epoch detections are separated by 5.1" 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 5651964416491866368 | 09:10:35.36 -22:32:54.9 (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 5651964416491866368,2461093.6055,11.46,0.05,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 5651964416491866368 20260222.1055 11.46CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:35.80 -22:32:49.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5636223601868907520,2461093.6055,11.23,0.05,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
Gaia DR3 5636223601868907520 20260222.1055 11.23CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:36.22 -27:45:46.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.30 08:47:38.91 -28:22:08.9
251.69899 9.41736 galactic Pyx Second-epoch detections are separated by 6.5" 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 | ATO J131.9066-28.3627 | 08:47:37.49 -28:22:24.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F3V 1982MSS...C03....0H HD 75198
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 J131.9066-28.3627,2461093.6055,11.30,0.05,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
ATO J131.9066-28.3627 20260222.1055 11.30CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:47:38.91 -28:22:08.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.37 09:06:48.78 -27:20:24.9
253.62028 13.34841 galactic Pyx Second-epoch detections are separated by 1.1" 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 5648296166526313728 | 09:06:48.08 -27:20:28.9 (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 5648296166526313728,2461093.6055,11.37,0.05,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 5648296166526313728 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:48.78 -27:20:24.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5651109129587008640,2461093.6055,11.38,0.05,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 5651109129587008640 20260222.1055 11.38CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:32.19 -24:45:06.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.36 09:07:03.26 -26:49:35.7
253.25463 13.72306 galactic Pyx Second-epoch detections are separated by 2.3" 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 5648536031861353600 | 09:07:02.53 -26:49:42.6 (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 5648536031861353600,2461093.6055,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5648536031861353600 20260222.1055 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:03.26 -26:49:35.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.46 09:07:53.25 -26:27:02.9
253.08502 14.10877 galactic Pyx Second-epoch detections are separated by 1.7" 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 | ATO J136.9793-26.4512 | 09:07:53.19 -26:27:09.9 (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 J136.9793-26.4512,2461093.6055,11.46,0.05,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
ATO J136.9793-26.4512 20260222.1055 11.46CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:53.25 -26:27:02.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.32 09:08:05.80 -29:01:46.8
255.12183 12.45848 galactic Pyx Second-epoch detections are separated by 7.6" 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 | ATO J137.0205-29.0219 | 09:08:05.03 -29:01:53.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J137.0205-29.0219,2461093.6055,11.32,0.05,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 J137.0205-29.0219 20260222.1055 11.32CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:05.80 -29:01:46.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.39 09:10:24.74 -27:07:23.8
253.98952 14.09579 galactic Pyx Second-epoch detections are separated by 1.2" 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 | Gaia DR3 5648282044673821184 | 09:10:23.91 -27:07:24.7 (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 5648282044673821184,2461093.6055,11.39,0.05,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 5648282044673821184 20260222.1055 11.39CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:24.74 -27:07:23.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J090336.45-212840.9,2461093.6055,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J090336.45-212840.9 20260222.1055 11.47CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:37.20 -21:29:03.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.47 09:08:11.83 -24:35:02.3
251.66163 15.37176 galactic Pyx Second-epoch detections are separated by 4.0" 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 | ATO J137.0561-24.5875 | 09:08:11.47 -24:35:06.8 (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 J137.0561-24.5875,2461093.6055,11.47,0.05,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 J137.0561-24.5875 20260222.1055 11.47CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:11.83 -24:35:02.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.44 09:10:14.50 -29:45:07.9
255.99339 12.33303 galactic Pyx Second-epoch detections are separated by 7.3" and 3.5 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 5635711023294572928 | 09:10:13.68 -29:44:52.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1982MSS...C03....0H HD 78973
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 5635711023294572928,2461093.6055,11.44,0.05,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
Gaia DR3 5635711023294572928 20260222.1055 11.44CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:14.50 -29:45:07.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5651592261868504320,2461093.6055,11.62,0.05,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 5651592261868504320 20260222.1055 11.62CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:50.42 -23:28:06.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASAS J090856-2124.4,2461093.6055,11.57,0.05,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
ASAS J090856-2124.4 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:56.17 -21:24:19.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.62 09:06:28.01 -25:39:28.1
252.24849 14.37938 galactic Pyx Second-epoch detections are separated by 1.5" and 3.5 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 | ATO J136.6216-25.6555 | 09:06:27.50 -25:39:33.8 (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 J136.6216-25.6555,2461093.6055,11.62,0.05,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
ATO J136.6216-25.6555 20260222.1055 11.62CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:28.01 -25:39:28.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.55 09:08:55.33 -27:27:36.7
254.02787 13.62490 galactic Pyx Second-epoch detections are separated by 5.8" 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 5648247036400946304 | 09:08:54.42 -27:27:39.2 (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 5648247036400946304,2461093.6055,11.55,0.05,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 5648247036400946304 20260222.1055 11.55CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:55.33 -27:27:36.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.71 09:10:56.07 -22:03:38.8
250.07305 17.47886 galactic Hya Second-epoch detections are separated by 1.4" 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 5655019409548945024 | 09:10:55.55 -22:03:43.8 (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 5655019409548945024,2461093.6055,11.71,0.05,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 5655019409548945024 20260222.1055 11.71CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:56.07 -22:03:38.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.59 09:11:21.31 -23:59:38.2
251.67924 16.30219 galactic Hya Second-epoch detections are separated by 1.7" 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 5651489457531507968 | 09:11:20.62 -23:59:46.1 (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 5651489457531507968,2461093.6055,11.59,0.05,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 5651489457531507968 20260222.1055 11.59CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:21.31 -23:59:38.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.64 09:12:16.76 -22:45:52.7
250.84644 17.26159 galactic Hya Second-epoch detections are separated by 2.3" 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 5651918507585008640 | 09:12:16.18 -22:45:57.7 (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 5651918507585008640,2461093.6055,11.64,0.05,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 5651918507585008640 20260222.1055 11.64CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:16.76 -22:45:52.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.71 09:08:40.94 -22:05:45.3
249.75085 17.05602 galactic Pyx Second-epoch detections are separated by 3.2" 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 5655006799524870784 | 09:08:40.54 -22:05:51.1 (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 5655006799524870784,2461093.6055,11.71,0.05,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 5655006799524870784 20260222.1055 11.71CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:40.94 -22:05:45.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.67 09:10:33.15 -22:26:26.5
250.31802 17.16667 galactic Pyx Second-epoch detections are separated by 4.9" and 3.0 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 5652000455560005504 | 09:10:32.63 -22:26:35.8 (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 5652000455560005504,2461093.6055,11.67,0.05,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 5652000455560005504 20260222.1055 11.67CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:33.15 -22:26:26.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.63 09:04:14.69 -21:26:46.2
248.54318 16.67150 galactic Pyx Second-epoch detections are separated by 5.9" 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 | ATO J136.0604-21.4595 | 09:04:14.36 -21:26:53.3 (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 J136.0604-21.4595,2461093.6055,11.63,0.05,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
ATO J136.0604-21.4595 20260222.1055 11.63CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:14.69 -21:26:46.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5635659273232501632,2461093.6055,11.59,0.05,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 5635659273232501632 20260222.1055 11.59CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:53.74 -29:11:21.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5634412156468905344,2461093.6055,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5634412156468905344 20260222.1055 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:23.80 -31:06:47.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.55 09:12:20.13 -29:47:54.1
256.33807 12.64175 galactic Pyx 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 5634950470485566080 | 09:12:19.42 -29:47:55.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3/5III 1982MSS...C03....0H HD 79291
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 5634950470485566080,2461093.6055,11.55,0.05,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 5634950470485566080 20260222.1055 11.55CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:20.13 -29:47:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.58 09:08:06.33 -29:40:44.4
255.62382 12.03306 galactic Pyx Second-epoch detections are separated by 6.9" 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 5635395527880249088 | 09:08:05.50 -29:40:48.5 (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 5635395527880249088,2461093.6055,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635395527880249088 20260222.1055 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:06.33 -29:40:44.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.72 09:11:48.09 -24:58:00.1
252.51547 15.74491 galactic Pyx Second-epoch detections are separated by 1.1" 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 | Large-amplitude variable Gaia DR2 5650307349389075456 | 09:11:47.40 -24:58:04.8 (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 5650307349389075456,2461093.6055,11.72,0.05,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
Large-amplitude variable Gaia DR2 5650307349389075456 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:48.09 -24:58:00.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.57 09:08:10.98 -29:56:02.5
255.83133 11.87779 galactic Pyx Second-epoch detections are separated by 7.5" 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 5635376698741507456 | 09:08:10.17 -29:56:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2/3III 1982MSS...C03....0H HD 78591
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 5635376698741507456,2461093.6055,11.57,0.05,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 5635376698741507456 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:10.98 -29:56:02.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.55 09:08:58.79 -30:23:55.5
256.30408 11.70041 galactic Pyx Second-epoch detections are separated by 1.2" 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 5635280186535545472 | 09:08:59.39 -30:23:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1925PASP...37...97V HD 78753
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 5635280186535545472,2461093.6055,11.55,0.05,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 5635280186535545472 20260222.1055 11.55CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:58.79 -30:23:55.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.77 09:11:54.01 -22:10:14.2
250.31229 17.57908 galactic Hya Second-epoch detections are separated by 1.3" 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 5676030935020873344 | 09:11:53.55 -22:10:17.5 (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 5676030935020873344,2461093.6055,11.77,0.05,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 5676030935020873344 20260222.1055 11.77CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:54.01 -22:10:14.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.81 09:09:49.25 -22:58:42.0
250.63432 16.69132 galactic Pyx Second-epoch detections are separated by 2.5" 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 5651947236622150528 | 09:09:48.63 -22:58:49.3 (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 5651947236622150528,2461093.6055,11.81,0.05,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 5651947236622150528 20260222.1055 11.81CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:49.25 -22:58:42.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.75 09:09:21.06 -25:53:25.9
252.86654 14.72274 galactic Pyx Second-epoch detections are separated by 2.8" 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 5650107135193810944 | 09:09:20.95 -25:53:32.1 (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 5650107135193810944,2461093.6055,11.75,0.05,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 5650107135193810944 20260222.1055 11.75CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:21.06 -25:53:25.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.62 09:08:12.59 -26:40:44.5
253.31201 14.01497 galactic Pyx Second-epoch detections are separated by 4.9" and 3.4 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 5648357636100262784 | 09:08:12.01 -26:40:45.9 (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 5648357636100262784,2461093.6055,11.62,0.05,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 5648357636100262784 20260222.1055 11.62CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:12.59 -26:40:44.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.65 09:11:06.94 -27:50:55.7
254.65790 13.73547 galactic Pyx Second-epoch detections are separated by 4.0" 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 | ATO J137.7757-27.8382 | 09:11:06.00 -27:51:04.1 (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 J137.7757-27.8382,2461093.6055,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J137.7757-27.8382 20260222.1055 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:06.94 -27:50:55.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.94 09:05:10.96 -21:21:30.8
248.61569 16.89624 galactic Pyx Second-epoch detections are separated by 2.6" 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 5655337408927319680 | 09:05:10.38 -21:21:39.6 (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 5655337408927319680,2461093.6055,11.94,0.05,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 5655337408927319680 20260222.1055 11.94CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:10.96 -21:21:30.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.61 09:09:48.69 -29:42:33.4
255.89718 12.29146 galactic Pyx Second-epoch detections are separated by 3.5" 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 5635339903762033408 | 09:09:48.50 -29:42:19.6 (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 5635339903762033408,2461093.6055,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635339903762033408 20260222.1055 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:48.69 -29:42:33.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5635456207176107520,2461093.6055,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635456207176107520 20260222.1055 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:52.71 -30:04:08.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.67 09:09:42.79 -29:26:29.6
255.67709 12.45245 galactic Pyx Second-epoch detections are separated by 3.5" 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 | ATO J137.4319-29.4377 | 09:09:41.57 -29:26:19.3 (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 J137.4319-29.4377,2461093.6055,11.67,0.05,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 J137.4319-29.4377 20260222.1055 11.67CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:42.79 -29:26:29.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.69 09:11:10.25 -30:08:57.2
256.43398 12.21992 galactic Pyx Second-epoch detections are separated by 3.8" and 3.4 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 5634563957788756864 | 09:11:10.73 -30:08:58.2 (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 Lite
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 5634563957788756864,2461093.6055,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5634563957788756864 20260222.1055 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:10.25 -30:08:57.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5651456300384008064,2461093.6055,11.82,0.05,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 5651456300384008064 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:12.53 -24:31:13.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
UNSW-V 399,2461093.6055,11.91,0.05,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
UNSW-V 399 20260222.1055 11.91CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:53.62 -22:09:26.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.88 09:11:42.14 -22:51:43.0
250.83387 17.09726 galactic Hya Second-epoch detections are separated by 1.7" 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 5651905626978891904 | 09:11:41.64 -22:51:47.5 (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 5651905626978891904,2461093.6055,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651905626978891904 20260222.1055 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:42.14 -22:51:43.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.82 09:10:26.74 -24:50:45.0
252.21203 15.59075 galactic Pyx Second-epoch detections are separated by 1.6" 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 5650319237858584320 | 09:10:26.08 -24:50:50.2 (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 5650319237858584320,2461093.6055,11.82,0.05,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 5650319237858584320 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:26.74 -24:50:45.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.57 09:00:58.49 -31:13:07.4
255.79115 9.86391 galactic Pyx Second-epoch detections are separated by 4.8" 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 5629179718071062400 | 09:00:59.11 -31:13:10.9 (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 Lite
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 5629179718071062400,2461093.6055,11.57,0.05,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 5629179718071062400 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:00:58.49 -31:13:07.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.93 09:04:17.90 -21:43:34.0
248.77831 16.50493 galactic Pyx Second-epoch detections are separated by 1.5" 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 5655183816601330688 | 09:04:17.43 -21:43:42.3 (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 5655183816601330688,2461093.6055,11.93,0.05,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 5655183816601330688 20260222.1055 11.93CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:17.90 -21:43:34.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.72 09:05:03.80 -26:38:49.0
252.81768 13.50051 galactic Pyx Second-epoch detections are separated by 7.4" 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 5648580081044452352 | 09:05:03.41 -26:38:52.8 (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 5648580081044452352,2461093.6055,11.72,0.05,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 5648580081044452352 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:03.80 -26:38:49.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
SSS_J091127.3-244305,2461093.6055,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SSS_J091127.3-244305 20260222.1055 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:26.14 -24:42:59.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.04 09:10:35.06 -23:20:36.4
251.04360 16.58967 galactic Pyx Second-epoch detections are separated by 8.9" 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 5651782103719632128 | 09:10:34.74 -23:20:46.6 (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 5651782103719632128,2461093.6055,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651782103719632128 20260222.1055 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:35.06 -23:20:36.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.71 09:07:21.40 -26:57:41.5
253.40529 13.68658 galactic Pyx Second-epoch detections are separated by 5.6" and 3.4 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 5648345648851114752 | 09:07:20.96 -26:57:42.9 (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 5648345648851114752,2461093.6055,11.71,0.05,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 5648345648851114752 20260222.1055 11.71CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:21.40 -26:57:41.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.73 09:10:14.77 -30:25:45.1
256.51220 11.88469 galactic Pyx Second-epoch detections are separated by 3.4" and 4.4 pix
The object was found in VSX 8" ASAS J091015-3025.8
Type: MISC
# Max. Min./Amp. JD0 Period
11.010 V Y 0.290 V 2452324.20000 198.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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
ASAS J091015-3025.8,2461093.6055,11.73,0.05,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
ASAS J091015-3025.8 20260222.1055 11.73CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:14.77 -30:25:45.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.88 09:09:16.78 -28:38:16.7
254.99390 12.91122 galactic Pyx Second-epoch detections are separated by 1.2" 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 5636029808648407296 | 09:09:15.98 -28:38:25.3 (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 5636029808648407296,2461093.6055,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5636029808648407296 20260222.1055 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:16.78 -28:38:16.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5634412156468905344,2461093.6055,11.77,0.05,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 5634412156468905344 20260222.1055 11.77CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:22.60 -31:06:42.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.86 09:12:18.81 -29:47:52.8
256.33453 12.63844 galactic Pyx Second-epoch detections are separated by 0.9" 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 5634950470485566080 | 09:12:19.42 -29:47:55.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3/5III 1982MSS...C03....0H HD 79291
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 5634950470485566080,2461093.6055,11.86,0.05,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 5634950470485566080 20260222.1055 11.86CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:18.81 -29:47:52.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.84 09:02:38.01 -30:57:43.0
255.82625 10.30076 galactic Pyx Second-epoch detections are separated by 1.1" and 3.7 pix
The object was found in VSX 9" ASAS J090239-3057.8
Type: M|SR
# Max. Min./Amp. JD0 Period
9.352 Ic Y 2.445 Ic 2453091.30000 354.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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
ASAS J090239-3057.8,2461093.6055,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J090239-3057.8 20260222.1055 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:02:38.01 -30:57:43.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.81 09:10:25.49 -30:30:23.2
256.59734 11.86215 galactic Pyx Second-epoch detections are separated by 2.6" 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 5634525096925052160 | 09:10:26.37 -30:30:22.3 (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 Lite
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 5634525096925052160,2461093.6055,11.81,0.05,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 5634525096925052160 20260222.1055 11.81CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:25.49 -30:30:23.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.03 09:12:22.19 -24:15:43.0
252.04822 16.30318 galactic Hya Second-epoch detections are separated by 3.2" 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 5651467368515964672 | 09:12:21.59 -24:15:49.1 (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 5651467368515964672,2461093.6055,12.03,0.05,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 5651467368515964672 20260222.1055 12.03CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:22.19 -24:15:43.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
BR Pyx,2461093.6055,11.85,0.05,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
BR Pyx 20260222.1055 11.85CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:14.12 -29:29:36.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.86 09:09:58.84 -28:58:44.9
255.36086 12.80175 galactic Pyx Second-epoch detections are separated by 2.9" 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 5635820940097149312 | 09:09:58.00 -28:58:44.8 (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 5635820940097149312,2461093.6055,11.86,0.05,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 5635820940097149312 20260222.1055 11.86CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:58.84 -28:58:44.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.01 09:11:33.73 -22:28:15.9
250.49987 17.32536 galactic Hya Second-epoch detections are separated by 4.1" and 3.4 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 5651986509803178880 | 09:11:33.22 -22:28:24.5 (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 5651986509803178880,2461093.6055,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651986509803178880 20260222.1055 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:33.73 -22:28:15.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5651459770717582080,2461093.6055,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651459770717582080 20260222.1055 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:09.08 -24:27:13.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.98 09:05:32.15 -28:25:49.8
254.28171 12.42506 galactic Pyx Second-epoch detections are separated by 1.6" 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 5648083758923689472 | 09:05:31.43 -28:25:55.8 (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 5648083758923689472,2461093.6055,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5648083758923689472 20260222.1055 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:32.15 -28:25:49.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5651165243336476544,2461093.6055,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651165243336476544 20260222.1055 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:30.00 -24:12:05.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.02 09:05:53.38 -29:12:04.9
254.93175 11.98170 galactic Pyx Second-epoch detections are separated by 2.5" and 3.4 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 5635659273232501632 | 09:05:52.77 -29:11:24.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5635659273232501632,2461093.6055,12.02,0.05,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 5635659273232501632 20260222.1055 12.02CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:53.38 -29:12:04.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.01 09:09:06.49 -29:44:29.3
255.81863 12.15559 galactic Pyx Second-epoch detections are separated by 3.2" 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 | ATO J137.2720-29.7314 | 09:09:06.40 -29:44:15.1 (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 J137.2720-29.7314,2461093.6055,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J137.2720-29.7314 20260222.1055 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:06.49 -29:44:29.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.14 09:06:11.50 -22:09:10.8
249.41291 16.57505 galactic Pyx Second-epoch detections are separated by 4.6" 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 5654967491983995776 | 09:06:11.05 -22:09:18.7 (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 5654967491983995776,2461093.6055,12.14,0.05,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 5654967491983995776 20260222.1055 12.14CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:11.50 -22:09:10.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.16 09:08:21.44 -24:36:45.5
251.70872 15.38104 galactic Pyx Second-epoch detections are separated by 2.4" and 3.5 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 5651114528362802432 | 09:08:20.90 -24:36:50.2 (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 5651114528362802432,2461093.6055,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651114528362802432 20260222.1055 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:21.44 -24:36:45.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.28 09:09:31.50 -21:51:06.3
249.68522 17.36238 galactic Pyx Second-epoch detections are separated by 4.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J137.3886-21.8505 | 09:09:31.02 -21:51:12.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J137.3886-21.8505,2461093.6055,12.28,0.05,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 J137.3886-21.8505 20260222.1055 12.28CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:31.50 -21:51:06.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.99 09:08:06.50 -27:30:22.4
253.94227 13.45825 galactic Pyx Second-epoch detections are separated by 3.8" 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 5648248445151437696 | 09:08:06.10 -27:30:25.4 (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 5648248445151437696,2461093.6055,11.99,0.05,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 5648248445151437696 20260222.1055 11.99CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:06.50 -27:30:22.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.13 09:09:28.31 -27:33:27.2
254.18574 13.65315 galactic Pyx Second-epoch detections are separated by 1.2" 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 5648230749881917952 | 09:09:27.53 -27:33:28.1 (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 5648230749881917952,2461093.6055,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5648230749881917952 20260222.1055 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:28.31 -27:33:27.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.11 09:11:46.37 -28:32:15.6
255.28785 13.38837 galactic Pyx Second-epoch detections are separated by 4.1" 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 5635928795316294912 | 09:11:45.91 -28:32:09.4 (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 5635928795316294912,2461093.6055,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635928795316294912 20260222.1055 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:46.37 -28:32:15.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.05 09:08:09.66 -29:56:02.1
255.82803 11.87427 galactic Pyx Second-epoch detections are separated by 1.5" 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 5635376698741507456 | 09:08:10.17 -29:56:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2/3III 1982MSS...C03....0H HD 78591
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 5635376698741507456,2461093.6055,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635376698741507456 20260222.1055 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:09.66 -29:56:02.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.04 09:04:39.69 -30:23:09.8
255.67032 11.00668 galactic Pyx Second-epoch detections are separated by 5.4" 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 5635256783256374144 | 09:04:38.30 -30:23:17.3 (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 Lite
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 5635256783256374144,2461093.6055,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635256783256374144 20260222.1055 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:39.69 -30:23:09.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.27 09:06:17.96 -22:23:56.3
249.62753 16.43801 galactic Pyx Second-epoch detections are separated by 1.9" 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 5654948353610509696 | 09:06:17.29 -22:24:07.0 (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 5654948353610509696,2461093.6055,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5654948353610509696 20260222.1055 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:17.96 -22:23:56.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.24 09:09:22.70 -23:43:53.1
251.16602 16.12801 galactic Pyx Second-epoch detections are separated by 4.1" and 3.4 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 5651745613677537536 | 09:09:22.01 -23:43:59.3 (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 5651745613677537536,2461093.6055,12.24,0.05,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 5651745613677537536 20260222.1055 12.24CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:22.70 -23:43:53.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.26 09:06:31.48 -21:59:03.9
249.32809 16.74169 galactic Pyx Second-epoch detections are separated by 4.6" 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 5655065172425203200 | 09:06:30.99 -21:59:13.0 (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 5655065172425203200,2461093.6055,12.26,0.05,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 5655065172425203200 20260222.1055 12.26CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:31.48 -21:59:03.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.34 09:08:15.67 -22:00:11.5
249.61103 17.04017 galactic Pyx Second-epoch detections are separated by 4.6" 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 5655055418554664576 | 09:08:15.29 -22:00:16.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5655055418554664576,2461093.6055,12.34,0.05,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
Gaia DR3 5655055418554664576 20260222.1055 12.34CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:15.67 -22:00:11.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.43 09:08:42.70 -22:26:12.6
250.02927 16.84309 galactic Pyx Second-epoch detections are separated by 2.6" 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 5654980308166807808 | 09:08:42.05 -22:26:25.3 (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 5654980308166807808,2461093.6055,12.43,0.05,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 5654980308166807808 20260222.1055 12.43CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:42.70 -22:26:12.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5679320746826445440,2461093.6055,12.32,0.05,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 5679320746826445440 20260222.1055 12.32CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:31.98 -21:20:37.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5635923469556475264,2461093.6055,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635923469556475264 20260222.1055 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:33.46 -28:39:03.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.28 09:10:11.27 -25:03:40.8
252.34232 15.40611 galactic Pyx 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 | Large-amplitude variable Gaia DR2 5650288966927330432 | 09:10:10.61 -25:03:46.9 (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 5650288966927330432,2461093.6055,12.28,0.05,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 5650288966927330432 20260222.1055 12.28CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:11.27 -25:03:40.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.22 09:07:19.50 -26:24:45.8
252.97084 14.03777 galactic Pyx Second-epoch detections are separated by 2.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J136.8424-26.4232 | 09:07:19.88 -26:25:06.0 (Gaia DR3) | CBH (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 J136.8424-26.4232,2461093.6055,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J136.8424-26.4232 20260222.1055 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:19.50 -26:24:45.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.26 09:12:03.72 -26:37:10.9
253.84781 14.70414 galactic Pyx Second-epoch detections are separated by 2.5" 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 5649822086806026112 | 09:12:02.87 -26:37:17.3 (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 5649822086806026112,2461093.6055,12.26,0.05,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 5649822086806026112 20260222.1055 12.26CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:03.72 -26:37:10.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5648131411581274240,2461093.6055,12.18,0.05,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
Gaia DR3 5648131411581274240 20260222.1055 12.18CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:19.59 -28:00:29.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.16 09:11:50.17 -30:05:06.4
256.48309 12.36994 galactic Pyx Second-epoch detections are separated by 1.1" and 4.1 pix
The object was found in VSX 9" ASASSN-V J091150.77-300509.9
Type: SRS
# Max. Min./Amp. JD0 Period
11.710 V 11.840 V 2458134.72200 26.730000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J091150.77-300509.9,2461093.6055,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J091150.77-300509.9 20260222.1055 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:50.17 -30:05:06.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.19 09:09:39.58 -29:31:57.6
255.73923 12.38350 galactic Pyx Second-epoch detections are separated by 6.2" 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 5635766922291500672 | 09:09:38.70 -29:31:42.7 (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 5635766922291500672,2461093.6055,12.19,0.05,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 5635766922291500672 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:39.58 -29:31:57.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.21 09:12:08.25 -27:37:51.8
254.64344 14.04905 galactic Pyx Second-epoch detections are separated by 6.3" 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 5636231951288044416 | 09:12:07.73 -27:38:02.4 (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 5636231951288044416,2461093.6055,12.21,0.05,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 5636231951288044416 20260222.1055 12.21CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:08.25 -27:37:51.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.36 09:07:37.42 -24:33:31.4
251.55439 15.28844 galactic Pyx Second-epoch detections are separated by 6.1" 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 5651119265710529024 | 09:07:36.81 -24:33:38.8 (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 5651119265710529024,2461093.6055,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651119265710529024 20260222.1055 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:37.42 -24:33:31.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.22 09:11:13.28 -29:30:45.7
255.95446 12.65120 galactic Pyx Second-epoch detections are separated by 7.9" and 3.5 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 5635720506583851008 | 09:11:12.47 -29:30:29.9 (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 5635720506583851008,2461093.6055,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635720506583851008 20260222.1055 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:13.28 -29:30:45.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5635221465745557248,2461093.6055,12.20,0.05,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 5635221465745557248 20260222.1055 12.20CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:06.31 -30:45:44.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.34 09:12:05.84 -24:44:52.9
252.38910 15.93866 galactic Pyx Second-epoch detections are separated by 5.8" 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 5650698294492134656 | 09:12:05.31 -24:44:56.3 (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 5650698294492134656,2461093.6055,12.34,0.05,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
Gaia DR3 5650698294492134656 20260222.1055 12.34CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:05.84 -24:44:52.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.29 09:10:05.03 -26:04:16.3
253.11921 14.72964 galactic Pyx Second-epoch detections are separated by 4.2" 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 5650086583774297856 | 09:10:04.48 -26:04:20.6 (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 5650086583774297856,2461093.6055,12.29,0.05,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
Gaia DR3 5650086583774297856 20260222.1055 12.29CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:05.03 -26:04:16.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.16 09:07:33.85 -29:37:44.0
255.50616 11.97739 galactic Pyx Second-epoch detections are separated by 6.1" 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 5635398379738532096 | 09:07:33.06 -29:37:46.1 (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 5635398379738532096,2461093.6055,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635398379738532096 20260222.1055 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:33.85 -29:37:44.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5650000242047725696,2461093.6055,12.28,0.05,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 5650000242047725696 20260222.1055 12.28CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:23.69 -25:56:31.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.49 09:11:12.33 -24:08:18.9
251.77055 16.18218 galactic Hya Second-epoch detections are separated by 0.6" 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 5651486094573296768 | 09:11:11.79 -24:08:22.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.468+/-0.043 (K)
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 5651486094573296768,2461093.6055,12.49,0.05,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 5651486094573296768 20260222.1055 12.49CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:12.33 -24:08:18.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.27 09:11:12.23 -29:30:45.0
255.95172 12.64849 galactic Pyx Second-epoch detections are separated by 5.8" 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 5635720506583851008 | 09:11:12.47 -29:30:29.9 (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 5635720506583851008,2461093.6055,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635720506583851008 20260222.1055 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:12.23 -29:30:45.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.15 09:05:22.89 -29:20:30.3
254.96663 11.80613 galactic Pyx Second-epoch detections are separated by 8.7" and 3.4 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 5635632854889921152 | 09:05:22.41 -29:20:33.1 (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 5635632854889921152,2461093.6055,12.15,0.05,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 5635632854889921152 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:22.89 -29:20:30.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.51 09:10:17.90 -23:54:34.1
251.44908 16.17333 galactic Pyx Second-epoch detections are separated by 1.4" 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 5651540035066381184 | 09:10:17.49 -23:54:37.8 (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 5651540035066381184,2461093.6055,12.51,0.05,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 5651540035066381184 20260222.1055 12.51CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:17.90 -23:54:34.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5636036787974365312,2461093.6055,12.28,0.05,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 5636036787974365312 20260222.1055 12.28CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:49.58 -28:30:36.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.34 09:10:01.18 -24:50:18.5
252.14097 15.52214 galactic Pyx Second-epoch detections are separated by 6.7" and 2.7 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 5651068623752453888 | 09:10:00.52 -24:50:26.2 (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 5651068623752453888,2461093.6055,12.34,0.05,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
Gaia DR3 5651068623752453888 20260222.1055 12.34CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:01.18 -24:50:18.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.28 09:09:27.92 -30:06:00.5
256.14616 11.97658 galactic Pyx Second-epoch detections are separated by 2.9" 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 5635311483958118272 | 09:09:27.45 -30:06:00.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5/7II 1982MSS...C03....0H HD 78858
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 5635311483958118272,2461093.6055,12.28,0.05,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 5635311483958118272 20260222.1055 12.28CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:27.92 -30:06:00.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.45 09:10:19.31 -21:58:44.2
249.91167 17.42268 galactic Pyx Second-epoch detections are separated by 5.6" 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 5655023223479910784 | 09:10:18.87 -21:58:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5655023223479910784,2461093.6055,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655023223479910784 20260222.1055 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:19.31 -21:58:44.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.39 08:17:06.82 -27:27:30.8
246.97737 4.48157 galactic Pup Second-epoch detections are separated by 7.4" and 2.1 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 5693420643434146176 | 08:17:09.25 -27:27:49.3 (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 5693420643434146176,2461093.6055,12.39,0.05,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 5693420643434146176 20260222.1055 12.39CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:17:06.82 -27:27:30.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.54 09:07:22.22 -22:46:02.6
250.08775 16.39369 galactic Pyx Second-epoch detections are separated by 0.5" 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 5654871795816205568 | 09:07:21.86 -22:46:09.7 (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 5654871795816205568,2461093.6055,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5654871795816205568 20260222.1055 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:22.22 -22:46:02.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5635419407897984000,2461093.6055,12.29,0.05,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
Gaia DR3 5635419407897984000 20260222.1055 12.29CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:27.92 -30:29:23.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.29 09:11:58.12 -27:26:51.6
254.47607 14.14222 galactic Pyx Second-epoch detections are separated by 8.8" and 2.8 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 5637738522736572288 | 09:11:57.47 -27:26:50.4 (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 5637738522736572288,2461093.6055,12.29,0.05,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
Gaia DR3 5637738522736572288 20260222.1055 12.29CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:58.12 -27:26:51.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.63 09:06:21.42 -22:39:19.3
249.84251 16.28516 galactic Pyx Second-epoch detections are separated by 3.1" 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 5654891655745193472 | 09:06:20.86 -22:39:27.9 (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 5654891655745193472,2461093.6055,12.63,0.05,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 5654891655745193472 20260222.1055 12.63CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:21.42 -22:39:19.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.43 09:10:47.56 -30:16:05.6
256.46930 12.07976 galactic Pyx Second-epoch detections are separated by 5.7" 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 5634555775872409216 | 09:10:48.12 -30:16:04.4 (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 Lite
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 5634555775872409216,2461093.6055,12.43,0.05,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 5634555775872409216 20260222.1055 12.43CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:47.56 -30:16:05.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.62 09:12:22.29 -23:39:25.7
251.57023 16.69783 galactic Hya Second-epoch detections are separated by 7.0" 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 5651571581602876544 | 09:12:21.81 -23:39:29.2 (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 5651571581602876544,2461093.6055,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651571581602876544 20260222.1055 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:22.29 -23:39:25.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.44 09:12:03.14 -26:38:24.3
253.86220 14.68909 galactic Pyx Second-epoch detections are separated by 2.5" 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 5649820403178513920 | 09:12:01.96 -26:38:21.8 (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 5649820403178513920,2461093.6055,12.44,0.05,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
Gaia DR3 5649820403178513920 20260222.1055 12.44CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:03.14 -26:38:24.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.61 09:10:57.33 -21:23:37.1
249.53966 17.91115 galactic Hya Second-epoch detections are separated by 1.5" 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 5679120944947963520 | 09:10:56.98 -21:23:40.5 (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 5679120944947963520,2461093.6055,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5679120944947963520 20260222.1055 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:57.33 -21:23:37.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.65 09:11:09.45 -24:40:26.0
252.18584 15.82537 galactic Pyx Second-epoch detections are separated by 8.0" 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 5650328411908682624 | 09:11:09.08 -24:40:30.0 (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 5650328411908682624,2461093.6055,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5650328411908682624 20260222.1055 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:09.45 -24:40:26.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.69 09:08:39.76 -22:08:38.5
249.78649 17.02176 galactic Pyx Second-epoch detections are separated by 6.0" 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 5655003604069207552 | 09:08:39.27 -22:08:41.4 (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 5655003604069207552,2461093.6055,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655003604069207552 20260222.1055 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:39.76 -22:08:38.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.44 09:07:08.36 -27:06:43.4
253.49055 13.55192 galactic Pyx Second-epoch detections are separated by 4.4" 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 5648317989260045696 | 09:07:07.61 -27:06:47.4 (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 5648317989260045696,2461093.6055,12.44,0.05,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
Gaia DR3 5648317989260045696 20260222.1055 12.44CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:08.36 -27:06:43.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.43 09:07:49.84 -28:18:59.7
254.53075 12.88195 galactic Pyx Second-epoch detections are separated by 4.2" 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 5636099975533051776 | 09:07:52.67 -28:19:02.2 (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 5636099975533051776,2461093.6055,12.43,0.05,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 5636099975533051776 20260222.1055 12.43CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:49.84 -28:18:59.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.68 09:08:29.08 -21:57:10.8
249.60521 17.11209 galactic Pyx Second-epoch detections are separated by 0.5" 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 5655079019399763328 | 09:08:28.70 -21:57:17.2 (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 5655079019399763328,2461093.6055,12.68,0.05,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 5655079019399763328 20260222.1055 12.68CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:29.08 -21:57:10.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.45 09:10:01.17 -27:05:19.3
253.90346 14.05254 galactic Pyx Second-epoch detections are separated by 5.4" 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 5648282976686743552 | 09:10:00.39 -27:05:23.5 (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 5648282976686743552,2461093.6055,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5648282976686743552 20260222.1055 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:01.17 -27:05:19.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.55 09:10:05.20 -24:20:58.9
251.76519 15.85114 galactic Pyx Second-epoch detections are separated by 4.7" 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 5651101540381604480 | 09:10:04.64 -24:21:04.3 (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 5651101540381604480,2461093.6055,12.55,0.05,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 5651101540381604480 20260222.1055 12.55CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:05.20 -24:20:58.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.39 09:11:08.42 -29:35:09.5
255.99861 12.58937 galactic Pyx Second-epoch detections are separated by 8.5" 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 5635719613230659072 | 09:11:08.14 -29:34:54.4 (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 5635719613230659072,2461093.6055,12.39,0.05,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 5635719613230659072 20260222.1055 12.39CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:08.42 -29:35:09.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.66 09:07:54.05 -22:55:45.2
250.29890 16.38410 galactic Pyx 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 5651866418220637568 | 09:07:53.57 -22:55:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 5651866418220637568,2461093.6055,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651866418220637568 20260222.1055 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:54.05 -22:55:45.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.62 09:11:37.77 -22:49:50.5
250.79758 17.10470 galactic Hya Second-epoch detections are separated by 4.2" and 3.5 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 | ATO J137.9165-22.8394 | 09:11:37.32 -22:49:55.5 (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 J137.9165-22.8394,2461093.6055,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J137.9165-22.8394 20260222.1055 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:37.77 -22:49:50.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.35 09:10:49.09 -30:16:00.4
256.47194 12.08483 galactic Pyx Second-epoch detections are separated by 5.1" 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 5634555775872409216 | 09:10:48.12 -30:16:04.4 (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 Lite
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 5634555775872409216,2461093.6055,12.35,0.05,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
Gaia DR3 5634555775872409216 20260222.1055 12.35CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:49.09 -30:16:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.50 09:08:46.82 -30:00:32.1
255.97605 11.92564 galactic Pyx Second-epoch detections are separated by 1.7" 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 5635327465535185664 | 09:08:45.76 -30:00:38.8 (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 Lite
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 5635327465535185664,2461093.6055,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635327465535185664 20260222.1055 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:46.82 -30:00:32.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.42 09:11:43.52 -24:19:09.7
251.99375 16.15442 galactic Hya Second-epoch detections are separated by 6.8" and 2.8 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 | Large-amplitude variable Gaia DR2 5651468399307053312 | 09:11:42.91 -24:19:18.5 (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 5651468399307053312,2461093.6055,12.42,0.05,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 5651468399307053312 20260222.1055 12.42CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:43.52 -24:19:09.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.65 09:06:52.33 -21:49:37.1
249.25450 16.90394 galactic Pyx Second-epoch detections are separated by 1.7" 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 5655075239828537472 | 09:06:52.21 -21:49:44.1 (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 5655075239828537472,2461093.6055,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655075239828537472 20260222.1055 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:52.33 -21:49:37.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.45 09:10:36.38 -28:34:25.6
255.14147 13.17245 galactic Pyx Second-epoch detections are separated by 2.0" 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 5636024487185501056 | 09:10:35.33 -28:34:25.5 (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 5636024487185501056,2461093.6055,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5636024487185501056 20260222.1055 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:36.38 -28:34:25.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.50 09:08:09.37 -27:26:02.5
253.89319 13.51344 galactic Pyx Second-epoch detections are separated by 1.5" 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 5648249338503140224 | 09:08:08.58 -27:26:09.6 (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 5648249338503140224,2461093.6055,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5648249338503140224 20260222.1055 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:09.37 -27:26:02.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.68 09:09:18.91 -24:40:29.2
251.90400 15.50673 galactic Pyx Second-epoch detections are separated by 0.4" 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 5651086215938357888 | 09:09:18.46 -24:40:35.3 (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 5651086215938357888,2461093.6055,12.68,0.05,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 5651086215938357888 20260222.1055 12.68CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:18.91 -24:40:29.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5651167816020820352,2461093.6055,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651167816020820352 20260222.1055 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:40.28 -24:07:51.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.65 09:09:47.86 -22:42:02.0
250.40872 16.86606 galactic Pyx Second-epoch detections are separated by 8.1" and 2.7 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 5651955792196743936 | 09:09:47.31 -22:42:06.8 (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 5651955792196743936,2461093.6055,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651955792196743936 20260222.1055 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:47.86 -22:42:02.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.60 09:07:49.13 -28:19:05.4
254.53023 12.87894 galactic Pyx Second-epoch detections are separated by 0.5" 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 5636099975533051776 | 09:07:52.67 -28:19:02.2 (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 5636099975533051776,2461093.6055,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5636099975533051776 20260222.1055 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:49.13 -28:19:05.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.40 09:07:34.45 -28:57:26.1
254.98910 12.41977 galactic Pyx Second-epoch detections are separated by 6.0" and 3.0 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 5635996415282061184 | 09:07:34.05 -28:57:31.3 (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 5635996415282061184,2461093.6055,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635996415282061184 20260222.1055 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:34.45 -28:57:26.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.74 09:11:39.06 -23:55:03.8
251.66471 16.40310 galactic Hya Second-epoch detections are separated by 6.4" 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 | Gaia DR3 5651513822882121856 | 09:11:38.31 -23:55:10.4 (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 5651513822882121856,2461093.6055,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651513822882121856 20260222.1055 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:39.06 -23:55:03.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.88 09:06:17.68 -21:25:57.7
248.84672 17.05009 galactic Pyx Second-epoch detections are separated by 3.1" 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 5655308993423820672 | 09:06:17.35 -21:26:04.2 (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 5655308993423820672,2461093.6055,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655308993423820672 20260222.1055 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:17.68 -21:25:57.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.64 09:07:16.37 -25:06:46.5
251.93979 14.87012 galactic Pyx Second-epoch detections are separated by 8.1" and 2.4 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 5650956714084995840 | 09:07:16.09 -25:06:52.1 (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 5650956714084995840,2461093.6055,12.64,0.05,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 5650956714084995840 20260222.1055 12.64CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:16.37 -25:06:46.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.53 09:11:09.47 -29:35:05.7
256.00039 12.59292 galactic Pyx Second-epoch detections are separated by 4.3" and 3.1 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 5635719613230659072 | 09:11:08.14 -29:34:54.4 (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 5635719613230659072,2461093.6055,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635719613230659072 20260222.1055 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:09.47 -29:35:05.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.89 09:06:37.37 -21:35:58.5
249.03235 17.00345 galactic Pyx Second-epoch detections are separated by 2.3" and 3.5 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 5655294150016851456 | 09:06:37.00 -21:36:03.1 (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 5655294150016851456,2461093.6055,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655294150016851456 20260222.1055 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:37.37 -21:35:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.65 09:11:37.95 -24:00:31.1
251.73380 16.34073 galactic Hya Second-epoch detections are separated by 6.2" and 2.7 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 5651511967456260864 | 09:11:37.28 -24:00:39.2 (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 5651511967456260864,2461093.6055,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651511967456260864 20260222.1055 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:37.95 -24:00:31.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.59 09:10:41.65 -29:35:41.6
255.93950 12.51089 galactic Pyx Second-epoch detections are separated by 7.3" 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 5635716795730547328 | 09:10:40.83 -29:35:28.2 (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 5635716795730547328,2461093.6055,12.59,0.05,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 5635716795730547328 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:41.65 -29:35:41.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.66 09:12:02.94 -28:13:49.5
255.09267 13.63752 galactic Pyx 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 5636130040304821504 | 09:12:02.17 -28:13:41.5 (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 5636130040304821504,2461093.6055,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5636130040304821504 20260222.1055 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:02.94 -28:13:49.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.78 09:05:57.65 -21:38:24.9
248.96338 16.85863 galactic Pyx Second-epoch detections are separated by 2.4" 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 5655269823322112128 | 09:05:57.20 -21:38:38.1 (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 5655269823322112128,2461093.6055,12.78,0.05,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 5655269823322112128 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:57.65 -21:38:24.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.62 09:11:22.72 -27:36:11.5
254.50742 13.94129 galactic Pyx Second-epoch detections are separated by 4.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J137.8401-27.6008 | 09:11:22.67 -27:36:22.9 (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 J137.8401-27.6008,2461093.6055,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J137.8401-27.6008 20260222.1055 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:22.72 -27:36:11.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.66 09:09:28.17 -28:04:28.5
254.58638 13.31324 galactic Pyx 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 | ATO J137.3748-28.0747 | 09:09:28.02 -28:04:37.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J137.3748-28.0747,2461093.6055,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J137.3748-28.0747 20260222.1055 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:28.17 -28:04:28.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.71 09:10:21.37 -24:31:04.3
251.93952 15.78860 galactic Pyx Second-epoch detections are separated by 7.4" and 2.6 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 5651084528015036800 | 09:10:20.93 -24:31:05.0 (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 5651084528015036800,2461093.6055,12.71,0.05,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 5651084528015036800 20260222.1055 12.71CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:21.37 -24:31:04.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.62 09:11:46.62 -27:54:12.7
254.79961 13.80901 galactic Pyx Second-epoch detections are separated by 5.9" 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 5636174673604596096 | 09:11:46.54 -27:54:20.4 (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 5636174673604596096,2461093.6055,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5636174673604596096 20260222.1055 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:46.62 -27:54:12.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.72 09:12:29.40 -25:12:25.5
252.81026 15.70530 galactic Pyx Second-epoch detections are separated by 5.4" and 2.9 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 J138.1275-25.2078 | 09:12:28.47 -25:12:35.1 (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 J138.1275-25.2078,2461093.6055,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J138.1275-25.2078 20260222.1055 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:29.40 -25:12:25.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.78 09:08:47.22 -27:46:01.5
254.24621 13.40128 galactic Pyx Second-epoch detections are separated by 3.7" 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 5648221468455133568 | 09:08:46.87 -27:46:09.8 (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 5648221468455133568,2461093.6055,12.78,0.05,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 5648221468455133568 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:47.22 -27:46:01.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.78 09:07:22.24 -22:30:03.1
249.87390 16.56393 galactic Pyx Second-epoch detections are separated by 1.7" 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 | ATO J136.8312-22.5109 | 09:07:21.55 -22:30:11.4 (Gaia DR3) | NSINE (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 J136.8312-22.5109,2461093.6055,12.78,0.05,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
ATO J136.8312-22.5109 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:22.24 -22:30:03.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.86 09:09:26.75 -22:01:53.3
249.81749 17.23320 galactic Pyx Second-epoch detections are separated by 7.9" and 2.6 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 5655029236433991424 | 09:09:26.20 -22:01:59.7 (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 5655029236433991424,2461093.6055,12.86,0.05,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 5655029236433991424 20260222.1055 12.86CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:26.75 -22:01:53.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.69 09:06:48.13 -24:12:21.7
251.14963 15.37214 galactic Pyx Second-epoch detections are separated by 6.8" 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 | ATO J136.7069-24.2049 | 09:06:47.72 -24:12:27.9 (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 J136.7069-24.2049,2461093.6055,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J136.7069-24.2049 20260222.1055 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:48.13 -24:12:21.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.87 09:04:31.61 -21:45:36.3
248.84070 16.52471 galactic Pyx Second-epoch detections are separated by 3.8" 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 5655276557830889856 | 09:04:31.04 -21:45:45.5 (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 5655276557830889856,2461093.6055,12.87,0.05,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 5655276557830889856 20260222.1055 12.87CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:31.61 -21:45:36.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.83 09:11:20.09 -23:26:36.2
251.23946 16.65615 galactic Hya Second-epoch detections are separated by 4.7" 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 5651593258300916224 | 09:11:19.77 -23:26:41.1 (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 5651593258300916224,2461093.6055,12.83,0.05,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 5651593258300916224 20260222.1055 12.83CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:20.09 -23:26:36.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.65 09:07:12.93 -27:57:07.2
254.15665 13.01756 galactic Pyx Second-epoch detections are separated by 6.1" and 3.5 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 5648126773016590720 | 09:07:12.50 -27:57:10.5 (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 5648126773016590720,2461093.6055,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5648126773016590720 20260222.1055 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:12.93 -27:57:07.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5635828842836901504,2461093.6055,12.64,0.05,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 5635828842836901504 20260222.1055 12.64CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:52.58 -28:49:01.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.85 09:12:05.95 -21:30:48.2
249.81589 18.03810 galactic Hya Second-epoch detections are separated by 5.5" 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 5679080297377303808 | 09:12:05.55 -21:30:54.7 (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 5679080297377303808,2461093.6055,12.85,0.05,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 5679080297377303808 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:05.95 -21:30:48.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.79 09:09:21.36 -24:00:03.9
251.37677 15.94991 galactic Pyx Second-epoch detections are separated by 5.0" 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 5651545085947926144 | 09:09:21.00 -24:00:11.9 (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 5651545085947926144,2461093.6055,12.79,0.05,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 5651545085947926144 20260222.1055 12.79CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:21.36 -24:00:03.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5649886167717491840,2461093.6055,12.79,0.05,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 5649886167717491840 20260222.1055 12.79CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:39.59 -26:15:29.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
UNSW-V 404,2461093.6055,12.80,0.05,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
UNSW-V 404 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:03.02 -21:38:46.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.71 09:10:22.11 -29:44:19.0
256.00165 12.36265 galactic Pyx Second-epoch detections are separated by 3.5" 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 5635711092014194304 | 09:10:21.96 -29:44:07.5 (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 5635711092014194304,2461093.6055,12.71,0.05,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 5635711092014194304 20260222.1055 12.71CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:22.11 -29:44:19.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.91 09:07:30.48 -21:16:18.3
248.90377 17.37063 galactic Pyx Second-epoch detections are separated by 7.6" 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 5655318403695513728 | 09:07:30.35 -21:16:24.2 (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 5655318403695513728,2461093.6055,12.91,0.05,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
Gaia DR3 5655318403695513728 20260222.1055 12.91CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:30.48 -21:16:18.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.65 09:11:46.87 -26:49:33.8
253.96555 14.52101 galactic Pyx Second-epoch detections are separated by 7.0" 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 5649782744905317376 | 09:11:46.35 -26:49:36.2 (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 5649782744905317376,2461093.6055,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5649782744905317376 20260222.1055 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:46.87 -26:49:33.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.89 09:12:21.66 -24:01:52.1
251.86457 16.45228 galactic Hya Second-epoch detections are separated by 4.9" 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 | Gaia DR3 5651509596634293376 | 09:12:21.09 -24:02:04.7 (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 5651509596634293376,2461093.6055,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651509596634293376 20260222.1055 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:21.66 -24:01:52.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.91 09:07:21.58 -22:36:33.0
249.95917 16.49285 galactic Pyx Second-epoch detections are separated by 2.7" and 3.5 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 5654882790932692608 | 09:07:20.94 -22:36:41.8 (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 5654882790932692608,2461093.6055,12.91,0.05,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
Gaia DR3 5654882790932692608 20260222.1055 12.91CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:21.58 -22:36:33.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.96 09:07:33.60 -22:45:43.9
250.11272 16.43063 galactic Pyx Second-epoch detections are separated by 2.3" 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 5654877469469683840 | 09:07:33.32 -22:45:51.6 (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 5654877469469683840,2461093.6055,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5654877469469683840 20260222.1055 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:33.60 -22:45:43.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.08 09:11:02.65 -21:29:55.2
249.63822 17.85960 galactic Hya Second-epoch detections are separated by 6.6" 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 5679071737505911040 | 09:11:02.06 -21:29:47.4 (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 5679071737505911040,2461093.6055,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5679071737505911040 20260222.1055 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:02.65 -21:29:55.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.65 09:10:48.31 -30:49:37.3
256.89742 11.70994 galactic Pyx Second-epoch detections are separated by 0.6" 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 | ATO J137.6961-30.8435 | 09:10:47.01 -30:49:52.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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 J137.6961-30.8435,2461093.6055,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J137.6961-30.8435 20260222.1055 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:48.31 -30:49:37.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.90 09:11:21.03 -28:06:10.0
254.88938 13.60662 galactic Pyx Second-epoch detections are separated by 4.4" 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 5636144364016159488 | 09:11:21.13 -28:06:15.9 (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 5636144364016159488,2461093.6055,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5636144364016159488 20260222.1055 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:21.03 -28:06:10.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.90 09:12:23.41 -23:28:38.0
251.43049 16.81819 galactic Hya Second-epoch detections are separated by 1.5" 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 5651670984325373184 | 09:12:22.95 -23:28:49.8 (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 5651670984325373184,2461093.6055,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651670984325373184 20260222.1055 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:23.41 -23:28:38.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.79 09:11:37.16 -28:16:46.5
255.06608 13.53407 galactic Pyx Second-epoch detections are separated by 5.8" and 3.3 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 5636129039574744448 | 09:11:37.03 -28:16:39.0 (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 5636129039574744448,2461093.6055,12.79,0.05,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 5636129039574744448 20260222.1055 12.79CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:37.16 -28:16:46.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.99 09:09:47.56 -22:01:56.6
249.87217 17.29431 galactic Pyx Second-epoch detections are separated by 6.3" and 2.8 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 5655028686678324864 | 09:09:47.06 -22:01:56.0 (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 5655028686678324864,2461093.6055,12.99,0.05,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 5655028686678324864 20260222.1055 12.99CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:47.56 -22:01:56.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.95 09:10:50.50 -21:24:28.2
249.53325 17.88172 galactic Hya Second-epoch detections are separated by 5.5" and 3.5 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 5679120876228346496 | 09:10:50.46 -21:24:39.8 (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 5679120876228346496,2461093.6055,12.95,0.05,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
Gaia DR3 5679120876228346496 20260222.1055 12.95CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:50.50 -21:24:28.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.93 09:10:12.11 -25:33:49.8
252.73949 15.08103 galactic Pyx Second-epoch detections are separated by 6.2" and 3.0 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 5650212001115549184 | 09:10:11.76 -25:33:53.6 (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 5650212001115549184,2461093.6055,12.93,0.05,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 5650212001115549184 20260222.1055 12.93CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:12.11 -25:33:49.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.97 09:08:33.17 -26:17:28.5
253.06005 14.32575 galactic Pyx Second-epoch detections are separated by 5.4" 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 5650061780340014464 | 09:08:32.55 -26:17:31.3 (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 5650061780340014464,2461093.6055,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5650061780340014464 20260222.1055 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:33.17 -26:17:28.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.77 09:06:25.04 -31:06:00.9
256.47159 10.82392 galactic Pyx Second-epoch detections are separated by 2.9" and 4.3 pix
The object was found in VSX10" ASAS J090626-3106.1
Type: MISC
# Max. Min./Amp. JD0 Period
12.370 V Y 0.870 V 2451961.30000 50.260000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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
ASAS J090626-3106.1,2461093.6055,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J090626-3106.1 20260222.1055 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:25.04 -31:06:00.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.96 09:11:17.88 -23:42:55.7
251.44974 16.47318 galactic Hya 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 5651567630232265344 | 09:11:17.22 -23:43:08.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 5651567630232265344,2461093.6055,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651567630232265344 20260222.1055 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:17.88 -23:42:55.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.10 09:05:28.38 -21:27:56.9
248.74720 16.88100 galactic Pyx Second-epoch detections are separated by 2.7" 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 5655288686818472704 | 09:05:27.96 -21:28:07.6 (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 5655288686818472704,2461093.6055,13.10,0.05,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
Gaia DR3 5655288686818472704 20260222.1055 13.10CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:28.38 -21:27:56.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.09 09:06:31.11 -21:49:54.4
249.20394 16.83746 galactic Pyx Second-epoch detections are separated by 2.1" 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 5655075793879414400 | 09:06:30.85 -21:50:03.5 (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 5655075793879414400,2461093.6055,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655075793879414400 20260222.1055 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:31.11 -21:49:54.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.91 09:09:21.84 -30:12:01.2
256.20812 11.89385 galactic Pyx Second-epoch detections are separated by 5.1" and 4.7 pix
The object was found in VSX 6" ASASSN-V J090922.29-301203.5
Type: SR
# Max. Min./Amp. JD0 Period
12.320 V 12.460 V 2457802.00000 466.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J090922.29-301203.5,2461093.6055,12.91,0.05,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
ASASSN-V J090922.29-301203.5 20260222.1055 12.91CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:21.84 -30:12:01.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.02 09:10:27.01 -30:05:26.6
256.28331 12.14234 galactic Pyx Second-epoch detections are separated by 4.5" 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 5635314988651431296 | 09:10:27.45 -30:05:28.9 (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 Lite
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 5635314988651431296,2461093.6055,13.02,0.05,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 5635314988651431296 20260222.1055 13.02CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:27.01 -30:05:26.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.15 09:10:17.71 -24:52:39.5
252.21404 15.54413 galactic Pyx Second-epoch detections are separated by 7.3" and 4.7 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 5650319061762984320 | 09:10:16.96 -24:52:47.3 (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 5650319061762984320,2461093.6055,13.15,0.05,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 5650319061762984320 20260222.1055 13.15CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:17.71 -24:52:39.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
OZ Pup,2461093.6055,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
OZ Pup 20260222.1055 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:21:53.01 -22:58:16.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.88 09:10:36.14 -28:41:34.3
255.23265 13.09309 galactic Pyx Second-epoch detections are separated by 5.7" 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 5636019127069193216 | 09:10:35.76 -28:41:27.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 5636019127069193216,2461093.6055,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5636019127069193216 20260222.1055 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:36.14 -28:41:34.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5696036587752957824,2461093.6055,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5696036587752957824 20260222.1055 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:20:48.01 -25:07:07.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.99 09:09:57.07 -27:27:45.8
254.18391 13.79558 galactic Pyx Second-epoch detections are separated by 3.5" 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 5648256382249732992 | 09:09:56.55 -27:27:50.2 (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 5648256382249732992,2461093.6055,12.99,0.05,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 5648256382249732992 20260222.1055 12.99CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:57.07 -27:27:45.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.11 09:05:06.37 -21:42:27.8
248.88690 16.66213 galactic Pyx Second-epoch detections are separated by 2.7" 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 5655275488382916864 | 09:05:05.90 -21:42:39.3 (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 5655275488382916864,2461093.6055,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655275488382916864 20260222.1055 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:06.37 -21:42:27.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.37 09:10:00.91 -21:37:30.3
249.57907 17.59494 galactic Pyx Second-epoch detections are separated by 6.1" 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 | Large-amplitude variable Gaia DR2 5679110155989689344 | 09:10:00.72 -21:37:36.5 (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 5679110155989689344,2461093.6055,13.37,0.05,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
Large-amplitude variable Gaia DR2 5679110155989689344 20260222.1055 13.37CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:00.91 -21:37:30.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.96 09:11:52.61 -28:46:38.4
255.48770 13.24645 galactic Pyx Second-epoch detections are separated by 1.8" 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 5635920956997609088 | 09:11:52.33 -28:46:32.1 (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 5635920956997609088,2461093.6055,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635920956997609088 20260222.1055 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:52.61 -28:46:38.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.19 09:09:36.88 -30:28:53.4
256.45994 11.74816 galactic Pyx Second-epoch detections are separated by 4.7" and 3.1 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 5634528326740208640 | 09:09:37.35 -30:28:57.2 (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 Lite
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 5634528326740208640,2461093.6055,13.19,0.05,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 5634528326740208640 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:36.88 -30:28:53.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.15 09:07:21.51 -22:23:28.5
249.78395 16.63169 galactic Pyx Second-epoch detections are separated by 1.6" 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 | Large-amplitude variable Gaia DR2 5654995117214033152 | 09:07:21.03 -22:23:41.4 (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 5654995117214033152,2461093.6055,13.15,0.05,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
Large-amplitude variable Gaia DR2 5654995117214033152 20260222.1055 13.15CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:21.51 -22:23:28.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.05 09:12:09.87 -27:10:10.1
254.29024 14.35866 galactic Pyx Second-epoch detections are separated by 3.0" 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 5637757862970132096 | 09:12:09.20 -27:10:13.5 (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 5637757862970132096,2461093.6055,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5637757862970132096 20260222.1055 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:09.87 -27:10:10.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.93 09:11:23.82 -27:14:20.1
254.22791 14.18460 galactic Pyx Second-epoch detections are separated by 5.5" 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 5649765874274039936 | 09:11:20.66 -27:14:23.1 (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 5649765874274039936,2461093.6055,12.93,0.05,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 5649765874274039936 20260222.1055 12.93CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:23.82 -27:14:20.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.17 09:07:05.65 -21:42:02.5
249.18675 17.02395 galactic Pyx Second-epoch detections are separated by 6.5" and 2.8 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 J136.7722-21.7032 | 09:07:05.35 -21:42:11.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J136.7722-21.7032,2461093.6055,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J136.7722-21.7032 20260222.1055 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:05.65 -21:42:02.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.21 09:01:02.88 -30:48:10.4
255.47921 10.14462 galactic Pyx Second-epoch detections are separated by 2.2" and 3.4 pix
The object was found in VSX11" ASASSN-V J090103.60-304815.9
Type: SR
# Max. Min./Amp. JD0 Period
15.190 g Y 0.820 g 2458865.60600 105.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J090103.60-304815.9,2461093.6055,13.21,0.05,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
ASASSN-V J090103.60-304815.9 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:02.88 -30:48:10.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.11 09:10:21.37 -21:19:32.0
249.39080 17.84762 galactic Pyx Second-epoch detections are separated by 6.4" and 3.0 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 5679125991533732736 | 09:10:20.76 -21:19:40.2 (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 5679125991533732736,2461093.6055,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5679125991533732736 20260222.1055 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:21.37 -21:19:32.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.14 09:12:31.33 -30:04:57.4
256.58258 12.48214 galactic Pyx Second-epoch detections are separated by 6.2" 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 5634925834553209600 | 09:12:30.54 -30:04:59.6 (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 Lite
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 5634925834553209600,2461093.6055,13.14,0.05,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 5634925834553209600 20260222.1055 13.14CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:31.33 -30:04:57.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.24 09:07:00.42 -22:30:41.7
249.82663 16.49240 galactic Pyx Second-epoch detections are separated by 8.2" 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 | Large-amplitude variable Gaia DR2 5654898978665174272 | 09:06:59.96 -22:30:44.5 (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 5654898978665174272,2461093.6055,13.24,0.05,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 5654898978665174272 20260222.1055 13.24CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:00.42 -22:30:41.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.13 09:11:27.03 -28:29:50.1
255.20851 13.36211 galactic Pyx Second-epoch detections are separated by 2.1" 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 | ATO J137.8644-28.4964 | 09:11:27.48 -28:29:47.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J137.8644-28.4964,2461093.6055,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J137.8644-28.4964 20260222.1055 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:27.03 -28:29:50.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.22 09:09:10.61 -21:23:31.3
249.26029 17.59393 galactic Pyx Second-epoch detections are separated by 1.1" 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 5679129191284917376 | 09:09:10.37 -21:23:41.9 (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 5679129191284917376,2461093.6055,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5679129191284917376 20260222.1055 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:10.61 -21:23:31.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.29 09:09:57.60 -22:06:02.1
249.95301 17.28031 galactic Pyx Second-epoch detections are separated by 8.6" 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 5655015660041213824 | 09:09:57.30 -22:06:06.9 (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 5655015660041213824,2461093.6055,13.29,0.05,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
Gaia DR3 5655015660041213824 20260222.1055 13.29CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:57.60 -22:06:02.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.27 09:08:38.99 -26:25:39.8
253.18152 14.25334 galactic Pyx Second-epoch detections are separated by 7.4" 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 5650050952725629568 | 09:08:38.74 -26:25:46.4 (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 5650050952725629568,2461093.6055,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5650050952725629568 20260222.1055 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:38.99 -26:25:39.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.34 09:12:09.52 -23:29:24.1
251.40459 16.76954 galactic Hya Second-epoch detections are separated by 3.3" 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 | ATO J138.0380-23.4914 | 09:12:09.13 -23:29:29.1 (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 J138.0380-23.4914,2461093.6055,13.34,0.05,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
ATO J138.0380-23.4914 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:09.52 -23:29:24.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.32 09:12:38.77 -25:43:25.2
253.23865 15.39261 galactic Pyx Second-epoch detections are separated by 4.5" 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 5650010236436322304 | 09:12:38.04 -25:43:27.3 (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 5650010236436322304,2461093.6055,13.32,0.05,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 5650010236436322304 20260222.1055 13.32CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:38.77 -25:43:25.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.35 09:10:58.88 -23:28:10.9
251.20552 16.57737 galactic Hya Second-epoch detections are separated by 2.8" 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 5651591849551644032 | 09:10:58.50 -23:28:15.4 (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 5651591849551644032,2461093.6055,13.35,0.05,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
Gaia DR3 5651591849551644032 20260222.1055 13.35CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:58.88 -23:28:10.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5651931259343678720,2461093.6055,13.43,0.05,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 5651931259343678720 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:59.34 -22:44:00.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.35 09:09:59.19 -27:17:05.0
254.05094 13.91837 galactic Pyx Second-epoch detections are separated by 4.2" and 3.1 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 | ATO J137.4936-27.2859 | 09:09:58.47 -27:17:09.5 (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 J137.4936-27.2859,2461093.6055,13.35,0.05,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 J137.4936-27.2859 20260222.1055 13.35CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:59.19 -27:17:05.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.34 09:12:02.46 -25:51:56.1
253.25673 15.19668 galactic Pyx Second-epoch detections are separated by 1.9" and 3.5 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 5650001852660140672 | 09:12:01.67 -25:52:03.2 (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 5650001852660140672,2461093.6055,13.34,0.05,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
Gaia DR3 5650001852660140672 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:02.46 -25:51:56.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.34 09:09:18.45 -22:42:04.1
250.33326 16.77909 galactic Pyx Second-epoch detections are separated by 6.8" and 3.5 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 5651968054326735232 | 09:09:18.19 -22:42:10.3 (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 5651968054326735232,2461093.6055,13.34,0.05,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
Gaia DR3 5651968054326735232 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:18.45 -22:42:04.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.12 09:05:31.01 -30:47:46.7
256.10906 10.87773 galactic Pyx Second-epoch detections are separated by 3.4" 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 5635163157268240384 | 09:05:31.53 -30:47:51.7 (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 Lite
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 5635163157268240384,2461093.6055,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5635163157268240384 20260222.1055 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:31.01 -30:47:46.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.30 09:09:37.97 -27:11:43.4
253.92834 13.91763 galactic Pyx Second-epoch detections are separated by 3.2" 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 | ATO J137.4028-27.1992 | 09:09:37.16 -27:11:48.4 (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 J137.4028-27.1992,2461093.6055,13.30,0.05,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
ATO J137.4028-27.1992 20260222.1055 13.30CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:37.97 -27:11:43.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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,2461093.6055,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1055 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:44.89 -21:12:30.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.33 09:10:04.50 -26:35:36.7
253.52603 14.38644 galactic Pyx Second-epoch detections are separated by 8.0" and 3.3 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 | ATO J137.5123-26.5933 | 09:10:04.09 -26:35:39.1 (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 J137.5123-26.5933,2461093.6055,13.33,0.05,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 J137.5123-26.5933 20260222.1055 13.33CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:04.50 -26:35:36.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.51 09:05:20.01 -21:17:41.9
248.58725 16.96360 galactic Pyx Second-epoch detections are separated by 5.7" 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 5655361490808027904 | 09:05:19.62 -21:17:51.0 (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 5655361490808027904,2461093.6055,13.51,0.05,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 5655361490808027904 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:20.01 -21:17:41.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.54 09:04:56.03 -21:51:33.7
248.98322 16.53534 galactic Pyx Second-epoch detections are separated by 6.1" 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 5655272091064900096 | 09:04:55.54 -21:51:40.0 (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 5655272091064900096,2461093.6055,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655272091064900096 20260222.1055 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:56.03 -21:51:33.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.53 09:10:28.42 -22:39:58.6
250.48626 17.00743 galactic Pyx Second-epoch detections are separated by 3.6" 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 5651961079299844736 | 09:10:27.94 -22:40:05.1 (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 5651961079299844736,2461093.6055,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651961079299844736 20260222.1055 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:28.42 -22:39:58.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.68 09:08:15.82 -21:12:21.0
248.96762 17.54851 galactic Pyx Second-epoch detections are separated by 5.8" 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 5679325965210143104 | 09:08:15.44 -21:12:25.5 (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 5679325965210143104,2461093.6055,13.68,0.05,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 5679325965210143104 20260222.1055 13.68CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:15.82 -21:12:21.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.42 09:08:06.35 -30:38:10.8
256.35916 11.40214 galactic Pyx Second-epoch detections are separated by 4.1" 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 5635177279121304448 | 09:08:06.84 -30:38:15.0 (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 Lite
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 5635177279121304448,2461093.6055,13.42,0.05,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 5635177279121304448 20260222.1055 13.42CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:06.35 -30:38:10.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.28 09:09:03.28 -29:34:55.9
255.68837 12.25199 galactic Pyx Second-epoch detections are separated by 8.3" 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 5635391954465326720 | 09:09:03.70 -29:34:44.0 (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 5635391954465326720,2461093.6055,13.28,0.05,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 5635391954465326720 20260222.1055 13.28CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:03.28 -29:34:55.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5655107370478926848,2461093.6055,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655107370478926848 20260222.1055 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:08:50.43 -21:34:53.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.59 09:11:27.87 -23:21:17.5
251.18925 16.73621 galactic Hya Second-epoch detections are separated by 5.5" 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 5651688022459144704 | 09:11:27.41 -23:21:25.9 (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 5651688022459144704,2461093.6055,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651688022459144704 20260222.1055 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:27.87 -23:21:17.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.38 09:10:58.71 -29:37:13.0
256.00097 12.54029 galactic Pyx Second-epoch detections are separated by 6.9" 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 | Large-amplitude variable Gaia DR2 5635713565915127808 | 09:10:58.87 -29:37:01.1 (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 5635713565915127808,2461093.6055,13.38,0.05,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
Large-amplitude variable Gaia DR2 5635713565915127808 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:58.71 -29:37:13.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.74 09:12:11.65 -21:28:49.3
249.80427 18.07628 galactic Hya Second-epoch detections are separated by 4.1" 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 5679092490787909120 | 09:12:11.09 -21:28:53.3 (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 5679092490787909120,2461093.6055,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5679092490787909120 20260222.1055 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:11.65 -21:28:49.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.30 09:10:26.21 -30:54:21.1
256.90377 11.59848 galactic Pyx Second-epoch detections are separated by 2.4" 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 5634451528428120192 | 09:10:26.88 -30:54:27.1 (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 Lite
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 5634451528428120192,2461093.6055,13.30,0.05,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 5634451528428120192 20260222.1055 13.30CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:26.21 -30:54:21.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.59 09:11:24.85 -22:38:56.8
250.61904 17.18426 galactic Hya Second-epoch detections are separated by 4.3" 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 | ATO J137.8539-22.6512 | 09:11:24.20 -22:39:01.5 (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 J137.8539-22.6512,2461093.6055,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J137.8539-22.6512 20260222.1055 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:24.85 -22:38:56.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.70 09:10:26.55 -22:48:42.1
250.59763 16.90819 galactic Pyx Second-epoch detections are separated by 8.2" 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 5651950363358291968 | 09:10:26.21 -22:48:47.7 (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 5651950363358291968,2461093.6055,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651950363358291968 20260222.1055 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:26.55 -22:48:42.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.71 09:10:07.04 -21:36:06.3
249.57622 17.62812 galactic Pyx Second-epoch detections are separated by 4.6" 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 5679111766602057728 | 09:10:06.61 -21:36:08.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 5679111766602057728,2461093.6055,13.71,0.05,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 5679111766602057728 20260222.1055 13.71CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:07.04 -21:36:06.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.88 09:11:02.03 -21:21:29.4
249.52334 17.94789 galactic Hya Second-epoch detections are separated by 3.6" 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 5679121529063362688 | 09:11:01.63 -21:21:34.0 (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 5679121529063362688,2461093.6055,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5679121529063362688 20260222.1055 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:02.03 -21:21:29.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.88 09:10:47.80 -22:39:12.6
250.52629 17.07263 galactic Hya Second-epoch detections are separated by 7.9" 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 5651959498751879040 | 09:10:47.17 -22:39:21.9 (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 5651959498751879040,2461093.6055,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651959498751879040 20260222.1055 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:47.80 -22:39:12.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.87 09:11:12.34 -21:43:32.2
249.84623 17.74259 galactic Hya Second-epoch detections are separated by 3.2" 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 5679047857487752704 | 09:11:11.94 -21:43:36.3 (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 5679047857487752704,2461093.6055,13.87,0.05,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 5679047857487752704 20260222.1055 13.87CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:12.34 -21:43:32.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.61 09:12:35.14 -26:10:33.3
253.58227 15.08472 galactic Pyx Second-epoch detections are separated by 8.8" 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 5649978178800456192 | 09:12:34.06 -26:10:39.2 (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 5649978178800456192,2461093.6055,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5649978178800456192 20260222.1055 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:35.14 -26:10:33.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.73 09:12:20.94 -24:57:10.7
252.58908 15.84772 galactic Pyx Second-epoch detections are separated by 3.8" 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 5650305390884182272 | 09:12:20.42 -24:56:59.6 (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 5650305390884182272,2461093.6055,13.73,0.05,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 5650305390884182272 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:20.94 -24:57:10.7 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 13.80 09:11:05.09 -23:33:12.0
251.28802 16.54123 galactic Hya Second-epoch detections are separated by 3.2" 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 5651588035620687488 | 09:11:04.55 -23:33:22.7 (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 5651588035620687488,2461093.6055,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651588035620687488 20260222.1055 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:05.09 -23:33:12.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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,2461093.6055,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1055 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:18.84 -21:57:08.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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,2461093.6055,13.87,0.05,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 20260222.1055 13.87CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:24.68 -21:24:20.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.60 09:05:51.54 -24:34:34.6
251.30108 14.96985 galactic Pyx Second-epoch detections are separated by 2.8" 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 5651126726069824640 | 09:05:51.08 -24:34:40.3 (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 5651126726069824640,2461093.6055,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5651126726069824640 20260222.1055 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:51.54 -24:34:34.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.60 08:34:29.42 -30:43:12.5
251.84585 5.71694 galactic Pyx Second-epoch detections are separated by 0.4" and 3.4 pix
The object was found in VSX 3" ASAS J083429-3043.3
Type: MISC
# Max. Min./Amp. JD0 Period
9.043 Ic Y 0.476 Ic 2452932.50000 246.700000000000 M8
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
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
ASAS J083429-3043.3,2461093.6055,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J083429-3043.3 20260222.1055 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:34:29.42 -30:43:12.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J082008.93-255105.8,2461093.6055,11.77,0.05,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
ASASSN-V J082008.93-255105.8 20260222.1055 11.77CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:20:08.99 -25:51:06.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J083203.80-245117.6,2461093.6055,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J083203.80-245117.6 20260222.1055 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:32:03.72 -24:51:17.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J084857.57-241225.6,2461093.6055,12.15,0.05,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
ASASSN-V J084857.57-241225.6 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:57.46 -24:12:27.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASAS J083539-2518.8,2461093.6055,11.80,0.05,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
ASAS J083539-2518.8 20260222.1055 11.80CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:35:39.23 -25:18:49.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 11.82 08:29:22.63 -30:36:43.9
251.10941 4.89057 galactic Pyx Second-epoch detections are separated by 0.7" and 3.3 pix
The object was found in VSX 3" ASASSN-V J082922.53-303646.4
Type: SR
# Max. Min./Amp. JD0 Period
13.180 V 14.600 V 2457438.70000 192.000000000000
The object was not found in astcheck.
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J082922.53-303646.4,2461093.6055,11.82,0.05,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
ASASSN-V J082922.53-303646.4 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:29:22.63 -30:36:43.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J085136.56-291115.2,2461093.6055,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J085136.56-291115.2 20260222.1055 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:51:36.33 -29:11:13.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
BC Pyx,2461093.6055,10.68,0.05,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
BC Pyx 20260222.1055 10.68CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:35:26.51 -27:16:12.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.71 08:28:13.68 -27:18:33.3
248.25742 6.59963 galactic Pyx Second-epoch detections are separated by 0.8" and 3.5 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 | ATO J127.0686-27.3100 | 08:28:13.68 -27:18:33.3 (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 J127.0686-27.3100,2461093.6055,12.71,0.05,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 J127.0686-27.3100 20260222.1055 12.71CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:28:13.68 -27:18:33.3 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.43 09:04:07.07 -21:16:19.1
248.38233 16.75801 galactic Pyx Second-epoch detections are separated by 2.2" 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 5655353180047254016 | 09:04:06.46 -21:16:19.6 (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 5655353180047254016,2461093.6055,12.43,0.05,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 5655353180047254016 20260222.1055 12.43CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:07.07 -21:16:19.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J084132.58-245741.0,2461093.6055,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J084132.58-245741.0 20260222.1055 11.79CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:41:32.52 -24:57:41.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 3995,2461093.6055,11.49,0.05,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
NSV 3995 20260222.1055 11.49CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:17:49.58 -26:00:48.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J082542.99-291546.0,2461093.6055,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J082542.99-291546.0 20260222.1055 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:25:43.23 -29:15:44.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J083722.53-242917.7,2461093.6055,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J083722.53-242917.7 20260222.1055 11.87CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:37:22.53 -24:29:20.0 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 4112,2461093.6055,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 4112 20260222.1055 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:14.43 -25:18:28.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASAS J083559-2431.7,2461093.6055,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J083559-2431.7 20260222.1055 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:35:58.85 -24:31:44.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J083054.40-264659.3,2461093.6055,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J083054.40-264659.3 20260222.1055 12.06CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:30:54.36 -26:46:59.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
IX Pup,2461093.6055,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IX Pup 20260222.1055 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:19:04.78 -24:02:11.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
CP Pyx,2461093.6055,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CP Pyx 20260222.1055 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:52:42.62 -25:14:45.8 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASAS J083204-2853.5,2461093.6055,11.81,0.05,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
ASAS J083204-2853.5 20260222.1055 11.81CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:32:04.46 -28:53:28.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J083154.28-274428.3,2461093.6055,12.59,0.05,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
ASASSN-V J083154.28-274428.3 20260222.1055 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:31:54.30 -27:44:27.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASAS J082916-2236.1,2461093.6055,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J082916-2236.1 20260222.1055 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:29:15.53 -22:36:10.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J082915.95-275637.4,2461093.6055,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J082915.95-275637.4 20260222.1055 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:29:15.97 -27:56:36.9 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASAS J081133-2619.1,2461093.6055,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J081133-2619.1 20260222.1055 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:33.44 -26:19:02.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASASSN-V J083943.16-264048.6,2461093.6055,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J083943.16-264048.6 20260222.1055 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:39:42.97 -26:40:47.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
FL Pup,2461093.6055,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FL Pup 20260222.1055 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:10:21.18 -23:00:47.6 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
SU Pyx,2461093.6055,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SU Pyx 20260222.1055 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:32:00.66 -27:15:32.4 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 4011,2461093.6055,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 4011 20260222.1055 10.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:20:07.68 -26:16:33.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
CC Pyx,2461093.6055,12.64,0.05,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
CC Pyx 20260222.1055 12.64CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:27.92 -22:13:13.1 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1055 2461093.6055 12.22 08:34:38.18 -26:48:42.5
248.68661 8.04934 galactic Pyx Second-epoch detections are separated by 1.0" and 3.4 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 5646662674513047552 | 08:34:38.42 -26:48:37.8 (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 5646662674513047552,2461093.6055,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5646662674513047552 20260222.1055 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:34:38.18 -26:48:42.5 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_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
ASAS J083759-2942.5,2461093.6055,11.52,0.05,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
ASAS J083759-2942.5 20260222.1055 11.52CV 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:37:58.80 -29:42:27.2 ;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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20_00sec_-14_90C_LIGHT_0015_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20_00sec_-15_00C_LIGHT_0265_fits__*pix.png resample_wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20_00sec_-14_90C_LIGHT_0014_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.76722969 09.01.2026 06:24:38.645 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
First image: 2461049.76722969 09.01.2026 06:24:38.645 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
Last image: 2461093.60575837 22.02.2026 02:32:07.523 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 185
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.36
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15777
Objects passed selection criteria: 15752
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 13811.2
Average stars matched: 13379 (96.8703 %)
Memory usage VmPeak: 120432 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 Sat Feb 21 23:52:49 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: 2461049.76722969 09.01.2026 06:24:38.645 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
First image: 2461049.76722969 09.01.2026 06:24:38.645 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
Last image: 2461093.60575837 22.02.2026 02:32:07.523 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1113
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.05
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: 208 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): 134901
Objects passed selection criteria: 134669
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 113819
Average stars matched: 109714 (96.3936 %)
Memory usage VmPeak: 1904552 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 Sat Feb 21 23:59:21 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:
Pyx-01-Q2b1x1
#######################################
########### Starting Pyx-01-Q2b1x1 ###########
Processing Pyx-01-Q2b1x1
server tau has sufficient free disk space available: 1098978 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1098978 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.png' -> 'transient_report/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits_preview.png'
Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
renamed 'Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.png' -> 'transient_report/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits_preview.png'
Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.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= 2372.3973
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 815.6578
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 3550.7095
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 1055.4063
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 3536.9937
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 1053.1055
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.49668
INFO: SECOND_EPOCH__SD_ratio= 0.002
----------------------------------------------
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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat to cache
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.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: 2461093.60520073
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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits exists and is non-empty
Saving wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits to local_wcs_cache/
'wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits' -> 'local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits'
wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits exists and is non-empty
Saving wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits to local_wcs_cache/
'wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits' -> 'local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits'
wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits exists and is non-empty
Saving wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits to local_wcs_cache/
'wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits' -> 'local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits'
wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits exists and is non-empty
Saving wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits to local_wcs_cache/
'wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits' -> 'local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.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 08:38:19.346 -26:00:33.84
Second-epoch image center 08:38:24.953 -26:00:04.51
Angular distance between the image centers 0.02 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 08:38:19.346 -26:00:33.84
Second-epoch image center 08:38:23.628 -25:59:53.48
Angular distance between the image centers 0.02 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 08:38:24.953 -26:00:04.51
Second-epoch second image center 08:38:23.628 -25:59:53.48
Angular distance between the image centers 0.00583 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits &> /tmp/tmp.UGKBrF06Ze
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits &> /tmp/tmp.frQpQ9aIoh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits &> /tmp/tmp.yx7irTwHgw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits &> /tmp/tmp.jQNY6YdXcF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
Calibrating the magnitude scale
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits and wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits and wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits and wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat
The reference image (wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits) and catalog (wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat) found
'wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.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 12391 out of 15978 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.802624
a=0.000000 b=1.000000 c=22.802624
From vast_summary.log: estimated ref. image limiting mag.: -8.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.44
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 169 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
2.1 pix Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
2.9 pix Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
2.9 pix Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
Limiting magnitude estimates:
14.4 mag. Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
14.4 mag. Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
13.8 mag. Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
13.9 mag. Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.3 (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.UGKBrF06Ze (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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1310, passed=15978
Got 15978 stars (including 14643 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat
util/solve_plate_with_UCAC5 got 15978 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 945 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: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits -region wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.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.frQpQ9aIoh (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/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1287, passed=16203
Got 16203 stars (including 14894 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat
util/solve_plate_with_UCAC5 got 16203 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 945 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 - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits -region wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.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.yx7irTwHgw (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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=946, passed=11640
Got 11640 stars (including 10692 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 11640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 930 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: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.76"
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits -region wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.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.jQNY6YdXcF (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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=987, passed=11734
Got 11734 stars (including 10742 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 11734 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 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: 0.79"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 924 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits -region wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.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 Pyx-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__out21148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out01791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21423.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 42s
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: 13s
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Considering the candidate 21146_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21146_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:48.62 -26:47:06.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21148_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21148_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:03.61 -28:36:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 0.140 5636033111482437376 137.26508563902 -28.60382922606 9.5612 9.0927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21149_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21149_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:13.16 -26:31:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 4.215 5649852941850830976 137.55611822642 -26.52322146088 9.5232 9.0702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21150_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21150_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21151_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21151_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:57.22 -29:46:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.42, MAG_FAINT_SEARCH_LIMIT=11.40)GAIADR2_OUTPUT=# 2.100 5635478369207335168 135.98790363370 -29.76912314326 9.1371 8.8272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21152_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21152_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:17:13.04 -24:06:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 3.091 5696347027988988672 124.30480131951 -24.11018910114 10.7689 9.9908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21154_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21154_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21155_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21155_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:56.89 -30:21:59.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21156_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21156_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:23.45 -23:10:31.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21160_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21160_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 21161_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21161_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:29.19 -26:17:12.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21162_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21162_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:26.39 -25:35:57.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21170_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21170_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:03.01 -21:25:02.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21174_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21174_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21176_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21176_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 21180_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21180_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:02.51 -28:57:18.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21186_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21186_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:57.67 -21:31:53.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21188_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21188_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:36.74 -30:32:46.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21190_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21190_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:52.39 -23:19:33.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21192_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21192_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:27.95 -23:31:09.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21195_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21195_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21198_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21198_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:17.82 -30:09:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.99, MAG_FAINT_SEARCH_LIMIT=10.97)GAIADR2_OUTPUT=# 2.894 5635310869779062400 137.32517270797 -30.16087692477 8.4540 7.4989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21208_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21208_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:15.72 -30:16:32.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21211_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21211_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21212_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21212_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21213_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21213_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:04.13 -27:01:45.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21215_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21215_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:53.10 -21:44:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.45, MAG_FAINT_SEARCH_LIMIT=11.43)GAIADR2_OUTPUT=# 4.602 5679059333640368256 137.72001330709 -21.73667166284 9.1852 8.7507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21216_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21216_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:36.70 -28:29:07.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21217_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21217_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:06.26 -27:26:25.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21218_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21218_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:06.38 -22:03:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.43, MAG_FAINT_SEARCH_LIMIT=11.41)GAIADR2_OUTPUT=# 3.033 5655054589624917632 137.02573881150 -22.06508978800 9.7355 9.6355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21223_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21223_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:43.50 -21:58:51.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21232_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21232_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21236_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21236_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:12.66 -28:48:58.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21239_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21239_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:40.80 -30:16:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.57, MAG_FAINT_SEARCH_LIMIT=11.55)GAIADR2_OUTPUT=# 2.535 5635306162497692928 137.42073176668 -30.27146709323 9.0178 8.2040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21240_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21240_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:22.56 -31:08:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.56, MAG_FAINT_SEARCH_LIMIT=11.54)GAIADR2_OUTPUT=# 1.354 5629146148606101248 136.09414741951 -31.13874331608 9.1546 8.4247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21241_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21241_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:35:26.51 -27:16:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.65, MAG_FAINT_SEARCH_LIMIT=11.63)GAIADR2_OUTPUT=# 0.843 5646585227661438848 128.86040649346 -27.26977035222 10.1270 8.7668 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21244_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21244_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:27.86 -21:14:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 4.968 5679322666675260928 137.11489721681 -21.25077061476 10.0051 9.8121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21247_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21247_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21249_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21249_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:14.46 -30:16:31.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 21253_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21253_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:48.56 -21:42:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 3.381 5655090293689021440 137.45139340845 -21.70340100121 9.6480 9.2802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21255_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21255_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 21256_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21256_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21263_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21263_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 21265_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21265_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:14.46 -29:55:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 3.708 5634942803967328384 138.06137999576 -29.92367984433 9.1699 8.2170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21266_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21266_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:27.68 -31:10:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 1.554 5635134501246615552 136.36552174421 -31.17948383383 9.3024 8.5470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21267_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21267_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 21269_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21269_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21271_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21271_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:45.25 -31:00:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 2.009 5634405112722588672 137.18866280493 -31.00754820996 9.2083 8.5236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21272_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21272_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:16.13 -23:52:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 2.729 5651514677579463936 138.06638993238 -23.88195451708 9.6762 9.2144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21273_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21273_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:12.28 -30:58:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 5.169 5634406384032877952 137.30249579603 -30.96762332286 9.1890 8.2375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21277_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21277_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21278_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21278_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 21279_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21279_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:39.13 -21:19:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 3.737 5679098404959417216 137.91355429758 -21.32743951426 9.8136 9.0372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21281_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21281_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:00.67 -27:15:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 0.551 5646622714136881152 128.00295593855 -27.25914831557 11.0791 10.8081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21283_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21283_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 21284_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21284_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21285_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21285_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21286_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21286_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:30.23 -30:18:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 3.956 5635296301252850304 137.12718753414 -30.30989636776 9.4473 8.4453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21287_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21287_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21290_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21290_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:36.10 -27:45:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 4.122 5636223601868907520 137.89915134518 -27.76521142615 9.6845 9.4074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21291_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21291_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:28:17.08 -25:06:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 0.126 5695288507527132544 127.07118766775 -25.11275150429 11.0838 10.4053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21296_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21296_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:31.14 -30:43:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 2.044 5635178035035603584 136.88007886830 -30.72138141998 9.5092 8.7574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21298_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21298_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:43.13 -23:32:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 0.914 5701864274251159296 128.42977034750 -23.54669189378 11.4572 10.8286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21299_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21299_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21302_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21302_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21304_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21304_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:10.25 -31:06:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 3.364 5634410094884714624 137.04162075717 -31.10224267950 9.3544 9.0577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21306_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21306_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:35.60 -22:32:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 4.066 5651964412194460800 137.64731983274 -22.54857650180 10.1344 9.7827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21308_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21308_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:24:55.38 -23:42:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 1.407 5696594860478349184 126.23093375391 -23.70865844138 11.4639 11.3334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21309_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21309_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:09.47 -30:46:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 0.645 5635183326435451264 136.53930061617 -30.77664511432 9.6029 8.9726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21316_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21316_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:45.99 -21:29:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 3.945 5679093010480673024 137.94194484548 -21.49677867980 9.8416 9.1330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21318_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21318_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:29:24.17 -26:38:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 0.594 5646903020875945088 127.35086792605 -26.64619461138 11.0715 10.1883 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21322_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21322_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:42:25.82 -26:58:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 1.073 5646266983458136064 130.60783774147 -26.96738985410 10.4746 9.1107 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21323_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21323_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:39:41.15 -25:37:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 1.160 5647218443271678208 129.92111659986 -25.62542732110 11.2237 10.5388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21324_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21324_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:36:19.69 -23:36:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 0.176 5701686222086026624 129.08207501011 -23.61637158272 11.3532 10.9846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21326_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21326_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:36:22.77 -26:29:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 0.756 5647050217998866304 129.09497594293 -26.49703268344 11.0283 10.1185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21332_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21332_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:56.92 -24:54:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 0.400 5695496864981285760 127.98724373717 -24.90586415024 11.2587 10.4739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21334_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21334_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21337_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21337_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:26.45 -30:59:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 2.462 5634414011894760960 136.85943106308 -30.99395741509 9.4129 8.9251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21338_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21338_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:23:36.23 -26:08:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 0.818 5695112894904615680 125.90087886904 -26.14645105336 10.7662 9.6018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21339_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21339_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:24:50.42 -23:11:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 1.170 5696835692185263488 126.21026376551 -23.18530737935 11.3776 11.0118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21340_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21340_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21341_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21341_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:24:09.93 -29:21:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 1.655 5644788900540250112 126.04088382142 -29.36286195978 10.5848 9.3325 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21343_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21343_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:38:18.82 -24:59:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.207 5647489369808259072 129.57842672125 -24.99144630663 11.4001 11.2355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21345_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21345_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:56.74 -25:43:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 0.827 5647356088390279936 128.48650691672 -25.72029805772 11.3783 10.9559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21346_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21346_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:34.88 -26:02:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 0.703 5647307160116642944 128.39534828788 -26.04627739396 11.1976 10.4916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21347_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21347_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:40:30.59 -26:04:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 0.486 5647121922468695680 130.12757920782 -26.08058001936 11.2729 10.5991 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 21349_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21349_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:59.59 -24:37:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 0.398 5695599188276792064 127.99839746918 -24.62005666407 11.1816 10.3360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21350_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21350_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:26.89 -25:06:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 1.124 5647485418438470144 129.36211469722 -25.10475038425 10.5191 9.1868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21351_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21351_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:40:33.10 -25:22:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 1.990 5647230950216334336 130.13787820523 -25.37641268547 11.3738 10.6866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21352_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21352_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:52:42.61 -25:14:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 3.508 5652672428964447360 133.17842568677 -25.24563749019 12.1207 10.2098 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21353_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21353_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:11.78 -25:58:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 0.188 5647279088214638464 129.29908191028 -25.97103111769 11.0410 10.0382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21354_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21354_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:25:32.82 -26:16:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 0.519 5694928520554029824 126.38689208639 -26.27676186542 11.2518 10.5467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21356_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21356_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:19.42 -25:21:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 1.173 5695444706897933440 127.83079138946 -25.36619452148 11.5306 11.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21357_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21357_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21358_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21358_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:01.00 -25:41:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 0.914 5695383580921948928 127.75398579532 -25.69824988479 11.1182 10.1396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21359_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21359_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:51.78 -24:52:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 1.146 5695532461665066368 128.71601059862 -24.88240749862 11.4033 10.7593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21360_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21360_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 21361_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21361_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:36:13.15 -25:37:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 1.512 5647396357996925056 129.05497560956 -25.62594156833 11.6190 11.4810 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 21362_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21362_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:22.19 -25:39:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 0.465 5694636939510248192 123.34232229751 -25.66507086284 11.0751 10.2707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21363_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21363_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:38:42.16 -26:41:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 1.217 5646994280337585792 129.67594035761 -26.68634448183 11.3989 11.3011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21368_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21368_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:26.16 -27:27:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.33, MAG_FAINT_SEARCH_LIMIT=12.31)GAIADR2_OUTPUT=# 0.683 5645821376317840000 129.35898972583 -27.46008833004 10.8283 9.5422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21369_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21369_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:24:47.36 -26:38:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 0.153 5694880824930013952 126.19730374728 -26.63492216386 11.3795 10.6971 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#
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Considering the candidate 21370_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21370_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:35:40.62 -25:12:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 0.495 5647468479087670912 128.91921950531 -25.20263477639 11.3690 10.6376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21371_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21371_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:29:27.20 -25:40:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 0.620 5695061252221830272 127.36351942835 -25.67156689735 11.3920 10.7475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21373_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21373_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:56.01 -21:24:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 2.428 5679132107567165056 137.23274192239 -21.40663349055 10.3505 9.8845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21374_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21374_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:36:14.62 -25:19:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 0.888 5647451986413230720 129.06109914434 -25.32437772421 11.3604 10.7094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21376_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21376_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:28.73 -26:54:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 1.209 5646825917627699584 128.12005733075 -26.90909844409 11.4301 11.0147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21377_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21377_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:15.22 -24:55:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 1.746 5695527135905674496 128.56363353411 -24.92272111675 11.5227 10.9017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21379_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21379_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:17:19.21 -26:55:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 2.508 5693521244440609664 124.32926167429 -26.91810062435 10.5326 9.1533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21380_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21380_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:40.30 -24:55:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 1.546 5695485766785723648 128.16819630263 -24.92842982054 11.4595 10.9656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21381_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21381_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:58.54 -25:43:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 0.481 5647335472546163584 128.24392100159 -25.72797761685 11.0441 9.9872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21382_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21382_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:26:44.89 -26:44:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 1.433 5694832141485184768 126.68735464787 -26.73608893392 11.5336 11.4565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21386_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21386_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:28:57.86 -27:49:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 4.475 5646671504953671424 127.24012330750 -27.82420308766 11.0389 9.9456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21389_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21389_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:28:20.20 -27:17:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 0.439 5646753796531678080 127.08405165220 -27.28473313937 11.3564 10.6849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21390_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21390_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:30:09.08 -26:22:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 0.941 5646913569321921408 127.53803604197 -26.36879902087 11.5144 11.3550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21391_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21391_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:25.51 -25:13:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.738 5695448074152038144 127.85648760411 -25.22784142230 11.1968 10.2046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21394_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21394_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:28:15.86 -26:21:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 0.682 5694961299740212480 127.06625616516 -26.36230352929 11.4833 11.0734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21398_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21398_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:29:26.40 -23:53:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 0.516 5695882896636621440 127.36013129919 -23.89166154337 11.4674 10.8290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21399_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21399_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:29:24.17 -25:47:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 0.412 5695050738141920128 127.35082074168 -25.78616470652 11.3931 10.7154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21400_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21400_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:36:13.36 -25:12:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 1.157 5647470575031655552 129.05582571106 -25.21537077876 11.4304 10.7418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21405_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21405_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:35:05.55 -24:38:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 0.655 5695563041831776512 128.77332467392 -24.64312760793 11.2622 10.3623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21407_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21407_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:39.74 -25:03:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.518 5695430546382228480 128.41570125482 -25.05126312715 11.3123 10.4382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21409_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21409_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:25:47.86 -25:02:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 2.023 5695347846796799872 126.44972984806 -25.03384600518 11.5705 11.5106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21410_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21410_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:29:47.06 -25:43:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 1.536 5695057266492162048 127.44630043263 -25.71937903931 11.6127 11.4285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21411_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21411_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:18:18.21 -26:19:08.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)
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Considering the candidate 21412_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21412_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:27:27.19 -24:33:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 1.334 5695744117657636992 126.86353983204 -24.55332161696 11.4506 11.0201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21413_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21413_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:24:53.11 -25:38:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.679 5695153473756400256 126.22147588277 -25.64292278217 11.4176 10.7700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21414_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21414_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:30:17.22 -24:44:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 1.109 5695689038996647040 127.57173556518 -24.74330320893 10.4093 8.9890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21416_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21416_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:29:28.06 -25:59:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.103 5694999782647793920 127.36689898430 -25.99536513737 11.2758 10.4069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21417_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21417_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21419_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21419_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:30:54.49 -27:54:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 1.252 5646473489792230656 127.72737115599 -27.90757888694 11.4571 11.2734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21423_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 21423_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 21425_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21425_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:40.24 -25:15:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 1.067 5695424194127890304 128.16787624137 -25.25142232475 11.6050 11.0881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21426_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21426_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:29:10.45 -24:53:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 0.457 5695673164790074112 127.29365841855 -24.89132011681 11.4767 10.7869 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#
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Considering the candidate 21427_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21427_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:35:43.17 -25:16:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 0.220 5647465008754117632 128.92981284746 -25.27689245346 11.6504 11.1137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21428_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21428_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:28.72 -25:16:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.687 5695414573400964736 128.36976877834 -25.27286134538 11.4099 10.6801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21432_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21432_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:13.29 -24:54:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 0.810 5695527204625151872 128.55552594731 -24.91445632317 11.6761 11.2354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21433_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21433_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:31.65 -23:53:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 1.120 5695870424051447680 127.88198774278 -23.90007134956 11.6952 11.4862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21434_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21434_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:17:49.57 -26:00:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 1.780 5694414155266798208 124.45609522396 -26.01329456421 10.6213 9.2580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21435_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21435_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:21:41.87 -27:10:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.361 5693354810175882880 125.42443413332 -27.17417993938 11.0586 10.0731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21436_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21436_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:14.29 -25:27:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.862 5647370038443895936 128.55963618750 -25.45570457748 12.1041 11.5437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21441_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21441_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:20:00.26 -24:27:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 0.365 5696355721000529792 125.00105506092 -24.45476460364 11.4378 10.7221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21443_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21443_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:40.02 -27:00:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 0.900 5646642574066220928 128.66697580570 -27.01495378927 11.4301 11.0009 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 21447_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21447_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:56.48 -23:19:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 1.097 5701897087801116288 128.73536234487 -23.31864093101 11.0877 10.0473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21448_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21448_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:16.46 -22:45:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 4.081 5651918507585008640 138.06741737887 -22.76602579952 10.1830 9.8318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21453_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21453_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:04.66 -25:19:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.776 5695422201268716288 128.01966775424 -25.31957696886 11.6390 11.4075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21455_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21455_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:20:38.13 -25:03:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 2.396 5696040195525485184 125.15926988554 -25.06028339697 11.5768 11.3251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21456_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21456_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:23:46.17 -23:56:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 3.797 5696584655636074624 125.94268609581 -23.94645645940 11.8550 11.4468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21458_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21458_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:27:23.76 -27:10:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 0.390 5646770804609468288 126.84898204216 -27.16658724546 11.5509 11.1472 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#
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Considering the candidate 21460_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21460_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:23.72 -25:25:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 1.442 5695394301160113280 128.09908132431 -25.42797108707 11.6554 11.5820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21462_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21462_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:29.06 -24:56:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.108 5695484220597521536 128.12128702566 -24.94030188277 11.5026 10.8676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21465_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21465_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:25:00.00 -27:02:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 0.872 5693322408941717888 126.25021632298 -27.04931367005 11.6778 11.4973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21466_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21466_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:30:50.56 -24:57:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 0.618 5695492741812825728 127.71077567499 -24.96294593180 11.5165 10.8721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21468_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21468_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:41:21.94 -22:47:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 1.789 5702196597343016704 130.34091500473 -22.79268196732 11.6566 11.1497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21471_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21471_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:40.19 -25:10:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 1.772 5695507172897869696 128.66767255826 -25.17003586024 11.6831 11.4349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21475_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21475_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:25.71 -23:30:07.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)
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Considering the candidate 21481_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21481_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:43.75 -23:26:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 0.318 5701693265832338048 129.43238428416 -23.43353111285 11.5847 11.0389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21483_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21483_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:27:49.02 -24:22:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 1.783 5695750474209183232 126.95422439164 -24.37177261566 11.8610 11.5581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21485_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21485_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:18:30.17 -24:31:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 1.795 5696270126588936064 124.62610941698 -24.52936761454 11.6565 11.6082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21489_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21489_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:14:47.28 -27:29:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 2.326 5693108657011720192 123.69737976415 -27.49341244915 11.6146 11.1311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21493_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21493_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:20:34.23 -25:34:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 0.186 5695954330536962816 125.14257586282 -25.56989013565 11.4105 10.5501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21496_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21496_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:15.31 -27:44:45.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)
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Considering the candidate 21506_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21506_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:20:52.48 -27:06:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 0.736 5693538634764123392 125.21889178218 -27.10126290111 11.7172 11.6257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21507_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21507_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:29:36.04 -26:55:02.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21510_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21510_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:25:30.16 -27:55:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 0.595 5645207230353589632 126.37550999809 -27.93015964740 11.4746 10.7753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21522_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 21522_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:09:30.00 -27:37:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 2.318 5693795989212982528 122.37452162154 -27.62229034804 11.1096 9.8375 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10096_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 10096_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01791_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 01791_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11121_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 11121_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 57s
Prepared the HTML report for the field Pyx-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 ####
08:33:37.49 -30:16:49.5
09:05:04.25 -25:05:21.8
08:24:25.94 -24:21:25.3
09:08:54.45 -24:08:34.9
09:10:28.13 -23:17:23.2
09:08:48.30 -26:25:20.0
09:08:47.12 -25:21:12.4
09:09:45.66 -27:00:52.5
09:06:10.27 -30:59:27.2
09:11:49.74 -22:13:56.6
09:08:59.86 -30:23:58.2
09:07:47.54 -29:57:09.4
09:06:48.27 -30:36:46.3
09:09:19.54 -23:32:20.3
09:11:47.17 -24:43:28.8
08:40:58.30 -23:27:03.0
09:10:50.09 -23:28:10.1
09:11:28.93 -30:14:13.7
08:15:13.73 -30:25:32.3
09:00:31.59 -25:43:16.2
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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat to cache
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
Creating symlink local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
Creating symlink local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
Creating symlink local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits exists and is non-empty
wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits exists and is non-empty
wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits exists and is non-empty
wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.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 08:38:19.346 -26:00:33.84
Second-epoch image center 08:38:24.953 -26:00:04.51
Angular distance between the image centers 0.02 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 08:38:19.346 -26:00:33.84
Second-epoch image center 08:38:23.628 -25:59:53.48
Angular distance between the image centers 0.02 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 08:38:24.953 -26:00:04.51
Second-epoch second image center 08:38:23.628 -25:59:53.48
Angular distance between the image centers 0.00583 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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits &> /tmp/tmp.BcXPwAh03W
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits &> /tmp/tmp.aSGR1G8DJi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits &> /tmp/tmp.oatPuMllgi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits &> /tmp/tmp.Ki3KFhP1Uj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
Calibrating the magnitude scale
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits and wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.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_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits and wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits and wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat
The reference image (wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits) and catalog (wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat) found
'wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.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 17565 out of 145614 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.610894
a=0.000000 b=1.000000 c=22.610894
From vast_summary.log: estimated ref. image limiting mag.: -8.05
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.56
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 943 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
2.0 pix Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
2.7 pix Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
2.7 pix Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
Limiting magnitude estimates:
14.6 mag. Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
14.5 mag. Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
14.1 mag. Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
14.1 mag. Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BcXPwAh03W (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/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=14696, passed=145605
Got 145605 stars (including 130674 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat
util/solve_plate_with_UCAC5 got 145605 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 940 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: 0.38"
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 939 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 - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits -region wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-24-38_20.00sec_-15.00C_LIGHT_0265.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.aSGR1G8DJi (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/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=14382, passed=142155
Got 142155 stars (including 127556 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat
util/solve_plate_with_UCAC5 got 142155 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 940 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: 0.37"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits -region wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-09_00-25-17_20.00sec_-14.90C_LIGHT_0266.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.oatPuMllgi (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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=9698, passed=85282
Got 85282 stars (including 75492 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 85282 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 928 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: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.76"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits -region wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-31-19_20.00sec_-14.90C_LIGHT_0014.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.Ki3KFhP1Uj (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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.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_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=9863, passed=86119
Got 86119 stars (including 76149 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 86119 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 926 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: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.78"
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 923 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Pyx-01-Q2b1x1_203249_TTUQ2b1x1_6751_xh1hqZb0/Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits -region wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015.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 Pyx-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out105050.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out169011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out24770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out73404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out167013.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out168120.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out168957.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out07553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99495.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 470s
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: 214s
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Considering the candidate 166893_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166893_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:51.47 -21:59:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.912 5655058953312558720 136.96409371000 -21.98732614230 12.3064 11.8048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166897_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166897_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166899_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166899_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:27:54.70 -22:48:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.000 5696952102976900736 126.97808780966 -22.80264515592 13.9400 13.3366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166901_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166901_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:00.64 -21:34:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 5.051 5655109668286376448 137.00142753730 -21.58130055051 12.4940 12.0804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166902_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166902_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 166908_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166908_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:14:37.05 -22:21:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.332 5699853370569379968 123.65377986331 -22.36064739154 13.6831 13.0243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166909_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166909_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:18:23.03 -22:59:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.561 5699565573401211136 124.59571141499 -22.98834141958 13.8373 13.5312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166914_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166914_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:52.52 -23:56:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.797 5651364598538594432 136.96971395651 -23.93309634044 12.1305 11.6313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166920_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166920_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 166922_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166922_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:26.62 -24:33:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.673 5651233722295184384 135.86077908964 -24.55191678821 13.0642 12.4787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166924_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166924_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:12:23.35 -21:45:38.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)
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Considering the candidate 166928_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 166928_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166936_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166936_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:15:01.41 -24:37:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.259 5696302910084616704 123.75549249884 -24.62828799790 13.8467 13.1572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166939_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166939_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 166940_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166940_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:12.60 -22:44:03.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 166941_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166941_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:11.54 -21:45:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 3.146 5655238586024272896 135.54873153528 -21.76260574251 12.5517 12.0031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166942_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166942_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:57.66 -21:18:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.690 5655340703166316160 136.23985347240 -21.31728851243 12.4483 12.0165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166943_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166943_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:35.50 -24:25:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.622 5651320545057197952 136.39831568960 -24.42988111551 12.4357 11.6737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166946_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166946_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:26.75 -21:39:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 1.041 5702950935336141312 128.61149007720 -21.66492660861 14.0538 13.6245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166948_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166948_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:30.59 -25:33:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 5.028 5650915757276800000 136.12670647908 -25.55377651441 12.4777 11.8725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166951_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166951_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:18.05 -22:48:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.316 5654885166051127424 136.57554368387 -22.80072269115 12.5315 11.9723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166953_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166953_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:59.82 -23:54:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.849 5651400053491768064 136.24851830179 -23.91156205327 12.4638 11.9170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166955_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166955_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:53.86 -23:39:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.869 5651433829115650944 136.47492361474 -23.65737915147 12.2085 11.7438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166958_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166958_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:23.52 -21:27:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 1.737 5655288892976746880 136.34795406441 -21.45709173259 12.2877 11.7366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166964_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166964_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:25.59 -21:54:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.283 5655069398673018240 136.60645130241 -21.90569676192 12.0602 11.3415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166965_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166965_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:37.71 -23:05:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.002 5654475937270739072 136.15697242231 -23.08840714467 12.3501 11.8935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166966_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166966_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:32.33 -22:29:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.901 5655122587546569344 135.88377732523 -22.49099964485 12.3985 11.7751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166967_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166967_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:24.84 -25:29:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.045 5650908915392518144 136.60334708422 -25.48475391980 12.2935 11.8910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166971_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 166971_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166980_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166980_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:16:37.24 -22:16:20.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)
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Considering the candidate 166981_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166981_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:05.94 -26:05:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.593 5649903068411170560 137.77395065032 -26.08591987165 11.8607 11.3849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 166982_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166982_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:05:59.75 -22:47:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.118 5699208747517616000 121.49898285679 -22.79238484864 13.3629 12.7741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 166985_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166985_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:49.62 -21:35:04.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 166989_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166989_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:06.93 -24:00:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.152 5651392803586966400 136.02952789347 -24.00856966060 12.2783 11.7232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 166990_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166990_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:52.38 -24:57:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.150 5651187744668412288 135.71889181931 -24.95539274042 12.4512 11.9623 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 166992_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166992_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 166993_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166993_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:39.21 -25:26:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.832 5650965127924486656 136.16235354501 -25.44094715399 12.0301 11.6221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 166994_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166994_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 166995_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166995_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:41.26 -21:37:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 0.926 5655281776215033600 136.42165426435 -21.61977559411 12.1161 11.5927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 166997_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166997_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 166999_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 166999_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:34.14 -29:46:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.382 5645269180959251200 129.39248320719 -29.76743848992 12.8553 12.1417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167002_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167002_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:06:09.37 -25:41:32.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 167003_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167003_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:41.89 -27:59:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.972 5636206937398784512 137.17469215900 -27.99031466811 11.7731 11.3369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167006_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167006_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:28.42 -24:35:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.854 5651083226641234176 137.61822651865 -24.59447661515 11.4352 10.7202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167008_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167008_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167009_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167009_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:10.07 -26:21:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.999 5648622927638184832 136.29296826429 -26.36561640659 12.2818 11.7887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167013_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167013_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:28.80 -22:52:00.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 167015_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167015_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:16.46 -28:15:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.237 5648098426232457472 136.31945451987 -28.25396872928 11.9287 11.2784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167016_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167016_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167017_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167017_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:33.00 -29:06:12.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 167020_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167020_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:52.24 -25:47:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.373 5650158326906890624 136.96808982289 -25.79845894069 11.7360 11.2619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167021_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167021_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:26.44 -22:20:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.529 5654995907487879168 136.85909864452 -22.34898174611 11.9496 11.4601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167022_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167022_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167024_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167024_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:04:29.05 -30:03:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.485 5596656675217340288 121.11963177119 -30.05036121631 12.0549 11.6179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167025_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167025_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167026_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167026_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:13.57 -23:47:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.073 5651557219231828480 137.30640429527 -23.79089640761 11.6877 10.9466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167027_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167027_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:07.47 -23:29:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.184 5651774677719237504 137.53164187266 -23.48852441855 11.8555 11.2850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167029_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167029_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167030_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167030_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 167031_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167031_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167034_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167034_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:19:29.54 -22:58:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.527 5699891612955172480 124.87308622985 -22.97964644027 13.4419 12.7877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167037_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167037_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167038_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167038_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:30.49 -24:57:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.392 5651017663963474560 136.37695197468 -24.96446140944 12.0825 11.6031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167039_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167039_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:27.61 -25:48:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.210 5650896584543079168 136.36407328801 -25.80641846354 11.9393 11.2692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167040_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167040_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:51.27 -25:23:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 2.836 5650935784707917696 136.96448704751 -25.39879847163 11.8436 11.3135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167041_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167041_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:35.44 -25:10:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.372 5650998907843524096 136.39839358580 -25.18171479651 11.9098 11.4375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167043_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167043_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:45.11 -25:00:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.970 5651051718761259008 136.93853516281 -25.00699506751 11.7689 11.2412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167044_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167044_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:49.84 -28:26:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.604 5636096745714730240 136.95684438465 -28.43725461046 11.4163 11.0096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167045_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167045_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:19:43.01 -25:09:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.943 5696026760866855296 124.93003423801 -25.16174507227 13.5834 12.8373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167048_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167048_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:40.18 -25:14:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.947 5650976986330505088 136.16695515191 -25.24661480488 11.8529 11.5039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167049_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167049_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:05:00.22 -30:19:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 5.451 5596262294141086848 121.25264180551 -30.31955181350 12.1352 11.6824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167055_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167055_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:11.63 -28:01:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.858 5648169280312157824 135.79702510955 -28.01799659741 11.7476 11.2634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167056_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167056_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:07.62 -24:31:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.824 5651128439759964288 136.53211981404 -24.52767654483 11.9283 11.4653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167059_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167059_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:08:33.47 -29:44:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.614 5596726532873473792 122.13901587127 -29.74907443751 13.4416 12.9909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167061_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167061_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:54.90 -28:13:03.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)
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Considering the candidate 167062_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167062_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:53.86 -23:31:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 0.621 5651808418982318080 136.72453701271 -23.52616036262 11.8808 11.3570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167064_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167064_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:07.01 -25:12:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.930 5650954034025428224 136.77930325073 -25.20942297243 11.7662 11.3875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167066_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167066_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:55.41 -28:55:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.913 5636044175318430208 136.73047917424 -28.92720841935 11.4473 10.9810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167067_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167067_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:54.64 -25:01:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.017 5650292987018518656 137.47743928527 -25.01938789909 11.5642 11.2781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167068_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167068_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:52:10.01 -25:26:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.814 5652293200530900992 133.04066638343 -25.43926448570 13.0852 12.3595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167071_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167071_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:40.98 -27:40:10.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)
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Considering the candidate 167074_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167074_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:45.43 -24:33:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.403 5651091674840620032 137.18935176408 -24.56505866289 11.5312 10.8290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167075_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167075_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:05.71 -23:25:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.269 5651789319264581760 137.27360938937 -23.41881017119 11.5636 10.8423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167078_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167078_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:37.02 -24:20:22.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 167080_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167080_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:54.09 -22:42:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.582 5654876056423977344 136.72470034451 -22.70638449791 11.9766 11.5879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167084_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167084_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 167086_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167086_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:00:19.14 -29:24:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 2.491 5647544688988306688 135.07935808409 -29.40843528163 11.6038 11.0996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167088_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167088_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:15.92 -25:09:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.461 5651001995922789888 136.31673234420 -25.15321299135 11.8659 11.3504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167091_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167091_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:03.66 -28:05:03.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)
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Considering the candidate 167093_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167093_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:56:11.78 -27:53:33.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)
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Considering the candidate 167096_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167096_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:00:37.10 -29:57:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.265 5635505345901465600 135.15327363067 -29.95959024895 11.3936 10.9060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167098_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167098_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:56:11.31 -30:05:37.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 167099_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167099_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:11.68 -25:28:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.171 5650184169727076096 137.04956700988 -25.46691097342 11.3467 11.0088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167100_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167100_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167101_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167101_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:47.98 -25:52:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.131 5649395231477504384 136.19923930417 -25.87366684440 11.6523 11.2106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167102_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167102_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167103_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167103_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 167105_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167105_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:05:59.90 -30:04:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.303 5596647161880411776 121.50073513725 -30.07146517272 12.1587 11.9142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167107_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167107_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 167108_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167108_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:35.85 -26:23:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.442 5648600151430017920 136.14980667445 -26.38609029398 11.6506 11.1917 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167109_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167109_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:01:58.07 -30:48:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.778 5629403881004815104 135.49177090772 -30.80916122652 10.9336 10.5261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167111_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167111_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167112_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167112_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:07.62 -26:10:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 3.533 5648629838243794816 136.28282641187 -26.17139436645 11.5425 11.1038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167113_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167113_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:44.07 -26:05:54.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
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Considering the candidate 167116_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167116_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:38:05.66 -24:41:22.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)
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Considering the candidate 167117_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167117_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:39:38.40 -27:02:48.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)
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Considering the candidate 167118_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167118_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 167120_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167120_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167121_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167121_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 167125_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167125_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:01:11.76 -21:40:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.000 5655970212229000192 135.29956436314 -21.67765553820 11.7368 11.2537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167126_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167126_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:22.11 -26:59:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.181 5649784943928708736 137.59061947534 -26.99836744197 11.0205 10.6185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167129_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167129_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:09:43.83 -21:40:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.292 5700868391598433920 122.43265224869 -21.66805290650 12.6063 12.2991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167132_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167132_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:46:44.97 -23:36:44.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 167133_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167133_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167134_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167134_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167135_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167135_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 167137_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167137_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:29:12.30 -24:34:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.788 5695752260916520960 127.30114240073 -24.57469588884 12.7204 11.8420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167138_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167138_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:01:45.50 -29:37:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 3.443 5635539808718908032 135.43855455450 -29.63025598782 11.0645 10.6537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167141_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167141_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:53.93 -24:35:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.363 5651115352996534656 136.97501089885 -24.59776747051 11.3368 10.8889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167142_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167142_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167143_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167143_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167144_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167144_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167150_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167150_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:13.62 -28:48:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 4.990 5636004902137354496 137.05710975702 -28.81040537664 10.7044 10.4649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167151_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167151_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:21.56 -26:14:35.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)
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Considering the candidate 167153_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167153_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:30.53 -30:16:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 3.077 5635446380290941312 136.12623358976 -30.26810198630 10.6546 10.2147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167154_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167154_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:00.39 -29:17:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 3.548 5635610104444584704 136.50267366042 -29.29081200328 10.8866 10.4751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167159_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167159_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167160_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167160_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:12.94 -28:37:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.465 5647737515839961984 135.55468926633 -28.61931684831 10.9777 10.5928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167161_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167161_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:07.82 -29:47:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.905 5635533761404969728 135.53189551646 -29.79848462284 10.7557 10.5618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167162_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167162_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:10.69 -28:56:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 3.416 5635670989900619648 136.54394401183 -28.94920826720 10.6347 10.1363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167163_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167163_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:55.77 -27:29:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.664 5648246383565924480 137.23177270049 -27.49320645940 10.7327 10.2549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167164_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167164_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:36.86 -29:59:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 1.101 5635551246212795008 136.40391268878 -29.99700043175 10.5166 10.2224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167165_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167165_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:35:23.51 -30:16:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 5.146 5643729864681058560 128.84941454260 -30.27868147471 11.8685 11.1983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167166_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167166_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:30.76 -26:42:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 4.856 5648356987562985344 137.12934714629 -26.70974206114 10.6631 10.3944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167167_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167167_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 167168_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167168_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:08:35.57 -24:32:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.428 5697949772345366656 122.14856400329 -24.54620151736 12.4295 11.7417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167169_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167169_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:45.72 -28:42:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 1.253 5647700166804135424 136.19084706183 -28.70266850326 10.6596 10.3509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167172_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167172_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167173_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167173_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:29.22 -27:28:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 3.375 5648210821235280128 136.37279382140 -27.48334120913 10.7435 10.4348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167174_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167174_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167176_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167176_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 167178_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167178_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 167180_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167180_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:46.81 -28:02:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 4.807 5648165535100639616 135.94382564863 -28.04543332849 10.6570 10.2364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167183_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167183_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:39.25 -28:03:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 2.792 5648118595404034048 136.66388033359 -28.05874343185 10.2372 9.9598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167184_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167184_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:16.49 -27:44:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 3.832 5648188899722478592 136.31753471238 -27.73723185555 10.4061 9.9912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167185_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167185_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:46.83 -30:03:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 3.799 5635445250719382784 135.69633529240 -30.05534887077 10.1760 9.8862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167187_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167187_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:02:31.23 -29:49:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 2.525 5597054256057600128 120.63070199542 -29.82851915921 10.3893 9.7128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167189_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167189_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 167190_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167190_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167191_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167191_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:58:09.97 -31:06:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.477 5629333198720793344 134.54201287891 -31.10980722345 9.6533 9.5003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167192_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167192_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167193_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167193_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:20.14 -29:01:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 4.569 5635676732276392832 136.33527528765 -29.02877559206 9.4577 9.2337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167195_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167195_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167197_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167197_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:56.90 -30:21:58.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167199_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167199_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:23.42 -23:10:31.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 167202_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167202_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:36.59 -25:50:17.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167203_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167203_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:46.29 -25:48:10.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167204_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167204_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:34.56 -29:49:01.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167205_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167205_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:50.70 -28:19:01.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167208_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167208_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:22.25 -28:56:49.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167209_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167209_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:26.43 -25:35:57.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167210_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167210_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:29.20 -26:17:12.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167219_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167219_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:03.01 -21:25:02.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167227_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167227_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:35.48 -31:01:04.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167228_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167228_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:32.11 -28:25:49.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167230_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167230_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:57.91 -21:31:48.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167231_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167231_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:01:55.24 -29:37:19.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167232_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167232_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:34.09 -31:01:03.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167235_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167235_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:14.71 -28:29:06.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167236_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167236_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:52.42 -23:19:33.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167242_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167242_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:27.90 -23:31:08.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167245_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167245_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:36.70 -30:32:45.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167254_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167254_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:17.84 -30:09:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.11, MAG_FAINT_SEARCH_LIMIT=11.09)GAIADR2_OUTPUT=# 2.617 5635310869779062400 137.32517270797 -30.16087692477 8.4540 7.4989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167256_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167256_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167259_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167259_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:54.35 -24:08:35.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167264_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167264_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167269_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167269_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:04.45 -27:01:45.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167270_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167270_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:15.56 -30:16:33.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167271_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167271_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:06.37 -27:26:24.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167273_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167273_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:36.71 -28:29:02.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167275_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167275_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167276_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167276_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:28.04 -23:17:23.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167277_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167277_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:23:50.95 -20:39:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 0.954 5706403058251054464 125.96232006761 -20.65276378687 10.4468 10.0918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167281_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167281_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 167282_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167282_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:06.39 -22:03:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 3.583 5655054589624917632 137.02573881150 -22.06508978800 9.7355 9.6355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167289_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167289_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167295_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167295_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:18.94 -25:23:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 4.608 5650186093872413824 137.07769745712 -25.39970794473 9.4705 9.2816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167298_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167298_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:19.91 -31:07:15.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 167300_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167300_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:46.99 -25:21:13.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167305_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167305_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 167307_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167307_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167308_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167308_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:27.87 -21:14:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 5.389 5679322666675260928 137.11489721681 -21.25077061476 10.0051 9.8121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167311_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167311_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:02.83 -30:52:36.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 167312_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167312_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:22.58 -31:08:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.72, MAG_FAINT_SEARCH_LIMIT=11.70)GAIADR2_OUTPUT=# 1.192 5629146148606101248 136.09414741951 -31.13874331608 9.1546 8.4247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167314_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167314_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:40.76 -30:16:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 2.799 5635306162497692928 137.42073176668 -30.27146709323 9.0178 8.2040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167315_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167315_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 167316_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167316_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167317_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167317_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167319_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167319_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:18.54 -31:07:11.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 167321_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167321_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 167323_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167323_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167324_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167324_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167326_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167326_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167327_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167327_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:47.94 -30:36:46.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167333_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167333_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 167337_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167337_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167341_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167341_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:49.72 -22:13:56.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167346_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167346_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:14.49 -29:55:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 3.306 5634942803967328384 138.06137999576 -29.92367984433 9.1699 8.2170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167349_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167349_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167351_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167351_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 167353_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167353_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167356_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167356_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:34.69 -24:11:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 3.184 5651491695210723456 138.14478113267 -24.18617073839 9.6956 9.0270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167357_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167357_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:27.71 -31:10:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 1.356 5635134501246615552 136.36552174421 -31.17948383383 9.3024 8.5470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167359_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167359_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 167363_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167363_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 167364_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167364_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167367_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167367_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:30.26 -30:18:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 3.555 5635296301252850304 137.12718753414 -30.30989636776 9.4473 8.4453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167369_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167369_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167370_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167370_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:19.64 -23:32:19.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167373_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167373_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 167374_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167374_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 167375_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167375_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:20.14 -26:25:04.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)
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Considering the candidate 167376_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167376_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:12.30 -30:58:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 4.905 5634406384032877952 137.30249579603 -30.96762332286 9.1890 8.2375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167379_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167379_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167380_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167380_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 167381_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167381_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:10.29 -30:59:27.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167383_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167383_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167387_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167387_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:45.28 -31:00:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 1.874 5634405112722588672 137.18866280493 -31.00754820996 9.2083 8.5236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167390_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167390_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 167392_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167392_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167393_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167393_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 167395_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167395_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:46.02 -21:29:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 2.101 5679093010480673024 137.94194484548 -21.49677867980 9.8416 9.1330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167399_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167399_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:00.25 -30:23:57.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167400_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167400_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 167402_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167402_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:39.14 -21:19:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 3.143 5679098404959417216 137.91355429758 -21.32743951426 9.8136 9.0372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167403_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167403_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167404_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167404_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 167407_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167407_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:31.18 -30:43:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 1.747 5635178035035603584 136.88007886830 -30.72138141998 9.5092 8.7574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167417_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167417_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:28.99 -30:14:14.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167421_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167421_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:26.49 -30:59:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 2.948 5634414011894760960 136.85943106308 -30.99395741509 9.4129 8.9251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167424_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167424_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:47.35 -24:43:27.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167426_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167426_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167427_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167427_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:09.52 -30:46:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 1.292 5635183326435451264 136.53930061617 -30.77664511432 9.6029 8.9726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167429_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167429_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167430_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167430_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167431_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167431_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 167433_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167433_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167440_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167440_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 167442_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167442_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 167444_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167444_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167445_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167445_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:32.74 -29:59:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 2.368 5635328358888394880 137.13717086659 -29.99879974874 9.7089 9.2130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167446_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167446_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167454_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167454_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167455_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167455_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167457_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167457_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167461_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167461_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167463_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167463_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167465_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167465_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167471_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167471_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167472_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167472_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167474_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167474_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:42.98 -24:17:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.67, MAG_FAINT_SEARCH_LIMIT=12.65)GAIADR2_OUTPUT=# 2.979 5699328731722711680 123.42824266610 -24.29627069676 12.4455 10.5564 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167477_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167477_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167479_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167479_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:32.26 -29:47:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 1.498 5635696106870734848 137.88393940901 -29.79634745064 9.6688 8.9498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167480_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167480_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 167483_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167483_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167486_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167486_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 167488_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167488_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:34.61 -31:05:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 3.535 5629193358887894784 135.89503911642 -31.09926018485 9.9208 8.9527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167490_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167490_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167492_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167492_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167497_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167497_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167498_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167498_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167499_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167499_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 167500_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167500_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167501_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167501_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167503_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167503_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 167506_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167506_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167507_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167507_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 167513_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167513_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167514_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167514_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167515_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167515_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 167520_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167520_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167521_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167521_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 167524_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167524_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167525_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167525_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167528_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167528_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167529_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167529_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 167532_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167532_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167535_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167535_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167536_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167536_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167538_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167538_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167539_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167539_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167541_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167541_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167543_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167543_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 167544_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167544_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:13.21 -31:05:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 3.311 5635148897976982528 136.30593221992 -31.09690325046 10.0629 9.1492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167546_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167546_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167548_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167548_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:05.60 -30:31:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 1.235 5635194184112617856 136.77368641563 -30.53024189406 9.9876 9.3092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167549_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167549_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167551_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167551_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167553_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167553_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:20:29.45 -20:37:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.525 5707188624950932480 125.12259147773 -20.62370921065 11.4740 10.6340 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#
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Considering the candidate 167556_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167556_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167557_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167557_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 167559_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167559_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167563_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167563_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167564_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167564_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167565_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167565_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167566_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167566_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 167570_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167570_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167573_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167573_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:08:22.20 -23:36:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 2.050 5698168089816867584 122.09286832005 -23.60504203623 11.7995 11.6417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167575_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167575_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167576_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167576_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167581_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167581_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167584_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167584_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 167587_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167587_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167590_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167590_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167596_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167596_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:03.38 -31:05:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 3.188 5629147110678791680 136.01491365493 -31.08816693952 10.2294 9.2537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167598_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167598_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167599_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167599_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 167600_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167600_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 167602_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167602_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 167612_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167612_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 167614_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167614_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167619_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167619_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:49.06 -27:27:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 4.677 5648212229984675840 136.45324930726 -27.45631174269 10.5286 10.1105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167623_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167623_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167624_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167624_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:25:08.23 -22:14:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.713 5700046467993997056 126.28413767525 -22.24130416794 12.2340 11.6099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167626_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167626_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167630_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167630_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 167631_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167631_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 167634_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167634_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:32.71 -30:50:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 1.234 5634501904101807488 137.38623470773 -30.83377185458 9.9386 9.2226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167636_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167636_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167638_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167638_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 167639_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167639_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:10.89 -31:10:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 5.454 5629145805008752896 136.04679469602 -31.16843314382 10.2552 9.5581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167640_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167640_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167641_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167641_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 167650_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167650_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:49.25 -30:23:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.855 5635289154427316992 136.95465565733 -30.39294538621 10.1722 9.5295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167654_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167654_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167655_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167655_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167656_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167656_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 167661_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167661_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 167666_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167666_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167669_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167669_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167670_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167670_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 167672_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167672_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167674_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167674_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167677_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167677_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:21.50 -30:37:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.591 5635212291688911104 136.34016023678 -30.63335449427 10.4607 9.4778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167679_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167679_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167686_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167686_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 167687_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167687_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167688_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167688_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:51.05 -26:17:07.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 167696_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167696_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167697_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167697_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 167699_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167699_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167702_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167702_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:44.03 -30:30:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 5.403 5635287363421776128 136.93319128390 -30.51184412972 10.2747 9.6311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167704_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167704_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:46.74 -23:21:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 4.721 5651779767257438464 137.44377114061 -23.36387174331 10.8179 10.3660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167709_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167709_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167712_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167712_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 167713_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167713_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 167714_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167714_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:51.16 -30:34:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 3.831 5635216719801445632 136.21418929733 -30.57457001500 10.6976 9.5056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167716_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167716_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167717_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167717_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167718_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167718_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:13.94 -30:13:05.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)
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Considering the candidate 167719_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167719_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:34.56 -30:12:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.183 5634919954741323136 138.14350879775 -30.20729405344 9.9854 9.2832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167721_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167721_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:34.91 -30:26:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 2.654 5635288501592311552 136.89623251963 -30.44770176537 10.4150 9.5568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167722_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167722_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 167728_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167728_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 167732_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167732_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 167733_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167733_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167735_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167735_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167736_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167736_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167741_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167741_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 167744_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167744_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 167745_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167745_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 167746_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167746_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167748_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167748_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 167750_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167750_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:44.64 -30:48:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 5.074 5634505065197643648 137.68448822128 -30.80732568428 9.9773 9.5069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167754_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167754_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167755_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167755_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167759_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167759_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 167760_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167760_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:11.74 -30:09:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.411 5635301489573047936 137.04893709537 -30.16377602811 10.5249 9.8323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167761_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167761_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167763_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167763_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167769_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167769_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 167771_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167771_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167779_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167779_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:50.04 -26:19:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 5.569 5649870843274248576 137.45677432297 -26.32578384279 10.8462 10.5524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167786_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167786_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167787_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167787_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167788_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167788_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:32.88 -23:15:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.181 5651693318155284096 138.13700520923 -23.25189415399 10.8783 10.1602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167789_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167789_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167797_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167797_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167803_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167803_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 167804_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167804_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167808_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167808_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:56.20 -30:52:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.867 5634442904133787520 137.98473169856 -30.87946186687 9.9692 9.5670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167811_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167811_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167812_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167812_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167815_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167815_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167816_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167816_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167819_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167819_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167821_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167821_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167825_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167825_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:17:30.50 -21:04:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.843 5701155157973925376 124.37675870768 -21.07560731754 12.3846 11.5974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167828_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167828_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:42.14 -30:32:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 4.138 5635412540248706176 135.67665475248 -30.54535189983 10.9238 9.4823 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167831_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167831_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167836_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167836_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:25.17 -28:58:31.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)
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Considering the candidate 167838_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167838_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:45.25 -30:37:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.024 5635235209641322752 136.43812325830 -30.63190420690 10.7007 9.9405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167840_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167840_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167844_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167844_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:20.61 -30:41:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 3.156 5635175969149956992 137.08643989381 -30.69181314778 10.5276 9.6359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167845_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167845_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167848_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167848_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167849_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167849_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167855_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167855_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:18.86 -31:00:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.471 5634414080614242432 136.82931198973 -31.00500685834 10.4044 9.7534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167856_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167856_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167857_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167857_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:04.56 -23:51:09.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)
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Considering the candidate 167858_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167858_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167861_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167861_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:22:40.73 -28:56:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.381 5645004920212764544 125.67002159472 -28.94442582293 12.4154 12.0740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167862_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167862_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167869_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167869_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:46.82 -30:49:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 2.943 5634458061075560960 137.69588660403 -30.83129996795 10.2368 9.5406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167874_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167874_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:58.33 -29:51:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.854 5635333164952990976 137.49297745966 -29.86451593207 10.5181 9.9712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167877_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167877_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:08.39 -31:06:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 1.999 5635139345969614464 136.53551632028 -31.11261631342 10.4648 9.8006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167879_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167879_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:39.14 -30:25:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.189 5634541177282511104 137.91211128425 -30.42099112065 10.1007 9.6332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167886_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167886_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:30.97 -30:32:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 3.137 5635193428198350720 136.87991736104 -30.54650768691 10.5329 9.8749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167890_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167890_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 167892_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167892_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167898_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167898_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 167901_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167901_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167902_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167902_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:43.21 -30:52:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 5.712 5629214352687851008 135.68141596168 -30.87833910629 10.9134 9.8330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167903_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167903_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:03.94 -30:40:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 4.921 5635190640758239744 136.76493865638 -30.66766923137 10.5809 10.4554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167906_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167906_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167908_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167908_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167909_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167909_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167910_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167910_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167913_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167913_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:12.69 -30:13:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 5.670 5635287024123435008 137.30454960656 -30.21759426394 10.3521 10.0731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167917_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167917_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 167918_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167918_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 167928_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167928_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167929_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167929_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:10:17.51 -20:49:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.646 5701364374421814272 122.57282483376 -20.82457862899 12.3273 11.9838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167930_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167930_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167933_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167933_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 167938_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167938_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:51.75 -29:46:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 2.837 5635338147115049472 137.46653156024 -29.77984580095 10.6103 9.7073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167939_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167939_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 167943_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167943_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167944_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167944_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:33.66 -30:08:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.431 5635299943384797184 137.14012263953 -30.14996366599 10.6170 9.9123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167946_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167946_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 167951_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167951_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167952_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167952_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:23.92 -28:58:35.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)
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Considering the candidate 167960_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167960_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 167963_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167963_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167969_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167969_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167972_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167972_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167973_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167973_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167977_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167977_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167979_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167979_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167983_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167983_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:26.95 -30:16:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.865 5634919130107604736 138.11192169216 -30.26726876377 10.3814 9.6886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167984_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167984_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 167986_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167986_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167992_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167992_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 167995_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 167995_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 167997_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 167997_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 168007_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168007_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:10.97 -24:23:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.298 5697825321371786752 123.29573229082 -24.39247111044 12.7540 12.5491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168018_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168018_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 168020_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168020_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 168022_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168022_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168025_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168025_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168027_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168027_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168035_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168035_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 168037_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168037_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 168039_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168039_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 168043_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168043_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168048_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168048_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:40.50 -25:18:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 5.163 5650947024638843904 136.66775854493 -25.31114742712 11.3380 10.9631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168049_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168049_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:10.80 -27:04:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 4.584 5637765460771354624 138.04370551047 -27.07879189359 10.8684 10.4893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168050_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168050_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168051_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168051_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168053_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168053_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (24.1") between the two second-epoch detections
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Considering the candidate 168054_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168054_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:40:59.26 -27:00:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 1.448 5646222629342971648 130.24699490240 -27.00331270733 12.4717 12.2767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168065_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168065_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168066_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168066_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168069_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168069_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 168070_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168070_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168074_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168074_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168077_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168077_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168078_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168078_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 168079_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168079_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 168081_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168081_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:28.74 -30:54:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 4.874 5634462149884611712 138.12111812337 -30.91420240627 10.4508 9.5615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168082_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168082_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168085_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168085_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168086_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168086_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:54.89 -22:20:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.555 5651996267968444928 137.97950702427 -22.34291735229 11.2486 10.5891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168089_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168089_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:04.49 -30:32:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.931 5634535847224174464 137.76842963592 -30.54682066437 10.5852 9.9199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168092_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168092_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:11.41 -22:42:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 2.711 5702740516299392128 128.04776938793 -22.71616769226 12.9394 12.6795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168098_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168098_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 168099_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168099_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168101_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168101_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168103_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168103_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168104_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168104_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:04.56 -21:55:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 4.494 5679040641942702080 137.77008284412 -21.92678677356 11.3339 10.5830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168105_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168105_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 168107_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168107_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168108_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168108_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:20.59 -31:00:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 3.473 5635152608828802560 136.08666693622 -31.01155083510 10.9028 10.0650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168109_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168109_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:36.30 -29:59:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.276 5635354094332486400 136.90197761742 -29.99321731766 11.0199 10.1646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168110_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168110_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 168112_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168112_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:52:41.10 -29:42:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 3.871 5641719648188244480 133.17235424715 -29.71581948947 11.6985 10.0162 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168117_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168117_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168120_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168120_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:55.09 -30:49:04.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)
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Considering the candidate 168121_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168121_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168122_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168122_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 168123_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168123_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:06.65 -30:30:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 5.414 5634536298199440384 137.77931596715 -30.50133593878 10.6820 9.8383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168130_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168130_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168131_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168131_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 168138_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168138_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168140_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168140_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:49.96 -21:57:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 5.044 5655059606147585920 136.95723300702 -21.96232363816 11.7752 11.6135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168143_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168143_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168144_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168144_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 168147_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168147_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168149_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168149_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:58.50 -23:54:51.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)
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Considering the candidate 168152_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168152_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:39:53.16 -23:48:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 2.034 5701703539394687488 129.97211734339 -23.80879320923 13.1060 12.6282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168161_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168161_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:07.39 -30:38:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 4.023 5635190851218023424 136.78199738172 -30.64513983255 10.9738 10.2294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168163_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168163_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 168171_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168171_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 168174_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168174_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168175_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168175_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 168180_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168180_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168181_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168181_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:17.26 -30:02:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.271 5634565744495123840 137.82199492231 -30.03848551536 10.7720 9.9723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168182_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168182_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168186_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168186_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 168188_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168188_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:12.43 -26:09:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 5.383 5649899636734934528 137.80021150213 -26.15544359750 11.3397 11.0706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168192_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168192_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 168194_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168194_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 168201_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168201_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 168205_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168205_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168207_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168207_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:15.35 -22:23:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 0.966 5700583171410047616 123.31414515891 -22.38692770564 12.6258 12.1253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168209_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168209_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:39.55 -29:27:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.418 5635405457844632960 137.16435269728 -29.46396894902 10.9781 10.4007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168213_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168213_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168220_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168220_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 168221_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168221_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:20.72 -30:35:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.642 5635271111265529728 137.08666803047 -30.59468696210 10.7327 10.1357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168224_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168224_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 168225_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168225_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168231_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168231_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:17.02 -30:41:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.468 5635186934207940224 136.57077218008 -30.69979461082 10.7937 10.4586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168234_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168234_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 168241_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168241_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:08.15 -22:05:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 4.070 5652016879515932672 137.78313884726 -22.08997666762 11.5292 11.0934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168242_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168242_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 168243_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168243_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168249_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168249_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:58.19 -25:22:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 2.997 5650222309036978048 137.74154411859 -25.37514554742 11.2616 10.8423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168251_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168251_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168252_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168252_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168253_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168253_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:28.77 -29:58:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.526 5635320421789296128 137.61996542816 -29.98037336699 10.8196 10.1221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168254_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168254_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168255_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168255_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168256_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168256_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168257_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168257_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168259_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168259_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168261_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168261_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168262_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168262_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 168271_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168271_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168272_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168272_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 168277_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168277_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168278_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168278_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168279_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168279_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168285_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168285_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:29.18 -30:36:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 3.142 5634488430785233024 138.12221155730 -30.60190731395 10.6062 9.7815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168286_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168286_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 168288_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168288_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 168291_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168291_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168294_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168294_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 168295_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168295_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168296_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168296_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168298_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168298_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:02.97 -28:45:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 3.713 5636006207807414784 137.01266983644 -28.76677638843 11.0202 10.6117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168299_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168299_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168301_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168301_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:59.63 -25:12:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.948 5650247838322490240 137.99705077271 -25.20862838168 11.2507 10.8110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168307_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168307_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 168311_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168311_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 168314_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168314_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 168320_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168320_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168321_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168321_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168324_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168324_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:04.53 -25:53:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.906 5647318464475567104 128.51856635300 -25.89320236746 13.2317 12.8761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168326_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168326_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 168329_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168329_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168333_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168333_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 168338_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168338_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168343_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168343_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:00.18 -30:39:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.686 5635177141682361472 137.00176478227 -30.66513210586 11.0239 10.0574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168348_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168348_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 168349_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168349_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:34.91 -22:14:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.104 5655000442973434624 137.14439267270 -22.24349068293 11.6006 11.1623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168350_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168350_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:27.56 -30:56:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 5.515 5629199543640899584 135.86510548879 -30.94587522764 11.3036 10.4341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168352_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168352_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 168358_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168358_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:37.15 -30:57:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.813 5634440709404638592 137.90504144970 -30.96409459786 10.6674 9.9169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168359_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168359_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168363_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168363_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168373_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168373_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:06.73 -26:23:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.071 5647062999822461824 129.27777247681 -26.39084069181 13.2960 12.6345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168374_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168374_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:12.05 -22:00:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.069 5655029472657040896 137.29989655320 -22.01112688306 11.8463 11.3979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168375_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168375_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168385_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168385_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 168389_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168389_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:46.37 -21:14:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.804 5655320705798580992 136.69273810272 -21.24834384885 11.7035 11.2497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168390_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168390_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168394_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168394_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 168397_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168397_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168398_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168398_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168399_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168399_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:11.10 -28:43:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 5.368 5636026686211390976 137.29461823055 -28.72961365137 11.2655 11.0214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168404_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168404_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 168406_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168406_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:34.16 -28:19:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 5.885 5636133854232920320 137.64110255995 -28.32864078511 11.1487 10.8879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168407_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168407_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:10.84 -21:31:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.126 5679072188479080832 137.79412121713 -21.52113434591 11.6363 11.2377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168411_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168411_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:40.18 -23:31:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.737 5701911377155698176 128.41719595740 -23.52405834380 13.0597 12.3908 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#
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Considering the candidate 168412_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168412_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 168422_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168422_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168423_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168423_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:15.47 -30:09:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.543 5635343648972089088 136.81395340140 -30.16433322412 11.1816 10.4286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168425_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168425_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:16.74 -24:53:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.934 5650306623537695744 138.06891111295 -24.88679188432 11.4840 10.6496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168432_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168432_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168435_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168435_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:56.56 -29:17:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.702 5635598976188089728 136.98599102821 -29.29327509205 11.0545 10.6211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168436_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168436_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:05:13.22 -23:54:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.217 5698804397815506944 121.30474428662 -23.90714367612 12.7890 12.0752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168444_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168444_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168447_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168447_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168448_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168448_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168453_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168453_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168454_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168454_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 168461_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168461_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 168463_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168463_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 168464_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168464_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 168465_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168465_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168466_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168466_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168468_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168468_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168470_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168470_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168471_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168471_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:30.86 -22:00:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 4.196 5655057441484072704 136.87846773392 -22.01543842316 11.7396 11.2668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168473_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168473_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:43.85 -20:59:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.430 5703226809675524224 128.18291455295 -20.99761924875 12.9791 12.4296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168478_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168478_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 168481_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168481_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168482_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168482_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168483_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168483_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:15.88 -25:14:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 3.796 5650938877084360320 137.06568897706 -25.24826751271 11.7049 11.3204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168485_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168485_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 168489_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168489_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168490_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168490_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 168497_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168497_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:26:54.04 -21:36:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.012 5706077465370071424 126.72525510088 -21.61380280165 13.1908 12.9322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168501_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168501_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168502_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168502_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 168505_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168505_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168506_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168506_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168510_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168510_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168511_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168511_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 168515_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168515_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:44.15 -22:05:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 4.033 5655030262930154624 137.18322014283 -22.09144281498 11.7048 11.1764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168525_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168525_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168528_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168528_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168529_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168529_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:37.70 -25:15:24.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 168530_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168530_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 168537_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168537_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168540_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168540_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 168542_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168542_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168545_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168545_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168550_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168550_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168555_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168555_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168559_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168559_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168561_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168561_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:20.14 -25:38:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 4.165 5650161389220555264 137.08345943673 -25.63994227861 11.9048 11.3432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168563_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168563_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 168572_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168572_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168574_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168574_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 168578_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168578_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168584_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168584_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168585_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168585_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168595_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168595_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168596_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168596_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 168604_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168604_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:59.66 -25:07:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 4.948 5650255363105179136 137.99756118437 -25.12376636886 11.6328 11.2934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168612_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168612_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:01.69 -30:49:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 1.968 5635159480776187264 136.50641326119 -30.81703150359 11.0627 10.6602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168614_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168614_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 168616_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168616_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168617_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168617_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 168618_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168618_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168620_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168620_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 168622_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168622_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 168623_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168623_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:03.54 -30:24:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.594 5635289669823382528 137.01525832452 -30.40257648551 11.1800 10.4350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168624_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168624_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:29.85 -26:24:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.572 5649889187076882944 137.62313768978 -26.40880256650 11.5764 11.0370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168625_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168625_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:12.79 -29:58:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 2.156 5635363130943441920 136.55328961784 -29.98298782708 11.4539 10.6481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168628_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168628_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:46.20 -30:35:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.081 5635180508936720128 136.94365204116 -30.59663265528 11.3394 10.6599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168634_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168634_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:26:41.52 -23:08:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.454 5696915917873827328 126.67307914389 -23.14895243934 13.3314 12.6454 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#
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Considering the candidate 168640_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168640_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168647_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168647_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168650_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168650_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:31.65 -26:27:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.930 5649867338580966272 137.38131138455 -26.45837569149 11.5722 11.1104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168655_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168655_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:41:38.03 -22:11:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.143 5702441857156493312 130.40890283028 -22.18548668905 13.3536 12.9090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168666_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168666_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 168669_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168669_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 168672_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168672_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:46.46 -26:06:10.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 168674_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168674_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168675_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168675_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 168679_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168679_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168680_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168680_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:10.88 -30:00:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 4.153 5635319425356640896 137.54402496726 -30.00225533936 10.9900 10.5806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168684_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168684_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 168692_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168692_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168695_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168695_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 168702_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168702_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 168706_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168706_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:41.54 -27:08:13.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 168709_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168709_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 168717_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168717_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 168723_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168723_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:26.90 -21:11:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 0.162 5703533642139256192 128.61205821947 -21.18909383332 13.3603 12.6888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168726_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168726_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 168730_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168730_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168731_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168731_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 168733_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168733_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:16:41.95 -27:52:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.317 5693034405615061248 124.17438218662 -27.87955995049 13.1875 12.7405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168741_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168741_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168748_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168748_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 168749_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168749_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 168751_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168751_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168753_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168753_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:39.82 -29:52:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.050 5635377866972608128 137.16713869774 -29.86912782331 11.4644 10.6596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168754_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168754_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:28.57 -26:05:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 4.772 5650123559148894208 136.61862015858 -26.08571477115 12.0536 11.6648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168761_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168761_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:09:24.12 -26:43:44.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)
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Considering the candidate 168766_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168766_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 168777_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168777_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 168787_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168787_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168798_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168798_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168799_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168799_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168804_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168804_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168806_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168806_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:30.61 -30:05:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.163 5634925834553209600 138.12723934521 -30.08322732005 10.9970 10.6392 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168807_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168807_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:49.01 -21:26:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.289 5702963334903497344 128.70383526996 -21.44530169414 13.4076 12.8166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168809_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168809_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 168811_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168811_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168812_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168812_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:22.11 -22:25:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.100 5651946407692552960 138.09274542941 -22.43111489692 11.7051 10.9013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168814_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168814_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:45:55.22 -27:09:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.671 5646073130117339392 131.48087021449 -27.16016231993 13.0884 10.7091 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168815_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168815_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:29.35 -24:45:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.875 5650324009565305856 137.87110820782 -24.75575523877 11.7942 11.1295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168825_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168825_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168833_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168833_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168836_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168836_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:04.22 -22:02:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.461 5655019748850077568 137.76621780058 -22.04714178725 11.9928 11.6696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168838_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168838_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 168841_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168841_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:17:09.77 -22:39:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.974 5699775202162775936 124.29082881241 -22.66129072046 13.4069 12.9028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168842_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168842_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:07:14.07 -21:16:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.805 5700949721100441216 121.80865167786 -21.27613961885 13.5807 12.8023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168845_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168845_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168851_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168851_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168857_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168857_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168863_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168863_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168866_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168866_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 168871_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168871_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168877_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168877_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 168878_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168878_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 168880_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168880_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168890_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168890_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 168892_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168892_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168896_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168896_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168897_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168897_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 168901_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168901_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 168902_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168902_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:09.44 -30:25:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.074 5635277815713646592 137.04054241982 -30.43263503573 11.4877 11.1178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168904_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168904_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 168913_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168913_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168917_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168917_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 168919_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168919_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168920_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168920_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168921_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168921_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:20:20.33 -27:11:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.314 5693536538832456704 125.08542950580 -27.19418219439 13.3992 12.7062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168922_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168922_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 168924_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168924_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168927_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168927_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 168929_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168929_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 168939_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168939_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 168941_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168941_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 168944_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168944_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:08:28.75 -22:23:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.836 5700558947797749888 122.11988441068 -22.38672507473 13.0082 12.6812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168945_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168945_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168951_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168951_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 168957_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168957_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:21.34 -22:30:58.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)
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Considering the candidate 168959_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168959_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 168960_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 168960_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 168973_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168973_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:07:35.40 -21:49:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.446 5700780636828233216 121.89820876943 -21.82519762950 13.2507 12.7752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168980_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168980_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 168981_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168981_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:24.51 -31:05:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 4.915 5629202945254818432 135.60318974339 -31.09434950980 11.5805 10.8353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168982_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168982_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:06.49 -30:09:57.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 168988_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168988_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:33.51 -24:49:03.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)
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Considering the candidate 168991_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168991_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 168992_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 168992_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 169006_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169006_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 169009_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169009_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:48.45 -24:20:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.640 5651465371354931328 137.95079002982 -24.33481499482 11.8251 11.2611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169011_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169011_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:49.76 -21:34:40.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
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Considering the candidate 169016_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169016_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 169019_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169019_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 169023_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169023_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:08.96 -22:30:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.098 5651944075526043392 138.03715439912 -22.51093805158 11.9180 11.2388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169027_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169027_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:17.60 -24:29:03.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)
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Considering the candidate 169029_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169029_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:06.38 -21:57:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.791 5679040435784272128 137.77592855229 -21.95001826515 11.8809 11.1615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169033_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169033_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 169041_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169041_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169044_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169044_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 169053_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169053_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169055_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169055_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:28.23 -21:46:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.995 5679058062330049920 137.61751131494 -21.77378408136 11.8962 11.1397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169057_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169057_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169059_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169059_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169060_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169060_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169073_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169073_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 169077_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169077_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 169084_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169084_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169087_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169087_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:35.73 -21:49:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.262 5679056928458685824 137.64832366406 -21.81835755404 11.9747 11.2614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169088_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169088_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 169098_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169098_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:04.07 -22:07:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.948 5655015385163307776 137.51614769449 -22.11868816184 12.1843 11.7158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169106_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169106_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169107_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169107_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169109_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169109_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:03.38 -22:09:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.903 5655011953485743488 137.51359451191 -22.16519518562 12.0941 11.6505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169117_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169117_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:57.14 -21:14:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 2.467 5679100668405613312 137.98764752528 -21.23580917167 11.8607 11.1728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169118_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169118_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:19.33 -23:26:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.427 5651672152556473856 138.07993943628 -23.43441916327 11.6449 11.0475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169123_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169123_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 169129_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169129_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169131_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169131_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169138_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169138_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169139_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169139_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:07.66 -21:29:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.673 5679092456428171392 138.03253784056 -21.49736711245 11.4782 10.7042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169154_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169154_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 169155_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169155_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:03:45.60 -26:48:54.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
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Considering the candidate 169173_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169173_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 169178_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169178_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169180_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169180_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:07:09.10 -22:02:55.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 169181_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169181_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:04:20.04 -30:43:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.584 5635207893648770048 136.08447878301 -30.72200428549 11.8566 11.0039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169204_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169204_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 169205_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169205_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 169207_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169207_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:53.64 -30:03:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.615 5635324128341812608 137.22521477447 -30.06570202707 11.5769 10.7489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169208_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169208_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 169217_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169217_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 169221_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169221_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 169224_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169224_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169226_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169226_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:52.25 -24:19:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.785 5651465405714138112 137.96718546184 -24.32227613644 12.0387 11.5670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169229_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169229_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169231_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169231_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169232_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169232_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 169235_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169235_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:07:52.17 -21:09:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.229 5700957177163635456 121.96779098333 -21.16416985784 13.1788 12.8069 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 169238_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169238_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169244_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169244_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:57.63 -22:32:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.384 5651938023916395520 137.99022366293 -22.54940588294 11.8973 11.1416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169250_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169250_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 169251_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169251_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 169255_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169255_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:54.22 -22:01:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.130 5676035985902411648 137.97620724939 -22.02953332178 12.1133 11.5894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169267_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169267_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169271_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169271_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:21:02.91 -22:57:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.889 5699883332258044032 125.26219524732 -22.95557640468 13.7084 13.2919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169280_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169280_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169281_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169281_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169286_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169286_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169296_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169296_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:22:53.01 -23:28:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.950 5696804253024114176 125.72037317163 -23.48000800456 14.5002 14.0347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169299_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169299_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 169301_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169301_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:33.39 -22:00:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 5.820 5676036608673457024 137.88779670261 -22.01346403801 12.1480 11.7072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169306_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169306_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 169311_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169311_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 169317_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169317_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 169318_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169318_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169333_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169333_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 169349_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169349_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 169353_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169353_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:01:47.78 -29:55:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.807 5597049205176123904 120.45059702695 -29.91938794637 12.8452 12.6490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169356_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169356_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 169357_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169357_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:45.56 -21:19:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.864 5679136265095504896 137.43869150837 -21.33130009988 12.2226 11.7915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169360_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169360_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 169370_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169370_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 169371_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169371_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:07:35.52 -21:21:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.571 5655303942542234112 136.89776091579 -21.35160550613 12.3557 11.8717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169379_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169379_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:10:09.13 -25:44:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.883 5697625485133583232 122.53838714333 -25.73571005552 13.9827 13.6450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169380_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169380_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169381_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169381_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 169383_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169383_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:11:53.79 -21:31:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.053 5679091979688355584 137.97427464370 -21.52503021836 11.9361 11.2380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169387_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169387_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169397_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169397_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:19:13.52 -23:48:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.171 5696448767172972160 124.80663118668 -23.81609356635 13.8169 13.3263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169400_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169400_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169427_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169427_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:20:33.07 -20:37:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.701 5707188590591191680 125.13768469052 -20.62413923189 13.4626 12.6580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169436_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169436_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:08:44.96 -21:39:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.386 5655093725367417472 137.18677979459 -21.66261233987 12.2734 11.8129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169446_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169446_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 169448_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169448_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 169454_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169454_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 169472_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169472_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 169475_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169475_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:19:49.70 -21:46:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.773 5700309427373834240 124.95706628077 -21.76924211807 14.0174 13.5662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169476_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169476_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 169481_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169481_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:23.40 -21:34:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.797 5655271781827177984 136.59662038537 -21.57244253380 12.2752 11.6395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169494_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169494_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169496_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169496_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 169502_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169502_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:12:30.51 -22:58:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.690 5651888786411322752 138.12760054896 -22.96969699806 12.1439 11.3769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169504_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169504_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 169512_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169512_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 169532_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169532_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169535_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169535_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169553_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169553_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 169571_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169571_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 169572_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169572_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169574_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169574_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:09:31.24 -22:37:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 3.002 5700537335522235392 122.37989046720 -22.62104402547 13.7692 13.2080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169575_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169575_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 169577_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169577_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 169595_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169595_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 169598_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169598_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169601_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169601_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169602_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169602_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169607_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169607_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 169610_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169610_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:27.43 -21:19:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.851 5679125269979226752 137.61460568049 -21.32210504529 12.2271 11.7853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169621_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169621_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 169629_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169629_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:06.65 -21:43:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 5.669 5703124967411646080 127.77789760065 -21.72503708739 14.1526 13.7534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169659_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169659_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 169673_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169673_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 169683_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169683_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:22:23.14 -22:12:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 0.729 5700082000261576576 125.59637114485 -22.21169809497 13.9217 13.4485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169686_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169686_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 169689_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169689_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169697_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169697_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 169720_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169720_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:12:49.71 -22:29:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.292 5700580834944488704 123.20710475823 -22.48474566852 13.9616 13.4575 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#
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Considering the candidate 169723_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169723_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 169738_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169738_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 169749_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169749_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:58.71 -24:20:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 5.670 5651474511045337344 137.74306597731 -24.34173621968 12.1421 11.6609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169754_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169754_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 169770_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169770_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:56.43 -21:47:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.696 5679045628401447552 137.73520645817 -21.79590541582 12.2544 11.5501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169781_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169781_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 169806_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169806_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:14:07.78 -23:58:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.139 5699389548460866944 123.53238099145 -23.97393444561 14.1243 13.1568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169807_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169807_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:16.50 -20:52:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 2.357 5701316923622573696 123.31817192118 -20.87778652345 14.0116 13.3012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169809_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169809_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:10:49.98 -21:12:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.845 5679150352588230912 137.70954918233 -21.21755359892 11.6191 11.1159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169811_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169811_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169823_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169823_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169829_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169829_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:18:07.62 -21:23:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.755 5700383369531856384 124.53193124767 -21.39195727437 14.0252 13.4596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169833_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169833_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 169843_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169843_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 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 169852_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169852_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:01:48.41 -29:53:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.033 5597049578827249024 120.45235208432 -29.89182540650 12.9035 12.6141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169854_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169854_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:14.63 -22:49:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.244 5699802827393513728 123.31108829870 -22.83208393690 14.0545 13.6915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169884_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 169884_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 169898_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169898_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 169941_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169941_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 169963_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169963_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 169976_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169976_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:09:42.27 -22:16:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 5.732 5655009342145645696 137.42543505267 -22.27984761917 12.4523 11.9770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169987_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 169987_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 24770_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 24770_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:04:06.58 -29:08:32.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)
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Considering the candidate 127246_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 127246_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 07553_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 07553_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 78474_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 78474_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 143215_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 143215_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:24:25.94 -24:21:25.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 94523_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 94523_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 140651_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 140651_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 90070_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 90070_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:05:04.14 -25:05:22.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 88013_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 88013_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 08759_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 08759_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 29635_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 29635_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 58042_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 58042_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 57098_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 57098_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 144684_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 144684_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 96445_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 96445_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 88573_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 88573_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 99495_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 99495_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 93813_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 93813_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 75316_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 75316_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 27532_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 27532_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 144141_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 144141_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 112079_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 112079_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 40361_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 40361_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 87904_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 87904_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164109_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 164109_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:30:12.05 -26:04:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 0.706 5694983908448867584 127.55012392121 -26.06904124884 12.1806 10.6867 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 13209_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 13209_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:37.49 -30:16:49.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 128600_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 128600_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 09006_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 09006_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:15:13.84 -30:25:34.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 105050_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 105050_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:01.29 -21:47:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 1.212 5703124039696786048 127.75568267008 -21.79368292356 10.3215 9.1654 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65346_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 65346_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 33286_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 33286_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 140292_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 140292_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 89384_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 89384_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 33663_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 33663_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 155942_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 155942_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:02.89 -29:51:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.599 5643815416127482112 128.26249732803 -29.85860279865 12.3874 11.0208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134108_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 134108_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:25:42.72 -23:37:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.366 5696617507848538880 126.42791966344 -23.62054110124 12.4670 10.9352 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50735_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 50735_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 117603_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 117603_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 47466_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 47466_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
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Considering the candidate 69357_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 69357_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67582_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 67582_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98405_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 98405_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 47190_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 47190_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 127311_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 127311_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58110_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 58110_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70961_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 70961_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112308_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 112308_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73404_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
The candidate 73404_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:24.20 -26:16:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 5.769 5646936899584749952 127.85260372223 -26.27850390584 13.0998 12.8036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65243_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 65243_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22407_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
Preparing report for the candidate 22407_Pyx-01-Q2b1x1_2026-02-21_20-32-07_20.00sec_-14.90C_LIGHT_0015
make_report_in_HTML.sh Phase 2 (HTML assembly): 88s
make_report_in_HTML.sh TOTAL: 772s
Prepared the HTML report for the field Pyx-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:33:37.49 -30:16:49.5
09:05:04.25 -25:05:21.8
08:24:25.94 -24:21:25.3
09:08:54.45 -24:08:34.9
09:10:28.13 -23:17:23.2
09:08:48.30 -26:25:20.0
09:08:47.12 -25:21:12.4
09:09:45.66 -27:00:52.5
09:06:10.27 -30:59:27.2
09:11:49.74 -22:13:56.6
09:08:59.86 -30:23:58.2
09:07:47.54 -29:57:09.4
09:06:48.27 -30:36:46.3
09:09:19.54 -23:32:20.3
09:11:47.17 -24:43:28.8
08:40:58.30 -23:27:03.0
09:10:50.09 -23:28:10.1
09:11:28.93 -30:14:13.7
08:15:13.73 -30:25:32.3
09:00:31.59 -25:43:16.2
08:34:29.42 -30:43:12.5
08:29:22.63 -30:36:43.9
09:09:27.92 -22:13:13.1
08:29:15.53 -22:36:10.4
09:05:51.54 -24:34:34.6
08:10:21.18 -23:00:47.6
08:35:58.85 -24:31:44.1
08:19:04.78 -24:02:11.5
08:48:57.46 -24:12:27.3
08:37:22.53 -24:29:20.0
09:04:39.67 -22:12:42.3
09:08:17.56 -22:33:32.5
09:03:32.72 -30:43:56.1
08:03:08.94 -30:12:59.6
09:03:25.60 -21:34:00.1
09:03:16.09 -22:25:07.6
09:08:53.27 -27:49:48.4
09:05:39.81 -22:50:17.9
09:08:24.57 -25:08:46.7
09:08:51.21 -24:26:52.8
09:06:56.51 -26:03:54.9
09:05:03.04 -30:24:57.1
09:04:41.48 -21:29:06.2
08:49:02.67 -26:34:04.2
08:51:35.56 -30:05:21.3
09:04:00.80 -22:04:46.7
09:03:43.39 -26:39:29.7
09:02:27.14 -21:22:11.9
09:08:50.98 -23:43:44.3
09:06:24.33 -21:29:19.7
09:10:53.24 -21:44:08.1
09:08:48.77 -26:25:21.9
09:03:58.06 -29:46:09.4
09:05:53.23 -24:45:40.8
09:10:25.71 -29:41:27.1
09:09:48.78 -21:42:07.9
09:09:46.25 -27:00:56.4
09:12:05.90 -28:29:09.8
09:08:56.41 -22:23:23.5
09:10:14.41 -26:31:16.2
09:10:31.78 -29:44:06.1
09:10:51.23 -29:40:12.2
09:09:20.14 -23:46:23.0
09:12:08.45 -28:14:18.9
09:12:16.59 -23:52:49.5
09:11:31.31 -28:08:30.1
09:06:38.77 -22:21:59.1
09:10:35.80 -22:32:49.8
09:11:36.22 -27:45:46.9
08:47:38.91 -28:22:08.9
09:06:48.78 -27:20:24.9
09:06:32.19 -24:45:06.2
09:07:03.26 -26:49:35.7
09:07:53.25 -26:27:02.9
09:08:05.80 -29:01:46.8
09:10:24.74 -27:07:23.8
09:03:37.20 -21:29:03.4
09:08:11.83 -24:35:02.3
09:10:14.50 -29:45:07.9
09:10:50.42 -23:28:06.3
09:08:56.17 -21:24:19.9
09:06:28.01 -25:39:28.1
09:08:55.33 -27:27:36.7
09:10:56.07 -22:03:38.8
09:11:21.31 -23:59:38.2
09:12:16.76 -22:45:52.7
09:08:40.94 -22:05:45.3
09:10:33.15 -22:26:26.5
09:04:14.69 -21:26:46.2
09:05:53.74 -29:11:21.4
09:07:23.80 -31:06:47.9
09:12:20.13 -29:47:54.1
09:08:06.33 -29:40:44.4
09:11:48.09 -24:58:00.1
09:08:10.98 -29:56:02.5
09:08:58.79 -30:23:55.5
09:11:54.01 -22:10:14.2
09:09:49.25 -22:58:42.0
09:09:21.06 -25:53:25.9
09:08:12.59 -26:40:44.5
09:11:06.94 -27:50:55.7
09:05:10.96 -21:21:30.8
09:09:48.69 -29:42:33.4
09:04:52.71 -30:04:08.3
09:09:42.79 -29:26:29.6
09:11:10.25 -30:08:57.2
09:11:12.53 -24:31:13.9
09:10:53.62 -22:09:26.7
09:11:42.14 -22:51:43.0
09:10:26.74 -24:50:45.0
09:00:58.49 -31:13:07.4
09:04:17.90 -21:43:34.0
09:05:03.80 -26:38:49.0
09:11:26.14 -24:42:59.9
09:10:35.06 -23:20:36.4
09:07:21.40 -26:57:41.5
09:10:14.77 -30:25:45.1
09:09:16.78 -28:38:16.7
09:07:22.60 -31:06:42.5
09:12:18.81 -29:47:52.8
09:02:38.01 -30:57:43.0
09:10:25.49 -30:30:23.2
09:12:22.19 -24:15:43.0
09:04:14.12 -29:29:36.0
09:09:58.84 -28:58:44.9
09:11:33.73 -22:28:15.9
09:11:09.08 -24:27:13.5
09:05:32.15 -28:25:49.8
09:08:30.00 -24:12:05.3
09:05:53.38 -29:12:04.9
09:09:06.49 -29:44:29.3
09:06:11.50 -22:09:10.8
09:08:21.44 -24:36:45.5
09:09:31.50 -21:51:06.3
09:08:06.50 -27:30:22.4
09:09:28.31 -27:33:27.2
09:11:46.37 -28:32:15.6
09:08:09.66 -29:56:02.1
09:04:39.69 -30:23:09.8
09:06:17.96 -22:23:56.3
09:09:22.70 -23:43:53.1
09:06:31.48 -21:59:03.9
09:08:15.67 -22:00:11.5
09:08:42.70 -22:26:12.6
09:08:31.98 -21:20:37.8
09:12:33.46 -28:39:03.0
09:10:11.27 -25:03:40.8
09:07:19.50 -26:24:45.8
09:12:03.72 -26:37:10.9
09:06:19.59 -28:00:29.7
09:11:50.17 -30:05:06.4
09:09:39.58 -29:31:57.6
09:12:08.25 -27:37:51.8
09:07:37.42 -24:33:31.4
09:11:13.28 -29:30:45.7
09:03:06.31 -30:45:44.0
09:12:05.84 -24:44:52.9
09:10:05.03 -26:04:16.3
09:07:33.85 -29:37:44.0
09:11:23.69 -25:56:31.6
09:11:12.33 -24:08:18.9
09:11:12.23 -29:30:45.0
09:05:22.89 -29:20:30.3
09:10:17.90 -23:54:34.1
09:09:49.58 -28:30:36.8
09:10:01.18 -24:50:18.5
09:09:27.92 -30:06:00.5
09:10:19.31 -21:58:44.2
08:17:06.82 -27:27:30.8
09:07:22.22 -22:46:02.6
09:03:27.92 -30:29:23.3
09:11:58.12 -27:26:51.6
09:06:21.42 -22:39:19.3
09:10:47.56 -30:16:05.6
09:12:22.29 -23:39:25.7
09:12:03.14 -26:38:24.3
09:10:57.33 -21:23:37.1
09:11:09.45 -24:40:26.0
09:08:39.76 -22:08:38.5
09:07:08.36 -27:06:43.4
09:07:49.84 -28:18:59.7
09:08:29.08 -21:57:10.8
09:10:01.17 -27:05:19.3
09:10:05.20 -24:20:58.9
09:11:08.42 -29:35:09.5
09:07:54.05 -22:55:45.2
09:11:37.77 -22:49:50.5
09:10:49.09 -30:16:00.4
09:08:46.82 -30:00:32.1
09:11:43.52 -24:19:09.7
09:06:52.33 -21:49:37.1
09:10:36.38 -28:34:25.6
09:08:09.37 -27:26:02.5
09:09:18.91 -24:40:29.2
09:08:40.28 -24:07:51.5
09:09:47.86 -22:42:02.0
09:07:49.13 -28:19:05.4
09:07:34.45 -28:57:26.1
09:11:39.06 -23:55:03.8
09:06:17.68 -21:25:57.7
09:07:16.37 -25:06:46.5
09:11:09.47 -29:35:05.7
09:06:37.37 -21:35:58.5
09:11:37.95 -24:00:31.1
09:10:41.65 -29:35:41.6
09:12:02.94 -28:13:49.5
09:05:57.65 -21:38:24.9
09:11:22.72 -27:36:11.5
09:09:28.17 -28:04:28.5
09:10:21.37 -24:31:04.3
09:11:46.62 -27:54:12.7
09:12:29.40 -25:12:25.5
09:08:47.22 -27:46:01.5
09:07:22.24 -22:30:03.1
09:09:26.75 -22:01:53.3
09:06:48.13 -24:12:21.7
09:04:31.61 -21:45:36.3
09:11:20.09 -23:26:36.2
09:07:12.93 -27:57:07.2
09:10:52.58 -28:49:01.2
09:12:05.95 -21:30:48.2
09:09:21.36 -24:00:03.9
09:11:39.59 -26:15:29.8
09:12:03.02 -21:38:46.1
09:10:22.11 -29:44:19.0
09:07:30.48 -21:16:18.3
09:11:46.87 -26:49:33.8
09:12:21.66 -24:01:52.1
09:07:21.58 -22:36:33.0
09:07:33.60 -22:45:43.9
09:11:02.65 -21:29:55.2
09:10:48.31 -30:49:37.3
09:11:21.03 -28:06:10.0
09:12:23.41 -23:28:38.0
09:11:37.16 -28:16:46.5
09:09:47.56 -22:01:56.6
09:10:50.50 -21:24:28.2
09:10:12.11 -25:33:49.8
09:08:33.17 -26:17:28.5
09:06:25.04 -31:06:00.9
09:11:17.88 -23:42:55.7
09:05:28.38 -21:27:56.9
09:06:31.11 -21:49:54.4
09:09:21.84 -30:12:01.2
09:10:27.01 -30:05:26.6
09:10:17.71 -24:52:39.5
08:21:53.01 -22:58:16.5
09:10:36.14 -28:41:34.3
08:20:48.01 -25:07:07.9
09:09:57.07 -27:27:45.8
09:05:06.37 -21:42:27.8
09:10:00.91 -21:37:30.3
09:11:52.61 -28:46:38.4
09:09:36.88 -30:28:53.4
09:07:21.51 -22:23:28.5
09:12:09.87 -27:10:10.1
09:11:23.82 -27:14:20.1
09:07:05.65 -21:42:02.5
09:01:02.88 -30:48:10.4
09:10:21.37 -21:19:32.0
09:12:31.33 -30:04:57.4
09:07:00.42 -22:30:41.7
09:11:27.03 -28:29:50.1
09:09:10.61 -21:23:31.3
09:09:57.60 -22:06:02.1
09:08:38.99 -26:25:39.8
09:12:09.52 -23:29:24.1
09:12:38.77 -25:43:25.2
09:10:58.88 -23:28:10.9
09:11:59.34 -22:44:00.2
09:09:59.19 -27:17:05.0
09:12:02.46 -25:51:56.1
09:09:18.45 -22:42:04.1
09:05:31.01 -30:47:46.7
09:09:37.97 -27:11:43.4
09:04:44.89 -21:12:30.4
09:10:04.50 -26:35:36.7
09:05:20.01 -21:17:41.9
09:04:56.03 -21:51:33.7
09:10:28.42 -22:39:58.6
09:08:15.82 -21:12:21.0
09:08:06.35 -30:38:10.8
09:09:03.28 -29:34:55.9
09:08:50.43 -21:34:53.3
09:11:27.87 -23:21:17.5
09:10:58.71 -29:37:13.0
09:12:11.65 -21:28:49.3
09:10:26.21 -30:54:21.1
09:11:24.85 -22:38:56.8
09:10:26.55 -22:48:42.1
09:10:07.04 -21:36:06.3
09:11:02.03 -21:21:29.4
09:10:47.80 -22:39:12.6
09:11:12.34 -21:43:32.2
09:12:35.14 -26:10:33.3
09:12:20.94 -24:57:10.7
09:11:05.09 -23:33:12.0
09:12:18.84 -21:57:08.9
09:04:24.68 -21:24:20.2
08:37:58.80 -29:42:27.2
08:25:43.23 -29:15:44.0
08:51:36.33 -29:11:13.0
08:32:04.46 -28:53:28.6
08:29:15.97 -27:56:36.9
08:31:54.30 -27:44:27.4
08:28:13.68 -27:18:33.3
08:35:26.51 -27:16:12.0
08:32:00.66 -27:15:32.4
08:34:38.18 -26:48:42.5
08:30:54.36 -26:46:59.4
08:39:42.97 -26:40:47.4
08:11:33.44 -26:19:02.2
08:20:07.68 -26:16:33.5
08:17:49.58 -26:00:48.5
08:20:08.99 -25:51:06.1
08:30:14.43 -25:18:28.9
08:35:39.23 -25:18:49.1
08:52:42.62 -25:14:45.8
08:41:32.52 -24:57:41.9
08:32:03.72 -24:51:17.2
09:04:07.07 -21:16:19.1
########### Completed Pyx-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 ####
09:08:54.45 -24:08:34.9
09:10:28.13 -23:17:23.2
09:08:48.30 -26:25:20.0
09:08:47.12 -25:21:12.4
09:09:45.66 -27:00:52.5
09:06:10.27 -30:59:27.2
09:11:49.74 -22:13:56.6
09:08:59.86 -30:23:58.2
09:07:47.54 -29:57:09.4
09:06:48.27 -30:36:46.3
09:09:19.54 -23:32:20.3
09:11:47.17 -24:43:28.8
08:40:58.30 -23:27:03.0
09:10:50.09 -23:28:10.1
09:11:28.93 -30:14:13.7
08:15:13.73 -30:25:32.3
09:00:31.59 -25:43:16.2
09:05:04.25 -25:05:21.8
08:33:37.49 -30:16:49.5
08:24:25.94 -24:21:25.3
09:04:39.67 -22:12:42.3
09:08:17.56 -22:33:32.5
09:03:32.72 -30:43:56.1
08:03:08.94 -30:12:59.6
09:03:25.60 -21:34:00.1
09:03:16.09 -22:25:07.6
09:08:53.27 -27:49:48.4
09:05:39.81 -22:50:17.9
09:08:24.57 -25:08:46.7
09:08:51.21 -24:26:52.8
09:06:56.51 -26:03:54.9
09:05:03.04 -30:24:57.1
09:04:41.48 -21:29:06.2
08:49:02.67 -26:34:04.2
08:51:35.56 -30:05:21.3
09:04:00.80 -22:04:46.7
09:03:43.39 -26:39:29.7
09:02:27.14 -21:22:11.9
09:08:50.98 -23:43:44.3
09:06:24.33 -21:29:19.7
09:10:53.24 -21:44:08.1
09:08:48.77 -26:25:21.9
09:03:58.06 -29:46:09.4
09:05:53.23 -24:45:40.8
09:10:25.71 -29:41:27.1
09:09:48.78 -21:42:07.9
09:09:46.25 -27:00:56.4
09:12:05.90 -28:29:09.8
09:08:56.41 -22:23:23.5
09:10:14.41 -26:31:16.2
09:10:31.78 -29:44:06.1
09:10:51.23 -29:40:12.2
09:09:20.14 -23:46:23.0
09:12:08.45 -28:14:18.9
09:12:16.59 -23:52:49.5
09:11:31.31 -28:08:30.1
09:06:38.77 -22:21:59.1
09:10:35.80 -22:32:49.8
09:11:36.22 -27:45:46.9
08:47:38.91 -28:22:08.9
09:06:48.78 -27:20:24.9
09:06:32.19 -24:45:06.2
09:07:03.26 -26:49:35.7
09:07:53.25 -26:27:02.9
09:08:05.80 -29:01:46.8
09:10:24.74 -27:07:23.8
09:03:37.20 -21:29:03.4
09:08:11.83 -24:35:02.3
09:10:14.50 -29:45:07.9
09:10:50.42 -23:28:06.3
09:08:56.17 -21:24:19.9
09:06:28.01 -25:39:28.1
09:08:55.33 -27:27:36.7
09:10:56.07 -22:03:38.8
09:11:21.31 -23:59:38.2
09:12:16.76 -22:45:52.7
09:08:40.94 -22:05:45.3
09:10:33.15 -22:26:26.5
09:04:14.69 -21:26:46.2
09:05:53.74 -29:11:21.4
09:07:23.80 -31:06:47.9
09:12:20.13 -29:47:54.1
09:08:06.33 -29:40:44.4
09:11:48.09 -24:58:00.1
09:08:10.98 -29:56:02.5
09:08:58.79 -30:23:55.5
09:11:54.01 -22:10:14.2
09:09:49.25 -22:58:42.0
09:09:21.06 -25:53:25.9
09:08:12.59 -26:40:44.5
09:11:06.94 -27:50:55.7
09:05:10.96 -21:21:30.8
09:09:48.69 -29:42:33.4
09:04:52.71 -30:04:08.3
09:09:42.79 -29:26:29.6
09:11:10.25 -30:08:57.2
09:11:12.53 -24:31:13.9
09:10:53.62 -22:09:26.7
09:11:42.14 -22:51:43.0
09:10:26.74 -24:50:45.0
09:00:58.49 -31:13:07.4
09:04:17.90 -21:43:34.0
09:05:03.80 -26:38:49.0
09:11:26.14 -24:42:59.9
09:10:35.06 -23:20:36.4
09:07:21.40 -26:57:41.5
09:10:14.77 -30:25:45.1
09:09:16.78 -28:38:16.7
09:07:22.60 -31:06:42.5
09:12:18.81 -29:47:52.8
09:02:38.01 -30:57:43.0
09:10:25.49 -30:30:23.2
09:12:22.19 -24:15:43.0
09:04:14.12 -29:29:36.0
09:09:58.84 -28:58:44.9
09:11:33.73 -22:28:15.9
09:11:09.08 -24:27:13.5
09:05:32.15 -28:25:49.8
09:08:30.00 -24:12:05.3
09:05:53.38 -29:12:04.9
09:09:06.49 -29:44:29.3
09:06:11.50 -22:09:10.8
09:08:21.44 -24:36:45.5
09:09:31.50 -21:51:06.3
09:08:06.50 -27:30:22.4
09:09:28.31 -27:33:27.2
09:11:46.37 -28:32:15.6
09:08:09.66 -29:56:02.1
09:04:39.69 -30:23:09.8
09:06:17.96 -22:23:56.3
09:09:22.70 -23:43:53.1
09:06:31.48 -21:59:03.9
09:08:15.67 -22:00:11.5
09:08:42.70 -22:26:12.6
09:08:31.98 -21:20:37.8
09:12:33.46 -28:39:03.0
09:10:11.27 -25:03:40.8
09:07:19.50 -26:24:45.8
09:12:03.72 -26:37:10.9
09:06:19.59 -28:00:29.7
09:11:50.17 -30:05:06.4
09:09:39.58 -29:31:57.6
09:12:08.25 -27:37:51.8
09:07:37.42 -24:33:31.4
09:11:13.28 -29:30:45.7
09:03:06.31 -30:45:44.0
09:12:05.84 -24:44:52.9
09:10:05.03 -26:04:16.3
09:07:33.85 -29:37:44.0
09:11:23.69 -25:56:31.6
09:11:12.33 -24:08:18.9
09:11:12.23 -29:30:45.0
09:05:22.89 -29:20:30.3
09:10:17.90 -23:54:34.1
09:09:49.58 -28:30:36.8
09:10:01.18 -24:50:18.5
09:09:27.92 -30:06:00.5
09:10:19.31 -21:58:44.2
08:17:06.82 -27:27:30.8
09:07:22.22 -22:46:02.6
09:03:27.92 -30:29:23.3
09:11:58.12 -27:26:51.6
09:06:21.42 -22:39:19.3
09:10:47.56 -30:16:05.6
09:12:22.29 -23:39:25.7
09:12:03.14 -26:38:24.3
09:10:57.33 -21:23:37.1
09:11:09.45 -24:40:26.0
09:08:39.76 -22:08:38.5
09:07:08.36 -27:06:43.4
09:07:49.84 -28:18:59.7
09:08:29.08 -21:57:10.8
09:10:01.17 -27:05:19.3
09:10:05.20 -24:20:58.9
09:11:08.42 -29:35:09.5
09:07:54.05 -22:55:45.2
09:11:37.77 -22:49:50.5
09:10:49.09 -30:16:00.4
09:08:46.82 -30:00:32.1
09:11:43.52 -24:19:09.7
09:06:52.33 -21:49:37.1
09:10:36.38 -28:34:25.6
09:08:09.37 -27:26:02.5
09:09:18.91 -24:40:29.2
09:08:40.28 -24:07:51.5
09:09:47.86 -22:42:02.0
09:07:49.13 -28:19:05.4
09:07:34.45 -28:57:26.1
09:11:39.06 -23:55:03.8
09:06:17.68 -21:25:57.7
09:07:16.37 -25:06:46.5
09:11:09.47 -29:35:05.7
09:06:37.37 -21:35:58.5
09:11:37.95 -24:00:31.1
09:10:41.65 -29:35:41.6
09:12:02.94 -28:13:49.5
09:05:57.65 -21:38:24.9
09:11:22.72 -27:36:11.5
09:09:28.17 -28:04:28.5
09:10:21.37 -24:31:04.3
09:11:46.62 -27:54:12.7
09:12:29.40 -25:12:25.5
09:08:47.22 -27:46:01.5
09:07:22.24 -22:30:03.1
09:09:26.75 -22:01:53.3
09:06:48.13 -24:12:21.7
09:04:31.61 -21:45:36.3
09:11:20.09 -23:26:36.2
09:07:12.93 -27:57:07.2
09:10:52.58 -28:49:01.2
09:12:05.95 -21:30:48.2
09:09:21.36 -24:00:03.9
09:11:39.59 -26:15:29.8
09:12:03.02 -21:38:46.1
09:10:22.11 -29:44:19.0
09:07:30.48 -21:16:18.3
09:11:46.87 -26:49:33.8
09:12:21.66 -24:01:52.1
09:07:21.58 -22:36:33.0
09:07:33.60 -22:45:43.9
09:11:02.65 -21:29:55.2
09:10:48.31 -30:49:37.3
09:11:21.03 -28:06:10.0
09:12:23.41 -23:28:38.0
09:11:37.16 -28:16:46.5
09:09:47.56 -22:01:56.6
09:10:50.50 -21:24:28.2
09:10:12.11 -25:33:49.8
09:08:33.17 -26:17:28.5
09:06:25.04 -31:06:00.9
09:11:17.88 -23:42:55.7
09:05:28.38 -21:27:56.9
09:06:31.11 -21:49:54.4
09:09:21.84 -30:12:01.2
09:10:27.01 -30:05:26.6
09:10:17.71 -24:52:39.5
08:21:53.01 -22:58:16.5
09:10:36.14 -28:41:34.3
08:20:48.01 -25:07:07.9
09:09:57.07 -27:27:45.8
09:05:06.37 -21:42:27.8
09:10:00.91 -21:37:30.3
09:11:52.61 -28:46:38.4
09:09:36.88 -30:28:53.4
09:07:21.51 -22:23:28.5
09:12:09.87 -27:10:10.1
09:11:23.82 -27:14:20.1
09:07:05.65 -21:42:02.5
09:01:02.88 -30:48:10.4
09:10:21.37 -21:19:32.0
09:12:31.33 -30:04:57.4
09:07:00.42 -22:30:41.7
09:11:27.03 -28:29:50.1
09:09:10.61 -21:23:31.3
09:09:57.60 -22:06:02.1
09:08:38.99 -26:25:39.8
09:12:09.52 -23:29:24.1
09:12:38.77 -25:43:25.2
09:10:58.88 -23:28:10.9
09:11:59.34 -22:44:00.2
09:09:59.19 -27:17:05.0
09:12:02.46 -25:51:56.1
09:09:18.45 -22:42:04.1
09:05:31.01 -30:47:46.7
09:09:37.97 -27:11:43.4
09:04:44.89 -21:12:30.4
09:10:04.50 -26:35:36.7
09:05:20.01 -21:17:41.9
09:04:56.03 -21:51:33.7
09:10:28.42 -22:39:58.6
09:08:15.82 -21:12:21.0
09:08:06.35 -30:38:10.8
09:09:03.28 -29:34:55.9
09:08:50.43 -21:34:53.3
09:11:27.87 -23:21:17.5
09:10:58.71 -29:37:13.0
09:12:11.65 -21:28:49.3
09:10:26.21 -30:54:21.1
09:11:24.85 -22:38:56.8
09:10:26.55 -22:48:42.1
09:10:07.04 -21:36:06.3
09:11:02.03 -21:21:29.4
09:10:47.80 -22:39:12.6
09:11:12.34 -21:43:32.2
09:12:35.14 -26:10:33.3
09:12:20.94 -24:57:10.7
09:11:05.09 -23:33:12.0
09:12:18.84 -21:57:08.9
09:04:24.68 -21:24:20.2
09:05:51.54 -24:34:34.6
08:34:29.42 -30:43:12.5
08:20:08.99 -25:51:06.1
08:32:03.72 -24:51:17.2
08:48:57.46 -24:12:27.3
08:35:39.23 -25:18:49.1
08:29:22.63 -30:36:43.9
08:51:36.33 -29:11:13.0
08:35:26.51 -27:16:12.0
08:28:13.68 -27:18:33.3
09:04:07.07 -21:16:19.1
08:41:32.52 -24:57:41.9
08:17:49.58 -26:00:48.5
08:25:43.23 -29:15:44.0
08:37:22.53 -24:29:20.0
08:30:14.43 -25:18:28.9
08:35:58.85 -24:31:44.1
08:30:54.36 -26:46:59.4
08:19:04.78 -24:02:11.5
08:52:42.62 -25:14:45.8
08:32:04.46 -28:53:28.6
08:31:54.30 -27:44:27.4
08:29:15.53 -22:36:10.4
08:29:15.97 -27:56:36.9
08:11:33.44 -26:19:02.2
08:39:42.97 -26:40:47.4
08:10:21.18 -23:00:47.6
08:32:00.66 -27:15:32.4
08:20:07.68 -26:16:33.5
09:09:27.92 -22:13:13.1
08:34:38.18 -26:48:42.5
08:37:58.80 -29:42:27.2
###################################################################################
09:08:54.45 -24:08:34.9 -- not an asteroid (will add it to exclusion list)
09:10:28.13 -23:17:23.2 -- not an asteroid (will add it to exclusion list)
09:08:48.30 -26:25:20.0 -- not an asteroid (will add it to exclusion list)
09:08:47.12 -25:21:12.4 -- not an asteroid (will add it to exclusion list)
09:09:45.66 -27:00:52.5 -- not an asteroid (will add it to exclusion list)
09:06:10.27 -30:59:27.2 -- not an asteroid (will add it to exclusion list)
09:11:49.74 -22:13:56.6 -- not an asteroid (will add it to exclusion list)
09:08:59.86 -30:23:58.2 -- not an asteroid (will add it to exclusion list)
09:07:47.54 -29:57:09.4 -- not an asteroid (will add it to exclusion list)
09:06:48.27 -30:36:46.3 -- not an asteroid (will add it to exclusion list)
09:09:19.54 -23:32:20.3 -- not an asteroid (will add it to exclusion list)
09:11:47.17 -24:43:28.8 -- not an asteroid (will add it to exclusion list)
08:40:58.30 -23:27:03.0 -- not an asteroid (will add it to exclusion list)
09:10:50.09 -23:28:10.1 -- not an asteroid (will add it to exclusion list)
09:11:28.93 -30:14:13.7 -- not an asteroid (will add it to exclusion list)
08:15:13.73 -30:25:32.3 -- not an asteroid (will add it to exclusion list)
09:00:31.59 -25:43:16.2 -- not an asteroid (will add it to exclusion list)
09:05:04.25 -25:05:21.8 -- not an asteroid (will add it to exclusion list)
08:33:37.49 -30:16:49.5 -- not an asteroid (will add it to exclusion list)
08:24:25.94 -24:21:25.3 -- not an asteroid (will add it to exclusion list)
09:04:39.67 -22:12:42.3 -- not an asteroid (will add it to exclusion list)
09:08:17.56 -22:33:32.5 -- not an asteroid (will add it to exclusion list)
09:03:32.72 -30:43:56.1 -- not an asteroid (will add it to exclusion list)
08:03:08.94 -30:12:59.6 -- not an asteroid (will add it to exclusion list)
09:03:25.60 -21:34:00.1 -- not an asteroid (will add it to exclusion list)
09:03:16.09 -22:25:07.6 -- not an asteroid (will add it to exclusion list)
09:08:53.27 -27:49:48.4 -- not an asteroid (will add it to exclusion list)
09:05:39.81 -22:50:17.9 -- not an asteroid (will add it to exclusion list)
09:08:24.57 -25:08:46.7 -- not an asteroid (will add it to exclusion list)
09:08:51.21 -24:26:52.8 -- not an asteroid (will add it to exclusion list)
09:06:56.51 -26:03:54.9 -- not an asteroid (will add it to exclusion list)
09:05:03.04 -30:24:57.1 -- not an asteroid (will add it to exclusion list)
09:04:41.48 -21:29:06.2 -- not an asteroid (will add it to exclusion list)
08:49:02.67 -26:34:04.2 -- not an asteroid (will add it to exclusion list)
08:51:35.56 -30:05:21.3 -- not an asteroid (will add it to exclusion list)
09:04:00.80 -22:04:46.7 -- not an asteroid (will add it to exclusion list)
09:03:43.39 -26:39:29.7 -- not an asteroid (will add it to exclusion list)
09:02:27.14 -21:22:11.9 -- not an asteroid (will add it to exclusion list)
09:08:50.98 -23:43:44.3 -- not an asteroid (will add it to exclusion list)
09:06:24.33 -21:29:19.7 -- not an asteroid (will add it to exclusion list)
09:10:53.24 -21:44:08.1 -- not an asteroid (will add it to exclusion list)
09:08:48.77 -26:25:21.9 -- not an asteroid (will add it to exclusion list)
09:03:58.06 -29:46:09.4 -- not an asteroid (will add it to exclusion list)
09:05:53.23 -24:45:40.8 -- not an asteroid (will add it to exclusion list)
09:10:25.71 -29:41:27.1 -- not an asteroid (will add it to exclusion list)
09:09:48.78 -21:42:07.9 -- not an asteroid (will add it to exclusion list)
09:09:46.25 -27:00:56.4 -- not an asteroid (will add it to exclusion list)
09:12:05.90 -28:29:09.8 -- not an asteroid (will add it to exclusion list)
09:08:56.41 -22:23:23.5 -- not an asteroid (will add it to exclusion list)
09:10:14.41 -26:31:16.2 -- not an asteroid (will add it to exclusion list)
09:10:31.78 -29:44:06.1 -- not an asteroid (will add it to exclusion list)
09:10:51.23 -29:40:12.2 -- not an asteroid (will add it to exclusion list)
09:09:20.14 -23:46:23.0 -- not an asteroid (will add it to exclusion list)
09:12:08.45 -28:14:18.9 -- not an asteroid (will add it to exclusion list)
09:12:16.59 -23:52:49.5 -- not an asteroid (will add it to exclusion list)
09:11:31.31 -28:08:30.1 -- not an asteroid (will add it to exclusion list)
09:06:38.77 -22:21:59.1 -- not an asteroid (will add it to exclusion list)
09:10:35.80 -22:32:49.8 -- not an asteroid (will add it to exclusion list)
09:11:36.22 -27:45:46.9 -- not an asteroid (will add it to exclusion list)
08:47:38.91 -28:22:08.9 -- not an asteroid (will add it to exclusion list)
09:06:48.78 -27:20:24.9 -- not an asteroid (will add it to exclusion list)
09:06:32.19 -24:45:06.2 -- not an asteroid (will add it to exclusion list)
09:07:03.26 -26:49:35.7 -- not an asteroid (will add it to exclusion list)
09:07:53.25 -26:27:02.9 -- not an asteroid (will add it to exclusion list)
09:08:05.80 -29:01:46.8 -- not an asteroid (will add it to exclusion list)
09:10:24.74 -27:07:23.8 -- not an asteroid (will add it to exclusion list)
09:03:37.20 -21:29:03.4 -- not an asteroid (will add it to exclusion list)
09:08:11.83 -24:35:02.3 -- not an asteroid (will add it to exclusion list)
09:10:14.50 -29:45:07.9 -- not an asteroid (will add it to exclusion list)
09:10:50.42 -23:28:06.3 -- not an asteroid (will add it to exclusion list)
09:08:56.17 -21:24:19.9 -- not an asteroid (will add it to exclusion list)
09:06:28.01 -25:39:28.1 -- not an asteroid (will add it to exclusion list)
09:08:55.33 -27:27:36.7 -- not an asteroid (will add it to exclusion list)
09:10:56.07 -22:03:38.8 -- not an asteroid (will add it to exclusion list)
09:11:21.31 -23:59:38.2 -- not an asteroid (will add it to exclusion list)
09:12:16.76 -22:45:52.7 -- not an asteroid (will add it to exclusion list)
09:08:40.94 -22:05:45.3 -- not an asteroid (will add it to exclusion list)
09:10:33.15 -22:26:26.5 -- not an asteroid (will add it to exclusion list)
09:04:14.69 -21:26:46.2 -- not an asteroid (will add it to exclusion list)
09:05:53.74 -29:11:21.4 -- not an asteroid (will add it to exclusion list)
09:07:23.80 -31:06:47.9 -- not an asteroid (will add it to exclusion list)
09:12:20.13 -29:47:54.1 -- not an asteroid (will add it to exclusion list)
09:08:06.33 -29:40:44.4 -- not an asteroid (will add it to exclusion list)
09:11:48.09 -24:58:00.1 -- not an asteroid (will add it to exclusion list)
09:08:10.98 -29:56:02.5 -- not an asteroid (will add it to exclusion list)
09:08:58.79 -30:23:55.5 -- not an asteroid (will add it to exclusion list)
09:11:54.01 -22:10:14.2 -- not an asteroid (will add it to exclusion list)
09:09:49.25 -22:58:42.0 -- not an asteroid (will add it to exclusion list)
09:09:21.06 -25:53:25.9 -- not an asteroid (will add it to exclusion list)
09:08:12.59 -26:40:44.5 -- not an asteroid (will add it to exclusion list)
09:11:06.94 -27:50:55.7 -- not an asteroid (will add it to exclusion list)
09:05:10.96 -21:21:30.8 -- not an asteroid (will add it to exclusion list)
09:09:48.69 -29:42:33.4 -- not an asteroid (will add it to exclusion list)
09:04:52.71 -30:04:08.3 -- not an asteroid (will add it to exclusion list)
09:09:42.79 -29:26:29.6 -- not an asteroid (will add it to exclusion list)
09:11:10.25 -30:08:57.2 -- not an asteroid (will add it to exclusion list)
09:11:12.53 -24:31:13.9 -- not an asteroid (will add it to exclusion list)
09:10:53.62 -22:09:26.7 -- not an asteroid (will add it to exclusion list)
09:11:42.14 -22:51:43.0 -- not an asteroid (will add it to exclusion list)
09:10:26.74 -24:50:45.0 -- not an asteroid (will add it to exclusion list)
09:00:58.49 -31:13:07.4 -- not an asteroid (will add it to exclusion list)
09:04:17.90 -21:43:34.0 -- not an asteroid (will add it to exclusion list)
09:05:03.80 -26:38:49.0 -- not an asteroid (will add it to exclusion list)
09:11:26.14 -24:42:59.9 -- not an asteroid (will add it to exclusion list)
09:10:35.06 -23:20:36.4 -- not an asteroid (will add it to exclusion list)
09:07:21.40 -26:57:41.5 -- not an asteroid (will add it to exclusion list)
09:10:14.77 -30:25:45.1 -- not an asteroid (will add it to exclusion list)
09:09:16.78 -28:38:16.7 -- not an asteroid (will add it to exclusion list)
09:07:22.60 -31:06:42.5 -- not an asteroid (will add it to exclusion list)
09:12:18.81 -29:47:52.8 -- not an asteroid (will add it to exclusion list)
09:02:38.01 -30:57:43.0 -- not an asteroid (will add it to exclusion list)
09:10:25.49 -30:30:23.2 -- not an asteroid (will add it to exclusion list)
09:12:22.19 -24:15:43.0 -- not an asteroid (will add it to exclusion list)
09:04:14.12 -29:29:36.0 -- not an asteroid (will add it to exclusion list)
09:09:58.84 -28:58:44.9 -- not an asteroid (will add it to exclusion list)
09:11:33.73 -22:28:15.9 -- not an asteroid (will add it to exclusion list)
09:11:09.08 -24:27:13.5 -- not an asteroid (will add it to exclusion list)
09:05:32.15 -28:25:49.8 -- not an asteroid (will add it to exclusion list)
09:08:30.00 -24:12:05.3 -- not an asteroid (will add it to exclusion list)
09:05:53.38 -29:12:04.9 -- not an asteroid (will add it to exclusion list)
09:09:06.49 -29:44:29.3 -- not an asteroid (will add it to exclusion list)
09:06:11.50 -22:09:10.8 -- not an asteroid (will add it to exclusion list)
09:08:21.44 -24:36:45.5 -- not an asteroid (will add it to exclusion list)
09:09:31.50 -21:51:06.3 -- not an asteroid (will add it to exclusion list)
09:08:06.50 -27:30:22.4 -- not an asteroid (will add it to exclusion list)
09:09:28.31 -27:33:27.2 -- not an asteroid (will add it to exclusion list)
09:11:46.37 -28:32:15.6 -- not an asteroid (will add it to exclusion list)
09:08:09.66 -29:56:02.1 -- not an asteroid (will add it to exclusion list)
09:04:39.69 -30:23:09.8 -- not an asteroid (will add it to exclusion list)
09:06:17.96 -22:23:56.3 -- not an asteroid (will add it to exclusion list)
09:09:22.70 -23:43:53.1 -- not an asteroid (will add it to exclusion list)
09:06:31.48 -21:59:03.9 -- not an asteroid (will add it to exclusion list)
09:08:15.67 -22:00:11.5 -- not an asteroid (will add it to exclusion list)
09:08:42.70 -22:26:12.6 -- not an asteroid (will add it to exclusion list)
09:08:31.98 -21:20:37.8 -- not an asteroid (will add it to exclusion list)
09:12:33.46 -28:39:03.0 -- not an asteroid (will add it to exclusion list)
09:10:11.27 -25:03:40.8 -- not an asteroid (will add it to exclusion list)
09:07:19.50 -26:24:45.8 -- not an asteroid (will add it to exclusion list)
09:12:03.72 -26:37:10.9 -- not an asteroid (will add it to exclusion list)
09:06:19.59 -28:00:29.7 -- not an asteroid (will add it to exclusion list)
09:11:50.17 -30:05:06.4 -- not an asteroid (will add it to exclusion list)
09:09:39.58 -29:31:57.6 -- not an asteroid (will add it to exclusion list)
09:12:08.25 -27:37:51.8 -- not an asteroid (will add it to exclusion list)
09:07:37.42 -24:33:31.4 -- not an asteroid (will add it to exclusion list)
09:11:13.28 -29:30:45.7 -- not an asteroid (will add it to exclusion list)
09:03:06.31 -30:45:44.0 -- not an asteroid (will add it to exclusion list)
09:12:05.84 -24:44:52.9 -- not an asteroid (will add it to exclusion list)
09:10:05.03 -26:04:16.3 -- not an asteroid (will add it to exclusion list)
09:07:33.85 -29:37:44.0 -- not an asteroid (will add it to exclusion list)
09:11:23.69 -25:56:31.6 -- not an asteroid (will add it to exclusion list)
09:11:12.33 -24:08:18.9 -- not an asteroid (will add it to exclusion list)
09:11:12.23 -29:30:45.0 -- not an asteroid (will add it to exclusion list)
09:05:22.89 -29:20:30.3 -- not an asteroid (will add it to exclusion list)
09:10:17.90 -23:54:34.1 -- not an asteroid (will add it to exclusion list)
09:09:49.58 -28:30:36.8 -- not an asteroid (will add it to exclusion list)
09:10:01.18 -24:50:18.5 -- not an asteroid (will add it to exclusion list)
09:09:27.92 -30:06:00.5 -- not an asteroid (will add it to exclusion list)
09:10:19.31 -21:58:44.2 -- not an asteroid (will add it to exclusion list)
08:17:06.82 -27:27:30.8 -- not an asteroid (will add it to exclusion list)
09:07:22.22 -22:46:02.6 -- not an asteroid (will add it to exclusion list)
09:03:27.92 -30:29:23.3 -- not an asteroid (will add it to exclusion list)
09:11:58.12 -27:26:51.6 -- not an asteroid (will add it to exclusion list)
09:06:21.42 -22:39:19.3 -- not an asteroid (will add it to exclusion list)
09:10:47.56 -30:16:05.6 -- not an asteroid (will add it to exclusion list)
09:12:22.29 -23:39:25.7 -- not an asteroid (will add it to exclusion list)
09:12:03.14 -26:38:24.3 -- not an asteroid (will add it to exclusion list)
09:10:57.33 -21:23:37.1 -- not an asteroid (will add it to exclusion list)
09:11:09.45 -24:40:26.0 -- not an asteroid (will add it to exclusion list)
09:08:39.76 -22:08:38.5 -- not an asteroid (will add it to exclusion list)
09:07:08.36 -27:06:43.4 -- not an asteroid (will add it to exclusion list)
09:07:49.84 -28:18:59.7 -- not an asteroid (will add it to exclusion list)
09:08:29.08 -21:57:10.8 -- not an asteroid (will add it to exclusion list)
09:10:01.17 -27:05:19.3 -- not an asteroid (will add it to exclusion list)
09:10:05.20 -24:20:58.9 -- not an asteroid (will add it to exclusion list)
09:11:08.42 -29:35:09.5 -- not an asteroid (will add it to exclusion list)
09:07:54.05 -22:55:45.2 -- not an asteroid (will add it to exclusion list)
09:11:37.77 -22:49:50.5 -- not an asteroid (will add it to exclusion list)
09:10:49.09 -30:16:00.4 -- not an asteroid (will add it to exclusion list)
09:08:46.82 -30:00:32.1 -- not an asteroid (will add it to exclusion list)
09:11:43.52 -24:19:09.7 -- not an asteroid (will add it to exclusion list)
09:06:52.33 -21:49:37.1 -- not an asteroid (will add it to exclusion list)
09:10:36.38 -28:34:25.6 -- not an asteroid (will add it to exclusion list)
09:08:09.37 -27:26:02.5 -- not an asteroid (will add it to exclusion list)
09:09:18.91 -24:40:29.2 -- not an asteroid (will add it to exclusion list)
09:08:40.28 -24:07:51.5 -- not an asteroid (will add it to exclusion list)
09:09:47.86 -22:42:02.0 -- not an asteroid (will add it to exclusion list)
09:07:49.13 -28:19:05.4 -- not an asteroid (will add it to exclusion list)
09:07:34.45 -28:57:26.1 -- not an asteroid (will add it to exclusion list)
09:11:39.06 -23:55:03.8 -- not an asteroid (will add it to exclusion list)
09:06:17.68 -21:25:57.7 -- not an asteroid (will add it to exclusion list)
09:07:16.37 -25:06:46.5 -- not an asteroid (will add it to exclusion list)
09:11:09.47 -29:35:05.7 -- not an asteroid (will add it to exclusion list)
09:06:37.37 -21:35:58.5 -- not an asteroid (will add it to exclusion list)
09:11:37.95 -24:00:31.1 -- not an asteroid (will add it to exclusion list)
09:10:41.65 -29:35:41.6 -- not an asteroid (will add it to exclusion list)
09:12:02.94 -28:13:49.5 -- not an asteroid (will add it to exclusion list)
09:05:57.65 -21:38:24.9 -- not an asteroid (will add it to exclusion list)
09:11:22.72 -27:36:11.5 -- not an asteroid (will add it to exclusion list)
09:09:28.17 -28:04:28.5 -- not an asteroid (will add it to exclusion list)
09:10:21.37 -24:31:04.3 -- not an asteroid (will add it to exclusion list)
09:11:46.62 -27:54:12.7 -- not an asteroid (will add it to exclusion list)
09:12:29.40 -25:12:25.5 -- not an asteroid (will add it to exclusion list)
09:08:47.22 -27:46:01.5 -- not an asteroid (will add it to exclusion list)
09:07:22.24 -22:30:03.1 -- not an asteroid (will add it to exclusion list)
09:09:26.75 -22:01:53.3 -- not an asteroid (will add it to exclusion list)
09:06:48.13 -24:12:21.7 -- not an asteroid (will add it to exclusion list)
09:04:31.61 -21:45:36.3 -- not an asteroid (will add it to exclusion list)
09:11:20.09 -23:26:36.2 -- not an asteroid (will add it to exclusion list)
09:07:12.93 -27:57:07.2 -- not an asteroid (will add it to exclusion list)
09:10:52.58 -28:49:01.2 -- not an asteroid (will add it to exclusion list)
09:12:05.95 -21:30:48.2 -- not an asteroid (will add it to exclusion list)
09:09:21.36 -24:00:03.9 -- not an asteroid (will add it to exclusion list)
09:11:39.59 -26:15:29.8 -- not an asteroid (will add it to exclusion list)
09:12:03.02 -21:38:46.1 -- not an asteroid (will add it to exclusion list)
09:10:22.11 -29:44:19.0 -- not an asteroid (will add it to exclusion list)
09:07:30.48 -21:16:18.3 -- not an asteroid (will add it to exclusion list)
09:11:46.87 -26:49:33.8 -- not an asteroid (will add it to exclusion list)
09:12:21.66 -24:01:52.1 -- not an asteroid (will add it to exclusion list)
09:07:21.58 -22:36:33.0 -- not an asteroid (will add it to exclusion list)
09:07:33.60 -22:45:43.9 -- not an asteroid (will add it to exclusion list)
09:11:02.65 -21:29:55.2 -- not an asteroid (will add it to exclusion list)
09:10:48.31 -30:49:37.3 -- not an asteroid (will add it to exclusion list)
09:11:21.03 -28:06:10.0 -- not an asteroid (will add it to exclusion list)
09:12:23.41 -23:28:38.0 -- not an asteroid (will add it to exclusion list)
09:11:37.16 -28:16:46.5 -- not an asteroid (will add it to exclusion list)
09:09:47.56 -22:01:56.6 -- not an asteroid (will add it to exclusion list)
09:10:50.50 -21:24:28.2 -- not an asteroid (will add it to exclusion list)
09:10:12.11 -25:33:49.8 -- not an asteroid (will add it to exclusion list)
09:08:33.17 -26:17:28.5 -- not an asteroid (will add it to exclusion list)
09:06:25.04 -31:06:00.9 -- not an asteroid (will add it to exclusion list)
09:11:17.88 -23:42:55.7 -- not an asteroid (will add it to exclusion list)
09:05:28.38 -21:27:56.9 -- not an asteroid (will add it to exclusion list)
09:06:31.11 -21:49:54.4 -- not an asteroid (will add it to exclusion list)
09:09:21.84 -30:12:01.2 -- not an asteroid (will add it to exclusion list)
09:10:27.01 -30:05:26.6 -- not an asteroid (will add it to exclusion list)
09:10:17.71 -24:52:39.5 -- not an asteroid (will add it to exclusion list)
08:21:53.01 -22:58:16.5 -- not an asteroid (will add it to exclusion list)
09:10:36.14 -28:41:34.3 -- not an asteroid (will add it to exclusion list)
08:20:48.01 -25:07:07.9 -- not an asteroid (will add it to exclusion list)
09:09:57.07 -27:27:45.8 -- not an asteroid (will add it to exclusion list)
09:05:06.37 -21:42:27.8 -- not an asteroid (will add it to exclusion list)
09:10:00.91 -21:37:30.3 -- not an asteroid (will add it to exclusion list)
09:11:52.61 -28:46:38.4 -- not an asteroid (will add it to exclusion list)
09:09:36.88 -30:28:53.4 -- not an asteroid (will add it to exclusion list)
09:07:21.51 -22:23:28.5 -- not an asteroid (will add it to exclusion list)
09:12:09.87 -27:10:10.1 -- not an asteroid (will add it to exclusion list)
09:11:23.82 -27:14:20.1 -- not an asteroid (will add it to exclusion list)
09:07:05.65 -21:42:02.5 -- not an asteroid (will add it to exclusion list)
09:01:02.88 -30:48:10.4 -- not an asteroid (will add it to exclusion list)
09:10:21.37 -21:19:32.0 -- not an asteroid (will add it to exclusion list)
09:12:31.33 -30:04:57.4 -- not an asteroid (will add it to exclusion list)
09:07:00.42 -22:30:41.7 -- not an asteroid (will add it to exclusion list)
09:11:27.03 -28:29:50.1 -- not an asteroid (will add it to exclusion list)
09:09:10.61 -21:23:31.3 -- not an asteroid (will add it to exclusion list)
09:09:57.60 -22:06:02.1 -- not an asteroid (will add it to exclusion list)
09:08:38.99 -26:25:39.8 -- not an asteroid (will add it to exclusion list)
09:12:09.52 -23:29:24.1 -- not an asteroid (will add it to exclusion list)
09:12:38.77 -25:43:25.2 -- not an asteroid (will add it to exclusion list)
09:10:58.88 -23:28:10.9 -- not an asteroid (will add it to exclusion list)
09:11:59.34 -22:44:00.2 -- not an asteroid (will add it to exclusion list)
09:09:59.19 -27:17:05.0 -- not an asteroid (will add it to exclusion list)
09:12:02.46 -25:51:56.1 -- not an asteroid (will add it to exclusion list)
09:09:18.45 -22:42:04.1 -- not an asteroid (will add it to exclusion list)
09:05:31.01 -30:47:46.7 -- not an asteroid (will add it to exclusion list)
09:09:37.97 -27:11:43.4 -- not an asteroid (will add it to exclusion list)
09:04:44.89 -21:12:30.4 -- not an asteroid (will add it to exclusion list)
09:10:04.50 -26:35:36.7 -- not an asteroid (will add it to exclusion list)
09:05:20.01 -21:17:41.9 -- not an asteroid (will add it to exclusion list)
09:04:56.03 -21:51:33.7 -- not an asteroid (will add it to exclusion list)
09:10:28.42 -22:39:58.6 -- not an asteroid (will add it to exclusion list)
09:08:15.82 -21:12:21.0 -- not an asteroid (will add it to exclusion list)
09:08:06.35 -30:38:10.8 -- not an asteroid (will add it to exclusion list)
09:09:03.28 -29:34:55.9 -- not an asteroid (will add it to exclusion list)
09:08:50.43 -21:34:53.3 -- not an asteroid (will add it to exclusion list)
09:11:27.87 -23:21:17.5 -- not an asteroid (will add it to exclusion list)
09:10:58.71 -29:37:13.0 -- not an asteroid (will add it to exclusion list)
09:12:11.65 -21:28:49.3 -- not an asteroid (will add it to exclusion list)
09:10:26.21 -30:54:21.1 -- not an asteroid (will add it to exclusion list)
09:11:24.85 -22:38:56.8 -- not an asteroid (will add it to exclusion list)
09:10:26.55 -22:48:42.1 -- not an asteroid (will add it to exclusion list)
09:10:07.04 -21:36:06.3 -- not an asteroid (will add it to exclusion list)
09:11:02.03 -21:21:29.4 -- not an asteroid (will add it to exclusion list)
09:10:47.80 -22:39:12.6 -- not an asteroid (will add it to exclusion list)
09:11:12.34 -21:43:32.2 -- not an asteroid (will add it to exclusion list)
09:12:35.14 -26:10:33.3 -- not an asteroid (will add it to exclusion list)
09:12:20.94 -24:57:10.7 -- not an asteroid (will add it to exclusion list)
09:11:05.09 -23:33:12.0 -- not an asteroid (will add it to exclusion list)
09:12:18.84 -21:57:08.9 -- not an asteroid (will add it to exclusion list)
09:04:24.68 -21:24:20.2 -- not an asteroid (will add it to exclusion list)
09:05:51.54 -24:34:34.6 -- not an asteroid (will add it to exclusion list)
08:34:29.42 -30:43:12.5 -- not an asteroid (will add it to exclusion list)
08:20:08.99 -25:51:06.1 -- not an asteroid (will add it to exclusion list)
08:32:03.72 -24:51:17.2 -- not an asteroid (will add it to exclusion list)
08:48:57.46 -24:12:27.3 -- not an asteroid (will add it to exclusion list)
08:35:39.23 -25:18:49.1 -- not an asteroid (will add it to exclusion list)
08:29:22.63 -30:36:43.9 -- not an asteroid (will add it to exclusion list)
08:51:36.33 -29:11:13.0 -- not an asteroid (will add it to exclusion list)
08:35:26.51 -27:16:12.0 -- not an asteroid (will add it to exclusion list)
08:28:13.68 -27:18:33.3 -- not an asteroid (will add it to exclusion list)
09:04:07.07 -21:16:19.1 -- not an asteroid (will add it to exclusion list)
08:41:32.52 -24:57:41.9 -- not an asteroid (will add it to exclusion list)
08:17:49.58 -26:00:48.5 -- not an asteroid (will add it to exclusion list)
08:25:43.23 -29:15:44.0 -- not an asteroid (will add it to exclusion list)
08:37:22.53 -24:29:20.0 -- not an asteroid (will add it to exclusion list)
08:30:14.43 -25:18:28.9 -- not an asteroid (will add it to exclusion list)
08:35:58.85 -24:31:44.1 -- not an asteroid (will add it to exclusion list)
08:30:54.36 -26:46:59.4 -- not an asteroid (will add it to exclusion list)
08:19:04.78 -24:02:11.5 -- not an asteroid (will add it to exclusion list)
08:52:42.62 -25:14:45.8 -- not an asteroid (will add it to exclusion list)
08:32:04.46 -28:53:28.6 -- not an asteroid (will add it to exclusion list)
08:31:54.30 -27:44:27.4 -- not an asteroid (will add it to exclusion list)
08:29:15.53 -22:36:10.4 -- not an asteroid (will add it to exclusion list)
08:29:15.97 -27:56:36.9 -- not an asteroid (will add it to exclusion list)
08:11:33.44 -26:19:02.2 -- not an asteroid (will add it to exclusion list)
08:39:42.97 -26:40:47.4 -- not an asteroid (will add it to exclusion list)
08:10:21.18 -23:00:47.6 -- not an asteroid (will add it to exclusion list)
08:32:00.66 -27:15:32.4 -- not an asteroid (will add it to exclusion list)
08:20:07.68 -26:16:33.5 -- not an asteroid (will add it to exclusion list)
09:09:27.92 -22:13:13.1 -- not an asteroid (will add it to exclusion list)
08:34:38.18 -26:48:42.5 -- not an asteroid (will add it to exclusion list)
08:37:58.80 -29:42:27.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
08:03:08.94 -30:12:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:10:21.18 -23:00:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:33.44 -26:19:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:13.73 -30:25:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:06.82 -27:27:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:49.58 -26:00:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:04.78 -24:02:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:07.68 -26:16:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:08.99 -25:51:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:48.01 -25:07:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:53.01 -22:58:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:25.94 -24:21:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:43.23 -29:15:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:28:13.68 -27:18:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:15.53 -22:36:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:15.97 -27:56:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:22.63 -30:36:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:30:14.43 -25:18:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:30:54.36 -26:46:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:31:54.30 -27:44:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:32:00.66 -27:15:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:32:03.72 -24:51:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:32:04.46 -28:53:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:33:37.49 -30:16:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:34:29.42 -30:43:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:34:38.18 -26:48:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:35:26.51 -27:16:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:35:39.23 -25:18:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:35:58.85 -24:31:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:37:22.53 -24:29:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:37:58.80 -29:42:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:39:42.97 -26:40:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:40:58.30 -23:27:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:41:32.52 -24:57:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:47:38.91 -28:22:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:48:57.46 -24:12:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:49:02.67 -26:34:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:51:35.56 -30:05:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:51:36.33 -29:11:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:52:42.62 -25:14:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:00:31.59 -25:43:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:00:58.49 -31:13:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:01:02.88 -30:48:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:02:27.14 -21:22:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:02:38.01 -30:57:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:03:06.31 -30:45:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:03:16.09 -22:25:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:03:25.60 -21:34:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:03:27.92 -30:29:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:03:32.72 -30:43:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:03:37.20 -21:29:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:03:43.39 -26:39:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:03:58.06 -29:46:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:00.80 -22:04:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:07.07 -21:16:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:14.12 -29:29:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:14.69 -21:26:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:17.90 -21:43:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:24.68 -21:24:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:31.61 -21:45:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:39.67 -22:12:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:39.69 -30:23:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:41.48 -21:29:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:44.89 -21:12:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:52.71 -30:04:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:56.03 -21:51:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:03.04 -30:24:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:03.80 -26:38:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:04.25 -25:05:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:06.37 -21:42:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:10.96 -21:21:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:20.01 -21:17:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:22.89 -29:20:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:28.38 -21:27:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:31.01 -30:47:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:32.15 -28:25:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:39.81 -22:50:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:51.54 -24:34:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:53.23 -24:45:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:53.38 -29:12:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:53.74 -29:11:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:05:57.65 -21:38:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:10.27 -30:59:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:11.50 -22:09:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:17.68 -21:25:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:17.96 -22:23:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:19.59 -28:00:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:21.42 -22:39:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:24.33 -21:29:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:25.04 -31:06:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:28.01 -25:39:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:31.11 -21:49:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:31.48 -21:59:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:32.19 -24:45:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:37.37 -21:35:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:38.77 -22:21:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:48.13 -24:12:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:48.27 -30:36:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:48.78 -27:20:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:52.33 -21:49:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:06:56.51 -26:03:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:00.42 -22:30:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:03.26 -26:49:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:05.65 -21:42:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:08.36 -27:06:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:12.93 -27:57:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:16.37 -25:06:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:19.50 -26:24:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:21.40 -26:57:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:21.51 -22:23:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:21.58 -22:36:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:22.22 -22:46:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:22.24 -22:30:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:22.60 -31:06:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:23.80 -31:06:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:30.48 -21:16:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:33.60 -22:45:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:33.85 -29:37:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:34.45 -28:57:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:37.42 -24:33:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:47.54 -29:57:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:49.13 -28:19:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:49.84 -28:18:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:53.25 -26:27:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:54.05 -22:55:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:05.80 -29:01:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:06.33 -29:40:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:06.35 -30:38:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:06.50 -27:30:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:09.37 -27:26:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:09.66 -29:56:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:10.98 -29:56:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:11.83 -24:35:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:12.59 -26:40:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:15.67 -22:00:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:15.82 -21:12:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:17.56 -22:33:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:21.44 -24:36:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:24.57 -25:08:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:29.08 -21:57:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:30.00 -24:12:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:31.98 -21:20:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:33.17 -26:17:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:38.99 -26:25:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:39.76 -22:08:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:40.28 -24:07:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:40.94 -22:05:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:42.70 -22:26:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:46.82 -30:00:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:47.12 -25:21:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:47.22 -27:46:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:48.30 -26:25:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:48.77 -26:25:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:50.43 -21:34:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:50.98 -23:43:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:51.21 -24:26:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:53.27 -27:49:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:54.45 -24:08:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:55.33 -27:27:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:56.17 -21:24:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:56.41 -22:23:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:58.79 -30:23:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:08:59.86 -30:23:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:03.28 -29:34:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:06.49 -29:44:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:10.61 -21:23:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:16.78 -28:38:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:18.45 -22:42:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:18.91 -24:40:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:19.54 -23:32:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:20.14 -23:46:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:21.06 -25:53:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:21.36 -24:00:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:21.84 -30:12:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:22.70 -23:43:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:26.75 -22:01:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:27.92 -22:13:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:27.92 -30:06:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:28.17 -28:04:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:28.31 -27:33:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:31.50 -21:51:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:36.88 -30:28:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:37.97 -27:11:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:39.58 -29:31:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:42.79 -29:26:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:45.66 -27:00:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:46.25 -27:00:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:47.56 -22:01:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:47.86 -22:42:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:48.69 -29:42:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:48.78 -21:42:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:49.25 -22:58:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:49.58 -28:30:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:57.07 -27:27:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:57.60 -22:06:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:58.84 -28:58:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:59.19 -27:17:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:00.91 -21:37:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:01.17 -27:05:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:01.18 -24:50:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:04.50 -26:35:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:05.03 -26:04:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:05.20 -24:20:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:07.04 -21:36:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:11.27 -25:03:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:12.11 -25:33:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:14.41 -26:31:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:14.50 -29:45:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:14.77 -30:25:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:17.71 -24:52:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:17.90 -23:54:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:19.31 -21:58:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:21.37 -21:19:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:21.37 -24:31:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:22.11 -29:44:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:24.74 -27:07:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:25.49 -30:30:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:25.71 -29:41:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:26.21 -30:54:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:26.55 -22:48:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:26.74 -24:50:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:27.01 -30:05:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:28.13 -23:17:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:28.42 -22:39:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:31.78 -29:44:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:33.15 -22:26:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:35.06 -23:20:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:35.80 -22:32:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:36.14 -28:41:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:36.38 -28:34:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:41.65 -29:35:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:47.56 -30:16:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:47.80 -22:39:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:48.31 -30:49:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:49.09 -30:16:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:50.09 -23:28:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:50.42 -23:28:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:50.50 -21:24:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:51.23 -29:40:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:52.58 -28:49:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:53.24 -21:44:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:53.62 -22:09:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:56.07 -22:03:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:57.33 -21:23:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:58.71 -29:37:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:58.88 -23:28:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:02.03 -21:21:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:02.65 -21:29:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:05.09 -23:33:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:06.94 -27:50:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:08.42 -29:35:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:09.08 -24:27:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:09.45 -24:40:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:09.47 -29:35:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:10.25 -30:08:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:12.23 -29:30:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:12.33 -24:08:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:12.34 -21:43:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:12.53 -24:31:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:13.28 -29:30:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:17.88 -23:42:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:20.09 -23:26:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:21.03 -28:06:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:21.31 -23:59:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:22.72 -27:36:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:23.69 -25:56:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:23.82 -27:14:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:24.85 -22:38:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:26.14 -24:42:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:27.03 -28:29:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:27.87 -23:21:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:28.93 -30:14:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:31.31 -28:08:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:33.73 -22:28:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:36.22 -27:45:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:37.16 -28:16:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:37.77 -22:49:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:37.95 -24:00:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:39.06 -23:55:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:39.59 -26:15:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:42.14 -22:51:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:43.52 -24:19:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:46.37 -28:32:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:46.62 -27:54:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:46.87 -26:49:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:47.17 -24:43:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:48.09 -24:58:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:49.74 -22:13:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:50.17 -30:05:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:52.61 -28:46:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:54.01 -22:10:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:58.12 -27:26:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:59.34 -22:44:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:02.46 -25:51:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:02.94 -28:13:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:03.02 -21:38:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:03.14 -26:38:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:03.72 -26:37:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:05.84 -24:44:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:05.90 -28:29:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:05.95 -21:30:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:08.25 -27:37:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:08.45 -28:14:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:09.52 -23:29:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:09.87 -27:10:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:11.65 -21:28:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:16.59 -23:52:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:16.76 -22:45:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:18.81 -29:47:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:18.84 -21:57:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:20.13 -29:47:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:20.94 -24:57:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:21.66 -24:01:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:22.19 -24:15:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:22.29 -23:39:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:23.41 -23:28:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:29.40 -25:12:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:31.33 -30:04:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:33.46 -28:39:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:35.14 -26:10:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:38.77 -25:43:25.2 -- 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)
08:03:08.94 -30:12:59.6 -- not a known variable star
08:10:21.18 -23:00:47.6 -- a known variable star
08:11:33.44 -26:19:02.2 -- a known variable star
08:15:13.73 -30:25:32.3 -- a known variable star
08:17:06.82 -27:27:30.8 -- not a known variable star
08:17:49.58 -26:00:48.5 -- a known variable star
08:19:04.78 -24:02:11.5 -- a known variable star
08:20:07.68 -26:16:33.5 -- a known variable star
08:20:08.99 -25:51:06.1 -- a known variable star
08:20:48.01 -25:07:07.9 -- a known variable star
08:21:53.01 -22:58:16.5 -- a known variable star
08:24:25.94 -24:21:25.3 -- a known variable star
08:25:43.23 -29:15:44.0 -- a known variable star
08:28:13.68 -27:18:33.3 -- not a known variable star
08:29:15.53 -22:36:10.4 -- a known variable star
08:29:15.97 -27:56:36.9 -- a known variable star
08:29:22.63 -30:36:43.9 -- a known variable star
08:30:14.43 -25:18:28.9 -- a known variable star
08:30:54.36 -26:46:59.4 -- a known variable star
08:31:54.30 -27:44:27.4 -- a known variable star
08:32:00.66 -27:15:32.4 -- a known variable star
08:32:03.72 -24:51:17.2 -- a known variable star
08:32:04.46 -28:53:28.6 -- a known variable star
08:33:37.49 -30:16:49.5 -- a known variable star
08:34:29.42 -30:43:12.5 -- a known variable star
08:34:38.18 -26:48:42.5 -- not a known variable star
08:35:26.51 -27:16:12.0 -- a known variable star
08:35:39.23 -25:18:49.1 -- a known variable star
08:35:58.85 -24:31:44.1 -- a known variable star
08:37:22.53 -24:29:20.0 -- a known variable star
08:37:58.80 -29:42:27.2 -- a known variable star
08:39:42.97 -26:40:47.4 -- a known variable star
08:40:58.30 -23:27:03.0 -- not a known variable star
08:41:32.52 -24:57:41.9 -- a known variable star
08:47:38.91 -28:22:08.9 -- not a known variable star
08:48:57.46 -24:12:27.3 -- a known variable star
08:49:02.67 -26:34:04.2 -- not a known variable star
08:51:35.56 -30:05:21.3 -- not a known variable star
08:51:36.33 -29:11:13.0 -- a known variable star
08:52:42.62 -25:14:45.8 -- a known variable star
09:00:31.59 -25:43:16.2 -- a known variable star
09:00:58.49 -31:13:07.4 -- not a known variable star
09:01:02.88 -30:48:10.4 -- a known variable star
09:02:27.14 -21:22:11.9 -- a known variable star
09:02:38.01 -30:57:43.0 -- a known variable star
09:03:06.31 -30:45:44.0 -- a known variable star
09:03:16.09 -22:25:07.6 -- not a known variable star
09:03:25.60 -21:34:00.1 -- not a known variable star
09:03:27.92 -30:29:23.3 -- a known variable star
09:03:32.72 -30:43:56.1 -- not a known variable star
09:03:37.20 -21:29:03.4 -- a known variable star
09:03:43.39 -26:39:29.7 -- not a known variable star
09:03:58.06 -29:46:09.4 -- not a known variable star
09:04:00.80 -22:04:46.7 -- not a known variable star
09:04:07.07 -21:16:19.1 -- not a known variable star
09:04:14.12 -29:29:36.0 -- a known variable star
09:04:14.69 -21:26:46.2 -- not a known variable star
09:04:17.90 -21:43:34.0 -- not a known variable star
09:04:24.68 -21:24:20.2 -- not a known variable star
09:04:31.61 -21:45:36.3 -- not a known variable star
09:04:39.67 -22:12:42.3 -- a known variable star
09:04:39.69 -30:23:09.8 -- not a known variable star
09:04:41.48 -21:29:06.2 -- not a known variable star
09:04:44.89 -21:12:30.4 -- not a known variable star
09:04:52.71 -30:04:08.3 -- a known variable star
09:04:56.03 -21:51:33.7 -- not a known variable star
09:05:03.04 -30:24:57.1 -- not a known variable star
09:05:03.80 -26:38:49.0 -- not a known variable star
09:05:04.25 -25:05:21.8 -- a known variable star
09:05:06.37 -21:42:27.8 -- not a known variable star
09:05:10.96 -21:21:30.8 -- not a known variable star
09:05:20.01 -21:17:41.9 -- not a known variable star
09:05:22.89 -29:20:30.3 -- not a known variable star
09:05:28.38 -21:27:56.9 -- not a known variable star
09:05:31.01 -30:47:46.7 -- not a known variable star
09:05:32.15 -28:25:49.8 -- not a known variable star
09:05:39.81 -22:50:17.9 -- not a known variable star
09:05:51.54 -24:34:34.6 -- not a known variable star
09:05:53.23 -24:45:40.8 -- not a known variable star
09:05:53.38 -29:12:04.9 -- not a known variable star
09:05:53.74 -29:11:21.4 -- a known variable star
09:05:57.65 -21:38:24.9 -- not a known variable star
09:06:10.27 -30:59:27.2 -- not a known variable star
09:06:11.50 -22:09:10.8 -- not a known variable star
09:06:17.68 -21:25:57.7 -- not a known variable star
09:06:17.96 -22:23:56.3 -- not a known variable star
09:06:19.59 -28:00:29.7 -- a known variable star
09:06:21.42 -22:39:19.3 -- not a known variable star
09:06:24.33 -21:29:19.7 -- not a known variable star
09:06:25.04 -31:06:00.9 -- a known variable star
09:06:28.01 -25:39:28.1 -- not a known variable star
09:06:31.11 -21:49:54.4 -- not a known variable star
09:06:31.48 -21:59:03.9 -- not a known variable star
09:06:32.19 -24:45:06.2 -- a known variable star
09:06:37.37 -21:35:58.5 -- not a known variable star
09:06:38.77 -22:21:59.1 -- not a known variable star
09:06:48.13 -24:12:21.7 -- not a known variable star
09:06:48.27 -30:36:46.3 -- not a known variable star
09:06:48.78 -27:20:24.9 -- not a known variable star
09:06:52.33 -21:49:37.1 -- not a known variable star
09:06:56.51 -26:03:54.9 -- not a known variable star
09:07:00.42 -22:30:41.7 -- not a known variable star
09:07:03.26 -26:49:35.7 -- not a known variable star
09:07:05.65 -21:42:02.5 -- not a known variable star
09:07:08.36 -27:06:43.4 -- not a known variable star
09:07:12.93 -27:57:07.2 -- not a known variable star
09:07:16.37 -25:06:46.5 -- not a known variable star
09:07:19.50 -26:24:45.8 -- not a known variable star
09:07:21.40 -26:57:41.5 -- not a known variable star
09:07:21.51 -22:23:28.5 -- not a known variable star
09:07:21.58 -22:36:33.0 -- not a known variable star
09:07:22.22 -22:46:02.6 -- not a known variable star
09:07:22.24 -22:30:03.1 -- not a known variable star
09:07:22.60 -31:06:42.5 -- a known variable star
09:07:23.80 -31:06:47.9 -- a known variable star
09:07:30.48 -21:16:18.3 -- not a known variable star
09:07:33.60 -22:45:43.9 -- not a known variable star
09:07:33.85 -29:37:44.0 -- not a known variable star
09:07:34.45 -28:57:26.1 -- not a known variable star
09:07:37.42 -24:33:31.4 -- not a known variable star
09:07:47.54 -29:57:09.4 -- not a known variable star
09:07:49.13 -28:19:05.4 -- not a known variable star
09:07:49.84 -28:18:59.7 -- not a known variable star
09:07:53.25 -26:27:02.9 -- not a known variable star
09:07:54.05 -22:55:45.2 -- not a known variable star
09:08:05.80 -29:01:46.8 -- not a known variable star
09:08:06.33 -29:40:44.4 -- not a known variable star
09:08:06.35 -30:38:10.8 -- not a known variable star
09:08:06.50 -27:30:22.4 -- not a known variable star
09:08:09.37 -27:26:02.5 -- not a known variable star
09:08:09.66 -29:56:02.1 -- not a known variable star
09:08:10.98 -29:56:02.5 -- not a known variable star
09:08:11.83 -24:35:02.3 -- not a known variable star
09:08:12.59 -26:40:44.5 -- not a known variable star
09:08:15.67 -22:00:11.5 -- not a known variable star
09:08:15.82 -21:12:21.0 -- not a known variable star
09:08:17.56 -22:33:32.5 -- not a known variable star
09:08:21.44 -24:36:45.5 -- not a known variable star
09:08:24.57 -25:08:46.7 -- not a known variable star
09:08:29.08 -21:57:10.8 -- not a known variable star
09:08:30.00 -24:12:05.3 -- a known variable star
09:08:31.98 -21:20:37.8 -- a known variable star
09:08:33.17 -26:17:28.5 -- not a known variable star
09:08:38.99 -26:25:39.8 -- not a known variable star
09:08:39.76 -22:08:38.5 -- not a known variable star
09:08:40.28 -24:07:51.5 -- a known variable star
09:08:40.94 -22:05:45.3 -- not a known variable star
09:08:42.70 -22:26:12.6 -- not a known variable star
09:08:46.82 -30:00:32.1 -- not a known variable star
09:08:47.12 -25:21:12.4 -- not a known variable star
09:08:47.22 -27:46:01.5 -- not a known variable star
09:08:48.30 -26:25:20.0 -- not a known variable star
09:08:48.77 -26:25:21.9 -- not a known variable star
09:08:50.43 -21:34:53.3 -- a known variable star
09:08:50.98 -23:43:44.3 -- not a known variable star
09:08:51.21 -24:26:52.8 -- not a known variable star
09:08:53.27 -27:49:48.4 -- not a known variable star
09:08:54.45 -24:08:34.9 -- not a known variable star
09:08:55.33 -27:27:36.7 -- not a known variable star
09:08:56.17 -21:24:19.9 -- a known variable star
09:08:56.41 -22:23:23.5 -- not a known variable star
09:08:58.79 -30:23:55.5 -- not a known variable star
09:08:59.86 -30:23:58.2 -- not a known variable star
09:09:03.28 -29:34:55.9 -- not a known variable star
09:09:06.49 -29:44:29.3 -- not a known variable star
09:09:10.61 -21:23:31.3 -- not a known variable star
09:09:16.78 -28:38:16.7 -- not a known variable star
09:09:18.45 -22:42:04.1 -- not a known variable star
09:09:18.91 -24:40:29.2 -- not a known variable star
09:09:19.54 -23:32:20.3 -- a known variable star
09:09:20.14 -23:46:23.0 -- not a known variable star
09:09:21.06 -25:53:25.9 -- not a known variable star
09:09:21.36 -24:00:03.9 -- not a known variable star
09:09:21.84 -30:12:01.2 -- a known variable star
09:09:22.70 -23:43:53.1 -- not a known variable star
09:09:26.75 -22:01:53.3 -- not a known variable star
09:09:27.92 -22:13:13.1 -- a known variable star
09:09:27.92 -30:06:00.5 -- not a known variable star
09:09:28.17 -28:04:28.5 -- not a known variable star
09:09:28.31 -27:33:27.2 -- not a known variable star
09:09:31.50 -21:51:06.3 -- not a known variable star
09:09:36.88 -30:28:53.4 -- not a known variable star
09:09:37.97 -27:11:43.4 -- not a known variable star
09:09:39.58 -29:31:57.6 -- not a known variable star
09:09:42.79 -29:26:29.6 -- not a known variable star
09:09:45.66 -27:00:52.5 -- not a known variable star
09:09:46.25 -27:00:56.4 -- not a known variable star
09:09:47.56 -22:01:56.6 -- not a known variable star
09:09:47.86 -22:42:02.0 -- not a known variable star
09:09:48.69 -29:42:33.4 -- not a known variable star
09:09:48.78 -21:42:07.9 -- a known variable star
09:09:49.25 -22:58:42.0 -- not a known variable star
09:09:49.58 -28:30:36.8 -- a known variable star
09:09:57.07 -27:27:45.8 -- not a known variable star
09:09:57.60 -22:06:02.1 -- not a known variable star
09:09:58.84 -28:58:44.9 -- not a known variable star
09:09:59.19 -27:17:05.0 -- not a known variable star
09:10:00.91 -21:37:30.3 -- not a known variable star
09:10:01.17 -27:05:19.3 -- not a known variable star
09:10:01.18 -24:50:18.5 -- not a known variable star
09:10:04.50 -26:35:36.7 -- not a known variable star
09:10:05.03 -26:04:16.3 -- not a known variable star
09:10:05.20 -24:20:58.9 -- not a known variable star
09:10:07.04 -21:36:06.3 -- not a known variable star
09:10:11.27 -25:03:40.8 -- not a known variable star
09:10:12.11 -25:33:49.8 -- not a known variable star
09:10:14.41 -26:31:16.2 -- not a known variable star
09:10:14.50 -29:45:07.9 -- not a known variable star
09:10:14.77 -30:25:45.1 -- a known variable star
09:10:17.71 -24:52:39.5 -- not a known variable star
09:10:17.90 -23:54:34.1 -- not a known variable star
09:10:19.31 -21:58:44.2 -- not a known variable star
09:10:21.37 -21:19:32.0 -- not a known variable star
09:10:21.37 -24:31:04.3 -- not a known variable star
09:10:22.11 -29:44:19.0 -- not a known variable star
09:10:24.74 -27:07:23.8 -- not a known variable star
09:10:25.49 -30:30:23.2 -- not a known variable star
09:10:25.71 -29:41:27.1 -- a known variable star
09:10:26.21 -30:54:21.1 -- not a known variable star
09:10:26.55 -22:48:42.1 -- not a known variable star
09:10:26.74 -24:50:45.0 -- not a known variable star
09:10:27.01 -30:05:26.6 -- not a known variable star
09:10:28.13 -23:17:23.2 -- not a known variable star
09:10:28.42 -22:39:58.6 -- not a known variable star
09:10:31.78 -29:44:06.1 -- a known variable star
09:10:33.15 -22:26:26.5 -- not a known variable star
09:10:35.06 -23:20:36.4 -- not a known variable star
09:10:35.80 -22:32:49.8 -- not a known variable star
09:10:36.14 -28:41:34.3 -- not a known variable star
09:10:36.38 -28:34:25.6 -- not a known variable star
09:10:41.65 -29:35:41.6 -- not a known variable star
09:10:47.56 -30:16:05.6 -- not a known variable star
09:10:47.80 -22:39:12.6 -- not a known variable star
09:10:48.31 -30:49:37.3 -- not a known variable star
09:10:49.09 -30:16:00.4 -- not a known variable star
09:10:50.09 -23:28:10.1 -- a known variable star
09:10:50.42 -23:28:06.3 -- a known variable star
09:10:50.50 -21:24:28.2 -- not a known variable star
09:10:51.23 -29:40:12.2 -- not a known variable star
09:10:52.58 -28:49:01.2 -- a known variable star
09:10:53.24 -21:44:08.1 -- not a known variable star
09:10:53.62 -22:09:26.7 -- a known variable star
09:10:56.07 -22:03:38.8 -- not a known variable star
09:10:57.33 -21:23:37.1 -- not a known variable star
09:10:58.71 -29:37:13.0 -- not a known variable star
09:10:58.88 -23:28:10.9 -- not a known variable star
09:11:02.03 -21:21:29.4 -- not a known variable star
09:11:02.65 -21:29:55.2 -- not a known variable star
09:11:05.09 -23:33:12.0 -- not a known variable star
09:11:06.94 -27:50:55.7 -- not a known variable star
09:11:08.42 -29:35:09.5 -- not a known variable star
09:11:09.08 -24:27:13.5 -- a known variable star
09:11:09.45 -24:40:26.0 -- not a known variable star
09:11:09.47 -29:35:05.7 -- not a known variable star
09:11:10.25 -30:08:57.2 -- not a known variable star
09:11:12.23 -29:30:45.0 -- not a known variable star
09:11:12.33 -24:08:18.9 -- not a known variable star
09:11:12.34 -21:43:32.2 -- not a known variable star
09:11:12.53 -24:31:13.9 -- a known variable star
09:11:13.28 -29:30:45.7 -- not a known variable star
09:11:17.88 -23:42:55.7 -- not a known variable star
09:11:20.09 -23:26:36.2 -- not a known variable star
09:11:21.03 -28:06:10.0 -- not a known variable star
09:11:21.31 -23:59:38.2 -- not a known variable star
09:11:22.72 -27:36:11.5 -- not a known variable star
09:11:23.69 -25:56:31.6 -- a known variable star
09:11:23.82 -27:14:20.1 -- not a known variable star
09:11:24.85 -22:38:56.8 -- not a known variable star
09:11:26.14 -24:42:59.9 -- a known variable star
09:11:27.03 -28:29:50.1 -- not a known variable star
09:11:27.87 -23:21:17.5 -- not a known variable star
09:11:28.93 -30:14:13.7 -- a known variable star
09:11:31.31 -28:08:30.1 -- not a known variable star
09:11:33.73 -22:28:15.9 -- not a known variable star
09:11:36.22 -27:45:46.9 -- a known variable star
09:11:37.16 -28:16:46.5 -- not a known variable star
09:11:37.77 -22:49:50.5 -- not a known variable star
09:11:37.95 -24:00:31.1 -- not a known variable star
09:11:39.06 -23:55:03.8 -- not a known variable star
09:11:39.59 -26:15:29.8 -- a known variable star
09:11:42.14 -22:51:43.0 -- not a known variable star
09:11:43.52 -24:19:09.7 -- not a known variable star
09:11:46.37 -28:32:15.6 -- not a known variable star
09:11:46.62 -27:54:12.7 -- not a known variable star
09:11:46.87 -26:49:33.8 -- not a known variable star
09:11:47.17 -24:43:28.8 -- not a known variable star
09:11:48.09 -24:58:00.1 -- not a known variable star
09:11:49.74 -22:13:56.6 -- not a known variable star
09:11:50.17 -30:05:06.4 -- a known variable star
09:11:52.61 -28:46:38.4 -- not a known variable star
09:11:54.01 -22:10:14.2 -- not a known variable star
09:11:58.12 -27:26:51.6 -- not a known variable star
09:11:59.34 -22:44:00.2 -- a known variable star
09:12:02.46 -25:51:56.1 -- not a known variable star
09:12:02.94 -28:13:49.5 -- not a known variable star
09:12:03.02 -21:38:46.1 -- a known variable star
09:12:03.14 -26:38:24.3 -- not a known variable star
09:12:03.72 -26:37:10.9 -- not a known variable star
09:12:05.84 -24:44:52.9 -- not a known variable star
09:12:05.90 -28:29:09.8 -- a known variable star
09:12:05.95 -21:30:48.2 -- not a known variable star
09:12:08.25 -27:37:51.8 -- not a known variable star
09:12:08.45 -28:14:18.9 -- a known variable star
09:12:09.52 -23:29:24.1 -- not a known variable star
09:12:09.87 -27:10:10.1 -- not a known variable star
09:12:11.65 -21:28:49.3 -- not a known variable star
09:12:16.59 -23:52:49.5 -- not a known variable star
09:12:16.76 -22:45:52.7 -- not a known variable star
09:12:18.81 -29:47:52.8 -- not a known variable star
09:12:18.84 -21:57:08.9 -- not a known variable star
09:12:20.13 -29:47:54.1 -- not a known variable star
09:12:20.94 -24:57:10.7 -- not a known variable star
09:12:21.66 -24:01:52.1 -- not a known variable star
09:12:22.19 -24:15:43.0 -- not a known variable star
09:12:22.29 -23:39:25.7 -- not a known variable star
09:12:23.41 -23:28:38.0 -- not a known variable star
09:12:29.40 -25:12:25.5 -- not a known variable star
09:12:31.33 -30:04:57.4 -- not a known variable star
09:12:33.46 -28:39:03.0 -- a known variable star
09:12:35.14 -26:10:33.3 -- not a known variable star
09:12:38.77 -25:43:25.2 -- not a known variable star
Found 242 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
321 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
No ../exclusion_list_TTUQ2.txt so we are not updating exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= YES
The observatory MPC code is 500
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461093.60520073 -observatory 500
23:23:18.41 -02:00:43.4 Mercury (-0.1mag)
23:04:10.45 -07:31:40.0 Venus (-3.9mag)
21:42:37.15 -14:53:48.6 Mars (1.1mag)
07:06:06.91 +22:54:18.3 Jupiter (-2.5mag)
00:05:24.59 -01:44:38.6 Saturn (1.0mag)
03:39:59.25 +19:21:42.8 Uranus (5.7mag)
00:03:40.42 -01:01:40.5 Neptune (7.8mag)
20:29:06.59 -22:59:35.2 Pluto (14.5mag)
01:50:54.39 +15:54:04.1 Moon (-9.5mag)
-rw-r--r-- 1 apache apache 362 Feb 21 23:52 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461093.60520073:
07:06:09.55 +22:54:15.9 Io (5.4mag)
07:06:17.69 +22:53:58.9 Europa (5.5mag)
07:05:56.69 +22:54:45.7 Ganymede (4.9mag)
07:06:25.24 +22:53:54.3 Callisto (6.2mag)
07:09:15.62 +23:10:42.9 Himalia (15.0mag)
07:06:06.15 +22:54:22.1 Thebe (15.9mag)
07:08:40.75 +23:19:09.5 Elara (17.0mag)
07:01:40.29 +24:02:18.4 Pasiphae (17.0mag)
07:15:07.81 +22:42:17.3 Carme (18.1mag)
00:05:36.23 -01:44:43.4 Titan (8.8mag)
00:05:29.94 -01:44:37.4 Rhea (10.1mag)
00:05:19.85 -01:45:59.9 Iapetus (11.5mag)
00:05:25.23 -01:44:41.5 Hyperion (14.8mag)
00:07:28.88 -01:31:38.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 21 23:52 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.60520073:
08:45:23.99 +24:30:39.8 JWST
10:20:16.15 +38:53:54.1 Chandra
14:46:55.81 -62:11:20.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 21 23:52 spacecraft.txt
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Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461093.60520073 at 500
16:59:35.90 -11:03:46.9 17.5mag 10P/Tempel 2
03:37:15.89 +28:57:39.1 18.0mag 123P/West-Hartley
08:23:43.42 +60:43:47.9 18.4mag 124P/Mrkos
21:19:24.81 -07:39:36.5 22.1mag 141P/Machholz
01:21:02.39 +11:54:00.9 17.6mag 145P/Shoemaker-Levy 5
11:03:01.84 +30:34:12.3 17.9mag 164P/Christensen
09:33:09.61 -33:51:55.8 18.0mag 195P/Hill
15:52:03.54 -06:36:10.0 19.2mag 210P/Christensen
18:16:37.70 -21:28:41.0 17.3mag 218P/LINEAR
16:21:29.13 -18:11:00.5 15.2mag 235P/LINEAR
03:56:19.13 +27:43:58.3 17.8mag 240P/NEAT
15:17:34.30 +06:38:38.3 14.8mag 24P/Schaumasse
11:23:32.27 -03:23:14.2 17.4mag 29P/Schwassmann-Wachmann 1
07:03:48.24 +27:24:48.9 19.6mag 407P/PanSTARRS-Fuls
17:07:03.86 -11:19:15.6 17.6mag 40P/Vaisala 1
11:02:14.78 -08:52:02.9 16.6mag 43P/Wolf-Harrington
13:25:29.56 -05:49:29.8 20.0mag 489P/Denning
04:34:19.90 +48:34:48.3 17.8mag 493P/2024 Q2 (LONEOS)
06:04:22.02 +47:32:00.3 17.7mag 63P/Wild 1
23:14:30.67 -02:08:03.2 16.2mag 78P/Gehrels 2
20:01:19.29 -22:18:43.7 15.0mag 88P/Howell
15:27:53.21 -29:00:26.9 18.7mag P/2023 S1 (PanSTARRS)
04:43:26.83 -72:36:04.4 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:50.41 +31:12:53.7 18.2mag C/2017 K2 (PanSTARRS)
20:06:36.63 -65:11:32.7 18.1mag C/2020 V2 (ZTF)
17:21:39.19 +04:21:04.8 16.3mag C/2021 G2 (ATLAS)
03:35:38.69 +24:36:38.8 15.8mag C/2022 N2 (PanSTARRS)
09:08:14.25 +29:49:20.5 15.3mag C/2022 QE78 (ATLAS)
08:35:41.43 -06:34:08.3 16.7mag C/2022 R6 (PanSTARRS)
23:52:58.53 +48:26:38.4 18.0mag C/2023 C2 (ATLAS)
09:51:11.00 -20:46:24.3 17.5mag C/2023 F3 (ATLAS)
20:34:39.53 +61:14:30.7 17.3mag C/2023 H5 (Lemmon)
19:34:29.79 -03:24:14.5 16.1mag C/2023 R1 (PANSTARRS)
02:48:54.31 +35:40:35.6 18.5mag C/2023 RS61 (PanSTARRS)
21:01:22.27 +81:19:52.9 18.0mag C/2023 X2 (Lemmon)
06:39:13.92 +63:49:09.4 17.3mag C/2024 A1 (ATLAS)
01:56:24.29 -24:41:44.6 11.2mag C/2024 E1 (Wierzchos)
11:45:00.94 -02:35:23.3 18.1mag C/2024 G2 (ATLAS)
19:28:16.26 +00:39:06.8 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.81 -01:43:15.0 17.7mag C/2024 G6 (ATLAS)
19:53:25.63 +03:14:35.6 15.6mag C/2024 J3 (ATLAS)
02:47:13.09 -31:35:01.0 15.4mag C/2024 T5 (ATLAS)
16:25:13.77 -58:12:43.0 15.6mag C/2025 A6 (Lemmon)
04:50:30.05 +62:15:37.9 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)
15:56:45.39 -13:03:36.8 14.8mag C/2025 L1 (ATLAS)
02:20:11.67 -19:05:34.4 16.7mag C/2025 Q3 (ATLAS)
02:09:30.91 +17:16:27.9 21.2mag C/2025 R2 (SWAN)
22:20:44.84 +17:39:10.6 16.4mag C/2025 R3 (PANSTARRS)
21:45:58.25 -16:49:49.2 21.5mag C/2025 T1 (ATLAS)
03:06:20.88 -20:35:23.6 18.3mag C/2026 A1 (MAPS)
21:02:51.43 +20:54:21.5 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 21 23:53 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
-rw-r--r-- 1 apache apache 6.2K Feb 21 23:52 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
-rw-r--r-- 1 apache apache 187K Feb 21 23:52 tocp_transients_list.txt