This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq
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 22.1474 2461093.6474 11.87 03:45:21.20 -12:52:15.0
202.43291 -46.98263 galactic Eri Second-epoch detections are separated by 6.7" and 6.5 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 5114274948147331456 | 03:45:20.64 -12:52:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 45 21.20 -12 52 15.0 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114274948147331456,2461093.6474,11.87,0.05,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
Gaia DR3 5114274948147331456 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:21.20 -12:52:15.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.87 03:52:56.16 -13:11:42.3
204.01627 -45.46073 galactic Eri Second-epoch detections are separated by 3.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5111390452409299328 | 03:52:56.59 -13:11:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 56.16 -13 11 42.3 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5111390452409299328,2461093.6474,11.87,0.05,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
Gaia DR3 5111390452409299328 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:56.16 -13:11:42.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.75 03:48:30.58 -13:35:22.9
203.86575 -46.60249 galactic Eri Second-epoch detections are separated by 2.6" 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 5113988873263501440 | 03:48:30.22 -13:35:26.2 (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!
TCP 2026 02 22.1474* 03 48 30.58 -13 35 22.9 11.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5113988873263501440,2461093.6474,11.75,0.05,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 5113988873263501440 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:30.58 -13:35:22.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.63 03:51:34.57 -13:32:15.7
204.25722 -45.90620 galactic Eri Second-epoch detections are separated by 2.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5110999988341979392 | 03:51:34.98 -13:32:10.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 34.57 -13 32 15.7 11.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5110999988341979392,2461093.6474,11.63,0.05,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
Gaia DR3 5110999988341979392 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:34.57 -13:32:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.33 03:48:00.50 -12:21:47.2
202.18847 -46.17696 galactic Eri Second-epoch detections are separated by 6.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114696099757637888 | 03:48:00.96 -12:21:42.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 00.50 -12 21 47.2 11.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114696099757637888,2461093.6474,11.33,0.05,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
Gaia DR3 5114696099757637888 20260222.1474 11.33CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:00.50 -12:21:47.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.32 03:53:10.14 -07:27:50.1
196.99879 -42.72549 galactic Eri Second-epoch detections are separated by 4.7" 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 3243316142368267264 | 03:53:10.55 -07:27:51.1 (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!
TCP 2026 02 22.1474* 03 53 10.14 -07 27 50.1 11.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243316142368267264,2461093.6474,11.32,0.05,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
Gaia DR3 3243316142368267264 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:10.14 -07:27:50.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.25 03:49:10.33 -12:53:58.7
203.06459 -46.15897 galactic Eri Second-epoch detections are separated by 0.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114471009111847168 | 03:49:09.78 -12:54:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 10.33 -12 53 58.7 11.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114471009111847168,2461093.6474,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5114471009111847168 20260222.1474 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:10.33 -12:53:58.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.12 03:51:25.28 -08:54:10.4
198.41816 -43.81625 galactic Eri Second-epoch detections are separated by 1.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3194660553816167040 | 03:51:26.09 -08:54:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 25.28 -08 54 10.4 11.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194660553816167040,2461093.6474,11.12,0.05,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
Gaia DR3 3194660553816167040 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:25.28 -08:54:10.4 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 10.81 03:52:48.28 -08:47:49.8
198.52174 -43.46649 galactic Eri Second-epoch detections are separated by 1.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3195040297644487808 | 03:52:48.73 -08:47:52.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 48.28 -08 47 49.8 10.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3195040297644487808,2461093.6474,10.81,0.05,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 3195040297644487808 20260222.1474 10.81CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:48.28 -08:47:49.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 10.37 03:52:07.70 -06:14:37.1
195.39766 -42.32131 galactic Eri Second-epoch detections are separated by 2.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245195551337497088 | 03:52:08.19 -06:14:38.8 (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!
TCP 2026 02 22.1474* 03 52 07.70 -06 14 37.1 10.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245195551337497088,2461093.6474,10.37,0.05,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 3245195551337497088 20260222.1474 10.37CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:07.70 -06:14:37.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 31.61 -07 38 15.7 10.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243221790526747648,2461093.6474,10.41,0.05,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 3243221790526747648 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:31.61 -07:38:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 55.77 -09 10 07.5 10.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SW Eri,2461093.6474,10.47,0.05,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
SW Eri 20260222.1474 10.47CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:55.77 -09:10:07.5 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 10.52 03:51:48.95 -06:40:42.4
195.84713 -42.61311 galactic Eri Second-epoch detections are separated by 0.3" and 5.1 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 3243619848095821824 | 03:51:49.61 -06:40:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1951TOYal..23.....B BD-07 693
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 48.95 -06 40 42.4 10.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243619848095821824,2461093.6474,10.52,0.05,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 3243619848095821824 20260222.1474 10.52CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:48.95 -06:40:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 10.56 03:46:35.21 -12:25:42.8
202.04909 -46.51681 galactic Eri Second-epoch detections are separated by 3.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114328347476836352 | 03:46:35.69 -12:25:37.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6/8IV 1988MSS...C04....0H HD 23682
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 46 35.21 -12 25 42.8 10.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114328347476836352,2461093.6474,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5114328347476836352 20260222.1474 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:35.21 -12:25:42.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 10.86 03:53:12.75 -06:57:12.8
196.40913 -42.45692 galactic Eri Second-epoch detections are separated by 3.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243408982381222272 | 03:53:13.29 -06:57:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 12.75 -06 57 12.8 10.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243408982381222272,2461093.6474,10.86,0.05,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 3243408982381222272 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:12.75 -06:57:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.11 03:51:56.87 -05:44:37.7
194.79107 -42.09775 galactic Eri Second-epoch detections are separated by 0.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245229704917320320 | 03:51:57.42 -05:44:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 56.87 -05 44 37.7 11.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245229704917320320,2461093.6474,11.11,0.05,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 3245229704917320320 20260222.1474 11.11CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:56.87 -05:44:37.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.15 03:46:46.49 -13:48:31.4
203.89289 -47.07703 galactic Eri Second-epoch detections are separated by 2.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5113887855631399040 | 03:46:46.78 -13:48:24.4 (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!
TCP 2026 02 22.1474* 03 46 46.49 -13 48 31.4 11.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5113887855631399040,2461093.6474,11.15,0.05,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
Gaia DR3 5113887855631399040 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:46.49 -13:48:31.4 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.46 03:51:08.68 -05:53:04.4
194.81063 -42.34168 galactic Eri Second-epoch detections are separated by 7.3" 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 3245221183702226176 | 03:51:09.24 -05:53:05.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 08.68 -05 53 04.4 11.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245221183702226176,2461093.6474,11.46,0.05,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 3245221183702226176 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:08.68 -05:53:04.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.41 03:50:41.76 -07:03:58.4
196.10552 -43.05097 galactic Eri Second-epoch detections are separated by 4.9" and 5.1 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 3243578753848781184 | 03:50:42.46 -07:04:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 41.76 -07 03 58.4 11.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243578753848781184,2461093.6474,11.41,0.05,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 3243578753848781184 20260222.1474 11.41CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:41.76 -07:03:58.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 04 41 47.76 -07 57 19.9 9.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VZ Eri,2461093.6474,9.32,0.05,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
VZ Eri 20260222.1474 9.32CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:47.76 -07:57:19.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 47.68 -12 16 26.3 13.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114531207373357056,2461093.6474,13.93,0.05,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 5114531207373357056 20260222.1474 13.93CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:47.68 -12:16:26.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 41.50 -11 33 32.2 13.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.87,0.05,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 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:41.50 -11:33:32.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 04 12 28.79 -05 30 31.5 13.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3203264438461460864,2461093.6474,13.77,0.05,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 3203264438461460864 20260222.1474 13.77CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:28.79 -05:30:31.5 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 12.64 -14 15 07.9 13.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.82,0.05,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 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:12.64 -14:15:07.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.44 03:52:05.12 -08:40:27.9
198.25405 -43.56123 galactic Eri Second-epoch detections are separated by 8.3" and 6.4 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 3195045932641528192 | 03:52:05.55 -08:40:31.3 (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!
TCP 2026 02 22.1474* 03 52 05.12 -08 40 27.9 13.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3195045932641528192,2461093.6474,13.44,0.05,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 3195045932641528192 20260222.1474 13.44CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:05.12 -08:40:27.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 49.13 -05 52 27.9 13.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J034949-0552.5,2461093.6474,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J034949-0552.5 20260222.1474 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:49.13 -05:52:27.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.46 03:52:19.44 -14:23:31.9
205.48367 -46.09940 galactic Eri Second-epoch detections are separated by 4.6" and 5.9 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 5110699443708206592 | 03:52:21.36 -14:23:11.9 (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!
TCP 2026 02 22.1474* 03 52 19.44 -14 23 31.9 13.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5110699443708206592,2461093.6474,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5110699443708206592 20260222.1474 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:19.44 -14:23:31.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.60 03:52:49.64 -09:19:03.8
199.15372 -43.71446 galactic Eri Second-epoch detections are separated by 4.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3194443812586193792 | 03:52:50.56 -09:19:03.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 49.64 -09 19 03.8 13.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194443812586193792,2461093.6474,13.60,0.05,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 3194443812586193792 20260222.1474 13.60CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:49.64 -09:19:03.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.49 03:46:40.94 -12:35:00.2
202.26576 -46.56483 galactic Eri Second-epoch detections are separated by 8.4" 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 5114309995081347840 | 03:46:40.74 -12:34:55.0 (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!
TCP 2026 02 22.1474* 03 46 40.94 -12 35 00.2 13.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114309995081347840,2461093.6474,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5114309995081347840 20260222.1474 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:40.94 -12:35:00.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 21.63 -13 50 06.3 13.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.51,0.05,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
target 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:21.63 -13:50:06.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 50.60 -10 33 01.9 13.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.45,0.05,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
target 20260222.1474 13.45CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:50.60 -10:33:01.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.56 03:51:59.07 -09:28:04.2
199.19718 -43.96895 galactic Eri Second-epoch detections are separated by 8.6" and 5.9 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 3194417664825373568 | 03:51:59.30 -09:28:10.4 (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!
TCP 2026 02 22.1474* 03 51 59.07 -09 28 04.2 13.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194417664825373568,2461093.6474,13.56,0.05,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 3194417664825373568 20260222.1474 13.56CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:59.07 -09:28:04.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.35 03:54:37.54 -13:32:56.3
204.72107 -45.23983 galactic Eri Second-epoch detections are separated by 1.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5111315956198695552 | 03:54:37.14 -13:32:57.7 (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!
TCP 2026 02 22.1474* 03 54 37.54 -13 32 56.3 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5111315956198695552,2461093.6474,13.35,0.05,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 5111315956198695552 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:37.54 -13:32:56.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.31 03:56:30.38 -05:02:09.5
194.78743 -40.76048 galactic Eri Second-epoch detections are separated by 4.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245386522762743936 | 03:56:30.80 -05:02:13.0 (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!
TCP 2026 02 22.1474* 03 56 30.38 -05 02 09.5 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245386522762743936,2461093.6474,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3245386522762743936 20260222.1474 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:30.38 -05:02:09.5 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 56.66 -11 54 48.6 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114825051856250368,2461093.6474,13.34,0.05,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 5114825051856250368 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:56.66 -11:54:48.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.26 03:48:35.69 -11:10:40.2
200.76595 -45.51095 galactic Eri Second-epoch detections are separated by 7.1" and 6.3 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 5115676688033843328 | 03:48:35.25 -11:10:40.8 (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!
TCP 2026 02 22.1474* 03 48 35.69 -11 10 40.2 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5115676688033843328,2461093.6474,13.26,0.05,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 5115676688033843328 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:35.69 -11:10:40.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.34 03:46:36.75 -14:18:13.1
204.52903 -47.32131 galactic Eri Second-epoch detections are separated by 4.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5110841658665184384 | 03:46:35.90 -14:18:19.8 (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!
TCP 2026 02 22.1474* 03 46 36.75 -14 18 13.1 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5110841658665184384,2461093.6474,13.34,0.05,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 5110841658665184384 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:36.75 -14:18:13.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.27 03:48:29.20 -11:38:15.8
201.33284 -45.74556 galactic Eri Second-epoch detections are separated by 6.9" 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 5114804023695755520 | 03:48:28.52 -11:38:16.7 (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!
TCP 2026 02 22.1474* 03 48 29.20 -11 38 15.8 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114804023695755520,2461093.6474,13.27,0.05,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 5114804023695755520 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:29.20 -11:38:15.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.20 03:49:45.92 -12:28:55.9
202.61640 -45.84550 galactic Eri Second-epoch detections are separated by 5.0" and 6.0 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 5114500043090731904 | 03:49:46.28 -12:28:48.8 (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!
TCP 2026 02 22.1474* 03 49 45.92 -12 28 55.9 13.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114500043090731904,2461093.6474,13.20,0.05,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 5114500043090731904 20260222.1474 13.20CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:45.92 -12:28:55.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.22 03:49:06.17 -08:19:44.2
197.33213 -44.03064 galactic Eri Second-epoch detections are separated by 1.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3242795180014012032 | 03:49:05.67 -08:19:42.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 06.17 -08 19 44.2 13.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3242795180014012032,2461093.6474,13.22,0.05,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 3242795180014012032 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:06.17 -08:19:44.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 31.19 -08 43 08.0 13.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1474 13.36CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:31.19 -08:43:08.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.10 03:50:44.63 -10:26:14.9
200.18636 -44.69898 galactic Eri Second-epoch detections are separated by 0.7" and 5.1 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 3194205252923337344 | 03:50:44.21 -10:26:16.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 44.63 -10 26 14.9 13.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194205252923337344,2461093.6474,13.10,0.05,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 3194205252923337344 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:44.63 -10:26:14.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.01 03:51:14.76 -10:24:29.6
200.23162 -44.57625 galactic Eri Second-epoch detections are separated by 7.2" 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 3194194773202834688 | 03:51:14.29 -10:24:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 14.76 -10 24 29.6 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194194773202834688,2461093.6474,13.01,0.05,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 3194194773202834688 20260222.1474 13.01CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:14.76 -10:24:29.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.04 03:50:00.70 -10:34:43.1
200.24297 -44.92416 galactic Eri Second-epoch detections are separated by 3.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3194196525549519872 | 03:50:00.10 -10:34:44.4 (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!
TCP 2026 02 22.1474* 03 50 00.70 -10 34 43.1 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3194196525549519872,2461093.6474,13.04,0.05,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
Large-amplitude variable Gaia DR2 3194196525549519872 20260222.1474 13.04CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:00.70 -10:34:43.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.90 03:49:32.40 -06:18:35.8
195.01814 -42.90449 galactic Eri Second-epoch detections are separated by 3.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243704854088417024 | 03:49:33.00 -06:18:29.9 (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!
TCP 2026 02 22.1474* 03 49 32.40 -06 18 35.8 12.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243704854088417024,2461093.6474,12.90,0.05,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 3243704854088417024 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:32.40 -06:18:35.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 04 07 32.82 -08 34 19.4 13.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.11,0.05,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
target 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:07:32.82 -08:34:19.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.00 03:47:21.53 -10:48:12.4
200.09107 -45.60520 galactic Eri Second-epoch detections are separated by 4.4" 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 5115749638054859904 | 03:47:20.98 -10:48:16.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 47 21.53 -10 48 12.4 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5115749638054859904,2461093.6474,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5115749638054859904 20260222.1474 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:21.53 -10:48:12.4 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.90 03:58:44.77 -05:09:21.5
195.30804 -40.34935 galactic Eri Second-epoch detections are separated by 2.4" 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 3245696000926190720 | 03:58:44.51 -05:09:15.7 (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!
TCP 2026 02 22.1474* 03 58 44.77 -05 09 21.5 12.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245696000926190720,2461093.6474,12.90,0.05,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 3245696000926190720 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:44.77 -05:09:21.5 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.91 03:50:20.84 -12:37:48.3
202.89670 -45.78328 galactic Eri Second-epoch detections are separated by 4.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114482622703380992 | 03:50:21.57 -12:37:47.7 (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!
TCP 2026 02 22.1474* 03 50 20.84 -12 37 48.3 12.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114482622703380992,2461093.6474,12.91,0.05,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 5114482622703380992 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:20.84 -12:37:48.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.97 03:58:28.09 -05:02:42.7
195.13664 -40.35013 galactic Eri Second-epoch detections are separated by 4.2" 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 3245712321801912064 | 03:58:28.39 -05:02:49.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 58 28.09 -05 02 42.7 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245712321801912064,2461093.6474,12.97,0.05,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 3245712321801912064 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:28.09 -05:02:42.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.73 03:56:30.44 -05:57:19.0
195.82560 -41.24137 galactic Eri Second-epoch detections are separated by 5.9" 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 3245078556427683072 | 03:56:30.92 -05:57:23.7 (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!
TCP 2026 02 22.1474* 03 56 30.44 -05 57 19.0 12.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245078556427683072,2461093.6474,12.73,0.05,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
Gaia DR3 3245078556427683072 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:30.44 -05:57:19.0 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.87 03:55:08.87 -06:37:09.2
196.35331 -41.87306 galactic Eri Second-epoch detections are separated by 2.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3244927407936878976 | 03:55:09.30 -06:37:11.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 55 08.87 -06 37 09.2 12.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3244927407936878976,2461093.6474,12.87,0.05,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 3244927407936878976 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:08.87 -06:37:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.71 03:51:12.34 -07:41:37.3
196.93413 -43.26148 galactic Eri Second-epoch detections are separated by 2.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243215605773848320 | 03:51:11.85 -07:41:36.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 12.34 -07 41 37.3 12.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243215605773848320,2461093.6474,12.71,0.05,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 3243215605773848320 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:12.34 -07:41:37.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.79 03:50:08.56 -11:25:14.2
201.32140 -45.28553 galactic Eri Second-epoch detections are separated by 2.3" 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 5114905213125754496 | 03:50:09.19 -11:25:12.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 08.56 -11 25 14.2 12.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114905213125754496,2461093.6474,12.79,0.05,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 5114905213125754496 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:08.56 -11:25:14.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.76 03:51:54.10 -12:51:39.5
203.43103 -45.54346 galactic Eri Second-epoch detections are separated by 2.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114436821172205824 | 03:51:54.78 -12:51:34.7 (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!
TCP 2026 02 22.1474* 03 51 54.10 -12 51 39.5 12.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114436821172205824,2461093.6474,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5114436821172205824 20260222.1474 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:54.10 -12:51:39.5 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 06.99 -07 37 21.1 12.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243304219539052544,2461093.6474,12.65,0.05,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 3243304219539052544 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:06.99 -07:37:21.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.43 03:51:10.25 -11:50:47.4
202.02299 -45.25439 galactic Eri 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 | ATO J057.7905-11.8467 | 03:51:09.74 -11:50:48.4 (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!
TCP 2026 02 22.1474* 03 51 10.25 -11 50 47.4 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.7905-11.8467,2461093.6474,12.43,0.05,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
ATO J057.7905-11.8467 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:10.25 -11:50:47.4 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.43 03:56:19.91 -05:59:00.8
195.82770 -41.29335 galactic Eri Second-epoch detections are separated by 3.1" and 5.1 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 3245078006671870208 | 03:56:20.48 -05:59:04.8 (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!
TCP 2026 02 22.1474* 03 56 19.91 -05 59 00.8 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245078006671870208,2461093.6474,12.43,0.05,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 3245078006671870208 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:19.91 -05:59:00.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.47 03:56:41.54 -05:19:18.0
195.14056 -40.87158 galactic Eri Second-epoch detections are separated by 2.5" 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 3245326496299830272 | 03:56:41.28 -05:19:13.0 (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!
TCP 2026 02 22.1474* 03 56 41.54 -05 19 18.0 12.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245326496299830272,2461093.6474,12.47,0.05,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
Gaia DR3 3245326496299830272 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:41.54 -05:19:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.41 03:50:27.79 -07:27:33.2
196.52840 -43.30134 galactic Eri Second-epoch detections are separated by 3.6" 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 3243281095435123456 | 03:50:27.16 -07:27:28.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 27.79 -07 27 33.2 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243281095435123456,2461093.6474,12.41,0.05,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 3243281095435123456 20260222.1474 12.41CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:27.79 -07:27:33.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.54 03:48:47.95 -10:42:27.6
200.20667 -45.24780 galactic Eri Second-epoch detections are separated by 5.9" 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 5115733007941465728 | 03:48:48.53 -10:42:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 47.95 -10 42 27.6 12.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5115733007941465728,2461093.6474,12.54,0.05,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 5115733007941465728 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:47.95 -10:42:27.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.43 03:49:58.65 -11:44:51.0
201.70962 -45.47027 galactic Eri Second-epoch detections are separated by 2.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114842025564920832 | 03:49:59.20 -11:44:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 58.65 -11 44 51.0 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114842025564920832,2461093.6474,12.43,0.05,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 5114842025564920832 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:58.65 -11:44:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.50 03:49:23.79 -13:34:19.4
203.97624 -46.40008 galactic Eri Second-epoch detections are separated by 7.0" 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 5111010639860851072 | 03:49:24.53 -13:34:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 23.79 -13 34 19.4 12.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5111010639860851072,2461093.6474,12.50,0.05,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 5111010639860851072 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:23.79 -13:34:19.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.37 03:50:31.72 -10:23:04.2
200.08557 -44.72074 galactic Eri Second-epoch detections are separated by 3.7" 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 3194206455514179584 | 03:50:32.13 -10:23:05.8 (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!
TCP 2026 02 22.1474* 03 50 31.72 -10 23 04.2 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194206455514179584,2461093.6474,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3194206455514179584 20260222.1474 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:31.72 -10:23:04.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.24 03:51:20.43 -14:16:46.7
205.19339 -46.26978 galactic Eri Second-epoch detections are separated by 3.5" 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 5110891102331211264 | 03:51:19.99 -14:16:51.6 (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!
TCP 2026 02 22.1474* 03 51 20.43 -14 16 46.7 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5110891102331211264,2461093.6474,12.24,0.05,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 5110891102331211264 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:20.43 -14:16:46.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.38 03:53:53.64 -08:40:06.7
198.54854 -43.16879 galactic Eri Second-epoch detections are separated by 1.7" and 5.1 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 3195036689871945984 | 03:53:54.28 -08:40:07.8 (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!
TCP 2026 02 22.1474* 03 53 53.64 -08 40 06.7 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3195036689871945984,2461093.6474,12.38,0.05,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 3195036689871945984 20260222.1474 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:53.64 -08:40:06.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.37 03:50:48.88 -11:10:50.2
201.12605 -45.02909 galactic Eri Second-epoch detections are separated by 3.5" 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 5114935655853918592 | 03:50:48.26 -11:10:52.2 (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!
TCP 2026 02 22.1474* 03 50 48.88 -11 10 50.2 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114935655853918592,2461093.6474,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5114935655853918592 20260222.1474 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:48.88 -11:10:50.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.29 03:58:16.87 -05:57:10.0
196.12522 -40.86256 galactic Eri Second-epoch detections are separated by 2.1" and 5.1 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 3245070305793678592 | 03:58:17.50 -05:57:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 58 16.87 -05 57 10.0 12.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245070305793678592,2461093.6474,12.29,0.05,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 3245070305793678592 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:16.87 -05:57:10.0 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.20 03:51:17.37 -13:32:08.3
204.21190 -45.96837 galactic Eri Second-epoch detections are separated by 0.7" and 5.1 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 5111002908919745664 | 03:51:16.97 -13:32:09.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 17.37 -13 32 08.3 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5111002908919745664,2461093.6474,12.20,0.05,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 5111002908919745664 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:17.37 -13:32:08.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 04 00 43.79 -05 06 38.2 12.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245534407076378496,2461093.6474,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3245534407076378496 20260222.1474 12.31CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:00:43.79 -05:06:38.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.25 03:51:07.41 -09:49:54.7
199.50055 -44.32974 galactic Eri Second-epoch detections are separated by 2.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3194300188880417152 | 03:51:07.83 -09:49:55.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 07.41 -09 49 54.7 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194300188880417152,2461093.6474,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3194300188880417152 20260222.1474 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:07.41 -09:49:54.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.21 03:51:13.85 -11:05:04.6
201.07200 -44.89428 galactic Eri Second-epoch detections are separated by 2.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114943764752159744 | 03:51:13.33 -11:05:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 13.85 -11 05 04.6 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114943764752159744,2461093.6474,12.21,0.05,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 5114943764752159744 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:13.85 -11:05:04.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 11.71 -05 59 11.3 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245207199288769920,2461093.6474,12.15,0.05,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 3245207199288769920 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:11.71 -05:59:11.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.96 03:54:22.86 -07:06:03.4
196.78071 -42.28251 galactic Eri Second-epoch detections are separated by 0.6" and 5.1 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 3243355587347868800 | 03:54:23.40 -07:06:04.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 22.86 -07 06 03.4 12.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243355587347868800,2461093.6474,11.96,0.05,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
Gaia DR3 3243355587347868800 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:22.86 -07:06:03.4 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.03 03:57:55.22 -05:38:11.8
195.70642 -40.77557 galactic Eri Second-epoch detections are separated by 2.3" 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 3245113843877169920 | 03:57:55.65 -05:38:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 57 55.22 -05 38 11.8 12.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245113843877169920,2461093.6474,12.03,0.05,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 3245113843877169920 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:55.22 -05:38:11.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.91 03:50:22.18 -10:38:01.2
200.36977 -44.87220 galactic Eri Second-epoch detections are separated by 5.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3194183468848938240 | 03:50:22.60 -10:38:00.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 22.18 -10 38 01.2 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194183468848938240,2461093.6474,11.91,0.05,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
Gaia DR3 3194183468848938240 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:22.18 -10:38:01.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.88 03:48:11.53 -13:54:28.0
204.23788 -46.80743 galactic Eri Second-epoch detections are separated by 2.9" 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 5110974355977150336 | 03:48:11.00 -13:54:31.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 11.53 -13 54 28.0 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5110974355977150336,2461093.6474,11.88,0.05,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 5110974355977150336 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:11.53 -13:54:28.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.96 03:56:58.38 -05:27:12.1
195.33731 -40.88111 galactic Eri Second-epoch detections are separated by 1.9" 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 3245319418193796608 | 03:56:58.10 -05:27:07.7 (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!
TCP 2026 02 22.1474* 03 56 58.38 -05 27 12.1 12.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245319418193796608,2461093.6474,11.96,0.05,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
Gaia DR3 3245319418193796608 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:58.38 -05:27:12.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.95 03:51:01.64 -13:39:45.3
204.33841 -46.07998 galactic Eri Second-epoch detections are separated by 7.2" 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 J057.7599-13.6536 | 03:51:02.39 -13:39:38.3 (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!
TCP 2026 02 22.1474* 03 51 01.64 -13 39 45.3 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.7599-13.6536,2461093.6474,11.95,0.05,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
ATO J057.7599-13.6536 20260222.1474 11.95CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:01.64 -13:39:45.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.81 03:52:39.60 -08:27:33.9
198.09268 -43.33171 galactic Eri Second-epoch detections are separated by 1.7" and 5.1 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 3195102969807196672 | 03:52:39.20 -08:27:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 39.60 -08 27 33.9 11.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3195102969807196672,2461093.6474,11.81,0.05,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 3195102969807196672 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:39.60 -08:27:33.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.79 03:58:07.97 -05:02:51.9
195.08184 -40.42250 galactic Eri Second-epoch detections are separated by 1.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245711772046131200 | 03:58:08.32 -05:02:57.8 (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!
TCP 2026 02 22.1474* 03 58 07.97 -05 02 51.9 11.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245711772046131200,2461093.6474,11.79,0.05,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
Gaia DR3 3245711772046131200 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:07.97 -05:02:51.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 10.67 03:48:29.45 -13:38:59.4
203.94209 -46.63229 galactic Eri Second-epoch detections are separated by 1.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5113987395794753920 | 03:48:28.93 -13:39:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6V 1988MSS...C04....0H HD 23926
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 29.45 -13 38 59.4 10.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5113987395794753920,2461093.6474,10.67,0.05,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 5113987395794753920 20260222.1474 10.67CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:29.45 -13:38:59.4 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 10.14 03:51:01.28 -06:03:40.1
194.99229 -42.46054 galactic Eri Second-epoch detections are separated by 0.7" and 5.1 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 3245214341816910848 | 03:51:01.77 -06:03:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 01.28 -06 03 40.1 10.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245214341816910848,2461093.6474,10.14,0.05,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 3245214341816910848 20260222.1474 10.14CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:01.28 -06:03:40.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 10.35 03:46:50.24 -09:23:17.5
198.23633 -45.04050 galactic Eri Second-epoch detections are separated by 2.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3194560360817840384 | 03:46:50.79 -09:23:17.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 46 50.24 -09 23 17.5 10.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194560360817840384,2461093.6474,10.35,0.05,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 3194560360817840384 20260222.1474 10.35CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:50.24 -09:23:17.5 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.06 03:56:14.05 -04:59:47.0
194.69574 -40.79708 galactic Eri Second-epoch detections are separated by 1.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245399338945155968 | 03:56:14.51 -04:59:51.0 (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!
TCP 2026 02 22.1474* 03 56 14.05 -04 59 47.0 11.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245399338945155968,2461093.6474,11.06,0.05,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
Gaia DR3 3245399338945155968 20260222.1474 11.06CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:14.05 -04:59:47.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.38 03:47:17.61 -08:57:18.8
197.78203 -44.72980 galactic Eri Second-epoch detections are separated by 3.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3242639908356200320 | 03:47:18.21 -08:57:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 47 17.61 -08 57 18.8 11.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3242639908356200320,2461093.6474,11.38,0.05,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 3242639908356200320 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:17.61 -08:57:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.32 03:53:38.64 -06:06:30.3
195.50637 -41.92927 galactic Eri Second-epoch detections are separated by 6.4" and 6.4 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 3245155144285145344 | 03:53:39.04 -06:06:33.0 (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!
TCP 2026 02 22.1474* 03 53 38.64 -06 06 30.3 11.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245155144285145344,2461093.6474,11.32,0.05,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
Gaia DR3 3245155144285145344 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:38.64 -06:06:30.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.49 03:47:15.12 -11:04:31.1
200.41767 -45.75530 galactic Eri Second-epoch detections are separated by 2.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5115691329579070720 | 03:47:15.63 -11:04:30.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 47 15.12 -11 04 31.1 11.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5115691329579070720,2461093.6474,11.49,0.05,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
Gaia DR3 5115691329579070720 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:15.12 -11:04:31.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 09.70 -05 59 11.9 11.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245207199288769920,2461093.6474,11.46,0.05,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 3245207199288769920 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:09.70 -05:59:11.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.46 03:48:04.92 -10:12:38.2
199.46659 -45.16850 galactic Eri Second-epoch detections are separated by 2.8" and 5.1 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 3194271635937435392 | 03:48:05.45 -10:12:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 04.92 -10 12 38.2 11.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194271635937435392,2461093.6474,11.46,0.05,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 3194271635937435392 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:04.92 -10:12:38.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.64 03:52:53.79 -06:32:50.3
195.88265 -42.31557 galactic Eri Second-epoch detections are separated by 3.2" and 5.1 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 3243624692818901632 | 03:52:54.59 -06:32:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 53.79 -06 32 50.3 11.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243624692818901632,2461093.6474,11.64,0.05,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 3243624692818901632 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:53.79 -06:32:50.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.57 03:51:42.07 -05:02:28.9
193.94701 -41.77685 galactic Eri Second-epoch detections are separated by 2.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3246087839383376512 | 03:51:42.60 -05:02:33.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 42.07 -05 02 28.9 11.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246087839383376512,2461093.6474,11.57,0.05,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 3246087839383376512 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:42.07 -05:02:28.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 55 42.76 -05 26 22.7 11.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245345875192288256,2461093.6474,11.56,0.05,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 3245345875192288256 20260222.1474 11.56CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:42.76 -05:26:22.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.68 03:54:51.91 -06:50:12.3
196.55643 -42.04461 galactic Eri Second-epoch detections are separated by 5.5" and 6.0 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 3244914110719991424 | 03:54:52.39 -06:50:14.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 51.91 -06 50 12.3 11.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3244914110719991424,2461093.6474,11.68,0.05,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 3244914110719991424 20260222.1474 11.68CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:51.91 -06:50:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.86 03:51:16.97 -06:20:49.9
195.36920 -42.55460 galactic Eri Second-epoch detections are separated by 4.5" 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 3243692518942374016 | 03:51:17.48 -06:20:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 16.97 -06 20 49.9 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243692518942374016,2461093.6474,11.86,0.05,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 3243692518942374016 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:16.97 -06:20:49.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.88 03:54:59.77 -05:12:33.3
194.71908 -41.17128 galactic Eri Second-epoch detections are separated by 5.1" 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 3245366284876821632 | 03:55:00.53 -05:12:38.7 (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!
TCP 2026 02 22.1474* 03 54 59.77 -05 12 33.3 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245366284876821632,2461093.6474,11.88,0.05,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 3245366284876821632 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:59.77 -05:12:33.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.62 03:56:36.47 -05:21:11.7
195.16151 -40.90607 galactic Eri Second-epoch detections are separated by 7.0" and 6.5 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 3245324670937120000 | 03:56:36.80 -05:21:16.7 (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!
TCP 2026 02 22.1474* 03 56 36.47 -05 21 11.7 11.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245324670937120000,2461093.6474,11.62,0.05,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 3245324670937120000 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:36.47 -05:21:11.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.85 03:47:30.11 -09:29:34.2
198.47848 -44.94841 galactic Eri Second-epoch detections are separated by 3.1" and 5.1 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 3194569500508245632 | 03:47:30.76 -09:29:32.7 (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!
TCP 2026 02 22.1474* 03 47 30.11 -09 29 34.2 11.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194569500508245632,2461093.6474,11.85,0.05,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
Gaia DR3 3194569500508245632 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:30.11 -09:29:34.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.90 03:45:20.32 -12:52:19.7
202.43232 -46.98641 galactic Eri Second-epoch detections are separated by 2.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114274948147331456 | 03:45:20.64 -12:52:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 45 20.32 -12 52 19.7 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114274948147331456,2461093.6474,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5114274948147331456 20260222.1474 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:20.32 -12:52:19.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.00 03:53:28.67 -05:39:12.4
194.95695 -41.72654 galactic Eri Second-epoch detections are separated by 3.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245256986549566848 | 03:53:29.58 -05:39:16.8 (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!
TCP 2026 02 22.1474* 03 53 28.67 -05 39 12.4 12.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245256986549566848,2461093.6474,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3245256986549566848 20260222.1474 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:28.67 -05:39:12.4 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.98 03:54:40.31 -05:39:20.5
195.16800 -41.47488 galactic Eri Second-epoch detections are separated by 2.5" 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 3245242555459507328 | 03:54:41.18 -05:39:29.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 40.31 -05 39 20.5 12.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245242555459507328,2461093.6474,11.98,0.05,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 3245242555459507328 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:40.31 -05:39:20.5 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 11.95 03:54:47.91 -05:35:42.9
195.12137 -41.41635 galactic Eri Second-epoch detections are separated by 1.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245337766294053248 | 03:54:48.65 -05:35:47.3 (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!
TCP 2026 02 22.1474* 03 54 47.91 -05 35 42.9 11.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245337766294053248,2461093.6474,11.95,0.05,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 3245337766294053248 20260222.1474 11.95CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:47.91 -05:35:42.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.05 03:49:55.70 -05:29:45.7
194.14770 -42.39273 galactic Eri Second-epoch detections are separated by 3.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3246048703641449856 | 03:49:56.39 -05:29:48.7 (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!
TCP 2026 02 22.1474* 03 49 55.70 -05 29 45.7 12.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246048703641449856,2461093.6474,12.05,0.05,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 3246048703641449856 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:55.70 -05:29:45.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.01 03:52:10.18 -06:23:21.0
195.57310 -42.38820 galactic Eri Second-epoch detections are separated by 1.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243645239942444160 | 03:52:10.81 -06:23:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 10.18 -06 23 21.0 12.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243645239942444160,2461093.6474,12.01,0.05,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 3243645239942444160 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:10.18 -06:23:21.0 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.06 03:51:06.92 -07:35:27.9
196.79705 -43.22894 galactic Eri Second-epoch detections are separated by 4.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243264254866300672 | 03:51:07.50 -07:35:30.0 (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!
TCP 2026 02 22.1474* 03 51 06.92 -07 35 27.9 12.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243264254866300672,2461093.6474,12.06,0.05,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
Gaia DR3 3243264254866300672 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:06.92 -07:35:27.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.10 03:47:24.78 -10:47:34.8
200.08679 -45.58855 galactic Eri Second-epoch detections are separated by 2.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5115750050371718784 | 03:47:25.50 -10:47:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 47 24.78 -10 47 34.8 12.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5115750050371718784,2461093.6474,12.10,0.05,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 5115750050371718784 20260222.1474 12.10CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:24.78 -10:47:34.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.11 03:50:39.84 -04:53:12.3
193.58580 -41.91185 galactic Eri Second-epoch detections are separated by 2.7" and 6.0 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 3246108180348438016 | 03:50:40.57 -04:53:17.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 39.84 -04 53 12.3 12.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246108180348438016,2461093.6474,12.11,0.05,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 3246108180348438016 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:39.84 -04:53:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.20 03:53:25.75 -06:06:09.0
195.46221 -41.97179 galactic Eri Second-epoch detections are separated by 0.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245158099222647040 | 03:53:26.47 -06:06:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 25.75 -06 06 09.0 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245158099222647040,2461093.6474,12.20,0.05,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 3245158099222647040 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:25.75 -06:06:09.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 35.11 -05 57 30.5 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245183761649810688,2461093.6474,12.21,0.05,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 3245183761649810688 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:35.11 -05:57:30.5 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.26 03:54:00.28 -06:14:11.3
195.71602 -41.91916 galactic Eri Second-epoch detections are separated by 1.2" 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 3245140743257978496 | 03:54:01.05 -06:14:14.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 00.28 -06 14 11.3 12.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245140743257978496,2461093.6474,12.26,0.05,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 3245140743257978496 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:00.28 -06:14:11.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.15 03:48:24.18 -07:39:24.9
196.40488 -43.84148 galactic Eri 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 3243438944072100608 | 03:48:23.86 -07:39:20.7 (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!
TCP 2026 02 22.1474* 03 48 24.18 -07 39 24.9 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243438944072100608,2461093.6474,12.15,0.05,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 3243438944072100608 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:24.18 -07:39:24.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.18 03:53:12.76 -06:55:24.3
196.37405 -42.44147 galactic Eri Second-epoch detections are separated by 1.3" 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 3243420939570172800 | 03:53:13.29 -06:55:25.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 12.76 -06 55 24.3 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243420939570172800,2461093.6474,12.18,0.05,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 3243420939570172800 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:12.76 -06:55:24.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.17 03:46:38.86 -10:32:48.7
199.64979 -45.63853 galactic Eri Second-epoch detections are separated by 5.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5115794786751021696 | 03:46:39.39 -10:32:50.8 (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!
TCP 2026 02 22.1474* 03 46 38.86 -10 32 48.7 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5115794786751021696,2461093.6474,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5115794786751021696 20260222.1474 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:38.86 -10:32:48.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.26 03:49:52.35 -06:40:42.8
195.50688 -43.02610 galactic Eri Second-epoch detections are separated by 5.4" 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 3243656544296338944 | 03:49:52.83 -06:40:41.7 (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!
TCP 2026 02 22.1474* 03 49 52.35 -06 40 42.8 12.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243656544296338944,2461093.6474,12.26,0.05,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 3243656544296338944 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:52.35 -06:40:42.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.35 03:57:40.59 -05:12:07.6
195.17603 -40.60029 galactic Eri Second-epoch detections are separated by 3.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245334021082583168 | 03:57:41.12 -05:12:10.8 (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!
TCP 2026 02 22.1474* 03 57 40.59 -05 12 07.6 12.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245334021082583168,2461093.6474,12.35,0.05,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 3245334021082583168 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:40.59 -05:12:07.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.24 03:53:53.55 -05:56:24.4
195.35672 -41.78883 galactic Eri Second-epoch detections are separated by 3.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245184006465358080 | 03:53:54.09 -05:56:27.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 53.55 -05 56 24.4 12.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245184006465358080,2461093.6474,12.24,0.05,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 3245184006465358080 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:53.55 -05:56:24.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.33 03:52:58.61 -05:51:53.9
195.11083 -41.94363 galactic Eri Second-epoch detections are separated by 5.2" 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 3245235305554671232 | 03:52:59.31 -05:51:56.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 58.61 -05 51 53.9 12.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245235305554671232,2461093.6474,12.33,0.05,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
Gaia DR3 3245235305554671232 20260222.1474 12.33CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:58.61 -05:51:53.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.39 03:49:45.41 -09:22:03.7
198.70459 -44.40152 galactic Eri Second-epoch detections are separated by 1.3" 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 3194619150331187456 | 03:49:46.18 -09:22:05.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 45.41 -09 22 03.7 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194619150331187456,2461093.6474,12.39,0.05,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 3194619150331187456 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:45.41 -09:22:03.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.49 03:53:57.80 -05:02:32.7
194.34966 -41.30089 galactic Eri Second-epoch detections are separated by 4.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3246124432504405504 | 03:53:58.36 -05:02:38.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 57.80 -05 02 32.7 12.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246124432504405504,2461093.6474,12.49,0.05,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 3246124432504405504 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:57.80 -05:02:32.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.45 03:47:33.56 -09:33:17.3
198.56476 -44.96613 galactic Eri Second-epoch detections are separated by 5.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3194542699912320384 | 03:47:34.13 -09:33:18.8 (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!
TCP 2026 02 22.1474* 03 47 33.56 -09 33 17.3 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194542699912320384,2461093.6474,12.45,0.05,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 3194542699912320384 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:33.56 -09:33:17.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.43 03:56:32.99 -04:52:02.6
194.60630 -40.66206 galactic Eri Second-epoch detections are separated by 1.8" and 5.1 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 3245402019004738688 | 03:56:33.44 -04:52:08.7 (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!
TCP 2026 02 22.1474* 03 56 32.99 -04 52 02.6 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245402019004738688,2461093.6474,12.43,0.05,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 3245402019004738688 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:32.99 -04:52:02.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.52 03:50:23.30 -05:41:52.9
194.46178 -42.40300 galactic Eri Second-epoch detections are separated by 4.5" 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 3245989845409633408 | 03:50:24.09 -05:41:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 23.30 -05 41 52.9 12.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245989845409633408,2461093.6474,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3245989845409633408 20260222.1474 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:23.30 -05:41:52.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.44 03:48:28.71 -08:05:35.8
196.94074 -44.04616 galactic Eri Second-epoch detections are separated by 2.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3242848987364240768 | 03:48:29.11 -08:05:34.8 (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!
TCP 2026 02 22.1474* 03 48 28.71 -08 05 35.8 12.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3242848987364240768,2461093.6474,12.44,0.05,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 3242848987364240768 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:28.71 -08:05:35.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.59 03:50:52.66 -04:59:02.1
193.73435 -41.91921 galactic Eri Second-epoch detections are separated by 4.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3246103851021406720 | 03:50:53.28 -04:59:08.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 52.66 -04 59 02.1 12.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246103851021406720,2461093.6474,12.59,0.05,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 3246103851021406720 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:52.66 -04:59:02.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 16.16 -05 34 06.2 12.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245247778139738880,2461093.6474,12.59,0.05,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 3245247778139738880 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:16.16 -05:34:06.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.54 03:51:00.45 -10:28:37.6
200.27839 -44.66037 galactic Eri Second-epoch detections are separated by 2.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3194192917776969856 | 03:51:01.12 -10:28:40.0 (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!
TCP 2026 02 22.1474* 03 51 00.45 -10 28 37.6 12.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194192917776969856,2461093.6474,12.54,0.05,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 3194192917776969856 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:00.45 -10:28:37.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.65 03:49:13.07 -06:44:31.1
195.46564 -43.19796 galactic Eri Second-epoch detections are separated by 5.8" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J057.3063-06.7410 | 03:49:13.52 -06:44:27.8 (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!
TCP 2026 02 22.1474* 03 49 13.07 -06 44 31.1 12.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.3063-06.7410,2461093.6474,12.65,0.05,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 J057.3063-06.7410 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:13.07 -06:44:31.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.62 03:45:42.04 -10:21:56.1
199.26310 -45.75737 galactic Eri Second-epoch detections are separated by 0.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5115966001326994048 | 03:45:42.61 -10:21:52.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 45 42.04 -10 21 56.1 12.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5115966001326994048,2461093.6474,12.62,0.05,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 5115966001326994048 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:42.04 -10:21:56.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.65 03:52:21.39 -06:29:02.3
195.71546 -42.39765 galactic Eri Second-epoch detections are separated by 1.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243640738816723456 | 03:52:21.99 -06:29:03.8 (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!
TCP 2026 02 22.1474* 03 52 21.39 -06 29 02.3 12.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243640738816723456,2461093.6474,12.65,0.05,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 3243640738816723456 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:21.39 -06:29:02.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.51 03:50:43.83 -06:06:51.7
195.00235 -42.55001 galactic Eri Second-epoch detections are separated by 5.5" and 5.9 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 3243712516307645184 | 03:50:44.20 -06:07:01.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 43.83 -06 06 51.7 12.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243712516307645184,2461093.6474,12.51,0.05,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 3243712516307645184 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:43.83 -06:06:51.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.54 03:48:54.77 -07:15:38.7
196.02321 -43.53044 galactic Eri Second-epoch detections are separated by 6.9" and 6.5 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 3243479381188049792 | 03:48:55.31 -07:15:39.0 (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!
TCP 2026 02 22.1474* 03 48 54.77 -07 15 38.7 12.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243479381188049792,2461093.6474,12.54,0.05,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 3243479381188049792 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:54.77 -07:15:38.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.62 03:54:57.51 -06:07:57.3
195.76166 -41.66257 galactic Eri Second-epoch detections are separated by 2.4" and 5.1 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 3245163802937586688 | 03:54:58.07 -06:08:02.7 (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!
TCP 2026 02 22.1474* 03 54 57.51 -06 07 57.3 12.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3245163802937586688,2461093.6474,12.62,0.05,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
Large-amplitude variable Gaia DR2 3245163802937586688 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:57.51 -06:07:57.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.70 03:52:51.64 -04:58:03.3
194.07013 -41.49336 galactic Eri Second-epoch detections are separated by 3.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3246136183532905984 | 03:52:52.04 -04:58:07.5 (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!
TCP 2026 02 22.1474* 03 52 51.64 -04 58 03.3 12.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246136183532905984,2461093.6474,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3246136183532905984 20260222.1474 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:51.64 -04:58:03.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.59 03:45:29.41 -12:19:17.7
201.73538 -46.70843 galactic Eri Second-epoch detections are separated by 8.2" and 6.1 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 5114379302968794496 | 03:45:29.90 -12:19:18.7 (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!
TCP 2026 02 22.1474* 03 45 29.41 -12 19 17.7 12.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114379302968794496,2461093.6474,12.59,0.05,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 5114379302968794496 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:29.41 -12:19:17.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.70 03:52:27.23 -06:36:05.1
195.86857 -42.43766 galactic Eri Second-epoch detections are separated by 0.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243625517452634496 | 03:52:27.98 -06:36:05.1 (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!
TCP 2026 02 22.1474* 03 52 27.23 -06 36 05.1 12.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243625517452634496,2461093.6474,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3243625517452634496 20260222.1474 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:27.23 -06:36:05.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.61 03:51:03.18 -07:59:49.9
197.26875 -43.44680 galactic Eri Second-epoch detections are separated by 7.7" and 6.0 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 3243171556589339392 | 03:51:03.79 -07:59:53.6 (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!
TCP 2026 02 22.1474* 03 51 03.18 -07 59 49.9 12.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243171556589339392,2461093.6474,12.61,0.05,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 3243171556589339392 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:03.18 -07:59:49.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.77 03:53:09.15 -05:20:16.3
194.54083 -41.62879 galactic Eri Second-epoch detections are separated by 5.9" 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 3246017504996806016 | 03:53:09.79 -05:20:22.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 09.15 -05 20 16.3 12.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246017504996806016,2461093.6474,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3246017504996806016 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:09.15 -05:20:16.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.63 03:53:16.85 -07:58:02.8
197.61170 -42.95425 galactic Eri Second-epoch detections are separated by 2.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3195156399200280832 | 03:53:17.51 -07:58:05.8 (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!
TCP 2026 02 22.1474* 03 53 16.85 -07 58 02.8 12.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3195156399200280832,2461093.6474,12.63,0.05,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 3195156399200280832 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:16.85 -07:58:02.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 12.61 -07 26 09.0 12.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243276010193881344,2461093.6474,12.71,0.05,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 3243276010193881344 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:12.61 -07:26:09.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.65 03:49:16.30 -12:08:49.6
202.10879 -45.80434 galactic Eri Second-epoch detections are separated by 7.6" and 6.8 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 5114723724987268864 | 03:49:16.68 -12:08:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 16.30 -12 08 49.6 12.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114723724987268864,2461093.6474,12.65,0.05,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 5114723724987268864 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:16.30 -12:08:49.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.84 03:46:42.80 -12:29:04.6
202.14201 -46.51415 galactic Eri Second-epoch detections are separated by 3.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114324636624116736 | 03:46:43.78 -12:29:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 46 42.80 -12 29 04.6 12.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114324636624116736,2461093.6474,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5114324636624116736 20260222.1474 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:42.80 -12:29:04.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.84 03:54:29.15 -06:23:45.2
195.98245 -41.89926 galactic Eri Second-epoch detections are separated by 5.7" 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 3244946443233703936 | 03:54:29.84 -06:23:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 29.15 -06 23 45.2 12.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3244946443233703936,2461093.6474,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3244946443233703936 20260222.1474 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:29.15 -06:23:45.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.87 03:53:13.71 -05:17:15.6
194.49731 -41.58615 galactic Eri Second-epoch detections are separated by 8.0" 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 3246111685041481856 | 03:53:14.60 -05:17:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1986AJ.....91..144S StKM 1- 425
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 13.71 -05 17 15.6 12.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246111685041481856,2461093.6474,12.87,0.05,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 3246111685041481856 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:13.71 -05:17:15.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 35.63 -05 20 32.1 12.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LN Eri,2461093.6474,12.95,0.05,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
LN Eri 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:35.63 -05:20:32.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.93 03:54:00.85 -05:50:16.1
195.26097 -41.70959 galactic Eri Second-epoch detections are separated by 3.9" and 6.0 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 3245233450128860416 | 03:54:01.57 -05:50:22.3 (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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 00.85 -05 50 16.1 12.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245233450128860416,2461093.6474,12.93,0.05,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 3245233450128860416 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:00.85 -05:50:16.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.93 03:51:47.94 -06:46:27.0
195.95570 -42.66604 galactic Eri Second-epoch detections are separated by 7.8" 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 | Large-amplitude variable Gaia DR2 3243616652640163456 | 03:51:48.54 -06:46:31.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 47.94 -06 46 27.0 12.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3243616652640163456,2461093.6474,12.93,0.05,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
Large-amplitude variable Gaia DR2 3243616652640163456 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:47.94 -06:46:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.98 03:51:05.65 -05:43:06.9
194.61099 -42.26484 galactic Eri Second-epoch detections are separated by 5.7" 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 3245982836023363072 | 03:51:03.11 -05:43:02.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 05.65 -05 43 06.9 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245982836023363072,2461093.6474,12.98,0.05,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 3245982836023363072 20260222.1474 12.98CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:05.65 -05:43:06.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.06 03:53:18.55 -05:36:01.7
194.86700 -41.73436 galactic Eri Second-epoch detections are separated by 6.9" and 6.7 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 3245258253562583808 | 03:53:19.07 -05:36:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 18.55 -05 36 01.7 13.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245258253562583808,2461093.6474,13.06,0.05,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
Gaia DR3 3245258253562583808 20260222.1474 13.06CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:18.55 -05:36:01.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 05.67 -10 23 58.4 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194250332899724416,2461093.6474,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3194250332899724416 20260222.1474 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:05.67 -10:23:58.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.01 03:49:13.92 -11:31:15.1
201.30321 -45.52981 galactic Eri Second-epoch detections are separated by 8.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114899921726066688 | 03:49:14.61 -11:31:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 13.92 -11 31 15.1 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114899921726066688,2461093.6474,13.01,0.05,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 5114899921726066688 20260222.1474 13.01CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:13.92 -11:31:15.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.01 03:52:54.55 -10:44:44.4
200.91720 -44.37227 galactic Eri Second-epoch detections are separated by 8.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3193420025524763136 | 03:52:55.18 -10:44:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 54.55 -10 44 44.4 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3193420025524763136,2461093.6474,13.01,0.05,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 3193420025524763136 20260222.1474 13.01CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:54.55 -10:44:44.4 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 36.18 -05 19 55.9 13.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246110722968806016,2461093.6474,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3246110722968806016 20260222.1474 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:36.18 -05:19:55.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 12.98 03:54:53.27 -05:16:25.5
194.77293 -41.22826 galactic Eri Second-epoch detections are separated by 8.1" and 5.1 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 3245364292011998336 | 03:54:53.88 -05:16:32.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 53.27 -05 16 25.5 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245364292011998336,2461093.6474,12.98,0.05,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 3245364292011998336 20260222.1474 12.98CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:53.27 -05:16:25.5 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 37.69 -06 41 51.0 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243665031151732864,2461093.6474,12.96,0.05,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 3243665031151732864 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:37.69 -06:41:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.05 03:50:22.16 -05:07:34.8
193.80473 -42.10244 galactic Eri Second-epoch detections are separated by 3.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J057.5936-05.1276 | 03:50:22.47 -05:07:39.4 (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!
TCP 2026 02 22.1474* 03 50 22.16 -05 07 34.8 13.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.5936-05.1276,2461093.6474,13.05,0.05,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
ATO J057.5936-05.1276 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:22.16 -05:07:34.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.03 03:48:05.25 -05:33:39.4
193.89036 -42.81483 galactic Eri Second-epoch detections are separated by 7.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3244555773007764352 | 03:48:05.73 -05:33:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 05.25 -05 33 39.4 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3244555773007764352,2461093.6474,13.03,0.05,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 3244555773007764352 20260222.1474 13.03CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:05.25 -05:33:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.04 03:49:29.23 -08:49:23.1
197.99536 -44.19327 galactic Eri Second-epoch detections are separated by 5.9" and 5.8 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 3194700548551278208 | 03:49:30.11 -08:49:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 29.23 -08 49 23.1 13.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194700548551278208,2461093.6474,13.04,0.05,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 3194700548551278208 20260222.1474 13.04CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:29.23 -08:49:23.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.13 03:46:46.74 -12:06:13.6
201.65851 -46.32920 galactic Eri Second-epoch detections are separated by 5.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114762409756508160 | 03:46:47.40 -12:06:18.8 (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!
TCP 2026 02 22.1474* 03 46 46.74 -12 06 13.6 13.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114762409756508160,2461093.6474,13.13,0.05,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 5114762409756508160 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:46.74 -12:06:13.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.12 03:53:23.28 -08:03:23.7
197.73539 -42.97565 galactic Eri Second-epoch detections are separated by 5.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3195154475054980480 | 03:53:23.88 -08:03:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 23.28 -08 03 23.7 13.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3195154475054980480,2461093.6474,13.12,0.05,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 3195154475054980480 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:23.28 -08:03:23.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.14 03:52:02.44 -07:25:59.2
196.76958 -42.95117 galactic Eri Second-epoch detections are separated by 8.4" and 6.4 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 3243366204506997760 | 03:52:02.93 -07:26:05.1 (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!
TCP 2026 02 22.1474* 03 52 02.44 -07 25 59.2 13.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243366204506997760,2461093.6474,13.14,0.05,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 3243366204506997760 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:02.44 -07:25:59.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.36 03:49:10.95 -09:54:26.1
199.27260 -44.78564 galactic Eri Second-epoch detections are separated by 1.5" 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 3194283558766692864 | 03:49:11.60 -09:54:28.7 (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!
TCP 2026 02 22.1474* 03 49 10.95 -09 54 26.1 13.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3194283558766692864,2461093.6474,13.36,0.05,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 3194283558766692864 20260222.1474 13.36CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:10.95 -09:54:26.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.31 03:48:41.59 -12:05:57.5
201.95641 -45.90930 galactic Eri Second-epoch detections are separated by 8.1" and 6.1 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 5114735338578840064 | 03:48:42.03 -12:05:58.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 41.59 -12 05 57.5 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114735338578840064,2461093.6474,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5114735338578840064 20260222.1474 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:41.59 -12:05:57.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.25 03:55:44.62 -05:29:04.3
195.16008 -41.15804 galactic Eri Second-epoch detections are separated by 2.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J058.9381-05.4864 | 03:55:45.16 -05:29:11.4 (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!
TCP 2026 02 22.1474* 03 55 44.62 -05 29 04.3 13.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J058.9381-05.4864,2461093.6474,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J058.9381-05.4864 20260222.1474 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:44.62 -05:29:04.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.27 03:51:14.16 -06:52:12.2
195.96967 -42.83522 galactic Eri Second-epoch detections are separated by 6.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243590882836404480 | 03:51:14.62 -06:52:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 14.16 -06 52 12.2 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243590882836404480,2461093.6474,13.27,0.05,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 3243590882836404480 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:14.16 -06:52:12.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.35 03:56:23.12 -05:37:39.4
195.43287 -41.09685 galactic Eri Second-epoch detections are separated by 3.5" 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 3245292686317357184 | 03:56:23.89 -05:37:45.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 56 23.12 -05 37 39.4 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245292686317357184,2461093.6474,13.35,0.05,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 3245292686317357184 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:23.12 -05:37:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.27 03:51:14.97 -06:55:24.5
196.03451 -42.85982 galactic Eri Second-epoch detections are separated by 3.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243587618661262976 | 03:51:15.22 -06:55:30.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 14.97 -06 55 24.5 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243587618661262976,2461093.6474,13.27,0.05,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 3243587618661262976 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:14.97 -06:55:24.5 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.34 03:45:57.50 -13:00:00.6
202.69797 -46.90705 galactic Eri Second-epoch detections are separated by 6.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114269175711287680 | 03:45:58.18 -13:00:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 45 57.50 -13 00 00.6 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114269175711287680,2461093.6474,13.34,0.05,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 5114269175711287680 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:57.50 -13:00:00.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.44 03:49:30.50 -05:57:56.4
194.61321 -42.73025 galactic Eri Second-epoch detections are separated by 2.9" 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 3244471415553949440 | 03:49:30.90 -05:57:57.4 (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 LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 30.50 -05 57 56.4 13.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3244471415553949440,2461093.6474,13.44,0.05,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 3244471415553949440 20260222.1474 13.44CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:30.50 -05:57:56.4 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 22.35 -13 59 10.0 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.6474,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.1474 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:22.35 -13:59:10.0 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.32 03:46:47.29 -14:12:46.3
204.43373 -47.24467 galactic Eri Second-epoch detections are separated by 7.5" and 5.8 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 5110868905940652416 | 03:46:47.89 -14:12:48.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 46 47.29 -14 12 46.3 13.3 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5110868905940652416,2461093.6474,13.32,0.05,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 5110868905940652416 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:47.29 -14:12:46.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.41 03:52:39.44 -06:27:58.6
195.74731 -42.32455 galactic Eri Second-epoch detections are separated by 2.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243629434462793472 | 03:52:40.33 -06:28:03.5 (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!
TCP 2026 02 22.1474* 03 52 39.44 -06 27 58.6 13.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243629434462793472,2461093.6474,13.41,0.05,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 3243629434462793472 20260222.1474 13.41CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:39.44 -06:27:58.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.41 03:50:11.46 -05:40:10.7
194.39394 -42.42959 galactic Eri Second-epoch detections are separated by 4.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3245990566964140672 | 03:50:12.16 -05:40:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 11.46 -05 40 10.7 13.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3245990566964140672,2461093.6474,13.41,0.05,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 3245990566964140672 20260222.1474 13.41CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:11.46 -05:40:10.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 45 58.17 -13 42 45.1 13.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5113904584528119040,2461093.6474,13.51,0.05,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 5113904584528119040 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:58.17 -13:42:45.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 53 35.22 -07 11 51.7 13.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.43,0.05,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
target 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:35.22 -07:11:51.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.49 03:46:47.74 -12:06:34.6
201.66871 -46.32820 galactic Eri Second-epoch detections are separated by 3.3" and 5.1 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 5114762409756508160 | 03:46:47.40 -12:06:18.8 (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!
TCP 2026 02 22.1474* 03 46 47.74 -12 06 34.6 13.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114762409756508160,2461093.6474,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5114762409756508160 20260222.1474 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:47.74 -12:06:34.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.45 03:46:17.90 -09:16:18.0
198.00028 -45.09938 galactic Eri Second-epoch detections are separated by 5.7" and 6.3 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 3242627195252811648 | 03:46:18.61 -09:16:11.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 46 17.90 -09 16 18.0 13.4 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3242627195252811648,2461093.6474,13.45,0.05,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 3242627195252811648 20260222.1474 13.45CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:17.90 -09:16:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.46 03:49:31.78 -06:21:59.4
195.08212 -42.93627 galactic Eri Second-epoch detections are separated by 8.5" and 6.1 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 3243677984773015040 | 03:49:31.49 -06:22:16.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 31.78 -06 21 59.4 13.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243677984773015040,2461093.6474,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3243677984773015040 20260222.1474 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:31.78 -06:21:59.4 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 49 09.21 -04 53 26.6 13.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.64,0.05,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
target 20260222.1474 13.64CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:09.21 -04:53:26.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.53 03:48:47.37 -07:04:15.4
195.77712 -43.45908 galactic Eri Second-epoch detections are separated by 2.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3243502406508779520 | 03:48:47.80 -07:04:24.4 (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!
TCP 2026 02 22.1474* 03 48 47.37 -07 04 15.4 13.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3243502406508779520,2461093.6474,13.53,0.05,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 3243502406508779520 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:47.37 -07:04:15.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 19.53 -07 01 56.8 13.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1474 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:19.53 -07:01:56.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.64 03:47:52.61 -07:39:54.1
196.32246 -43.95782 galactic Eri Second-epoch detections are separated by 2.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:47:52.61 -07:39:54.1 (user input) | T | P | (position from user input) J-Ks=0.988+/-0.069 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 47 52.61 -07 39 54.1 13.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.64,0.05,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
target 20260222.1474 13.64CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:52.61 -07:39:54.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 51 58.89 -05 21 18.0 13.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246031072798377600,2461093.6474,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3246031072798377600 20260222.1474 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:58.89 -05:21:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.67 03:50:42.21 -05:24:56.6
194.19462 -42.18667 galactic Eri Second-epoch detections are separated by 2.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3246004310859458688 | 03:50:43.43 -05:24:48.7 (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!
TCP 2026 02 22.1474* 03 50 42.21 -05 24 56.6 13.7 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246004310859458688,2461093.6474,13.67,0.05,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 3246004310859458688 20260222.1474 13.67CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:42.21 -05:24:56.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.79 03:45:58.57 -13:00:19.2
202.70755 -46.90541 galactic Eri Second-epoch detections are separated by 1.2" 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 5114269175711287680 | 03:45:58.18 -13:00:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 45 58.57 -13 00 19.2 13.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114269175711287680,2461093.6474,13.79,0.05,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 5114269175711287680 20260222.1474 13.79CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:58.57 -13:00:19.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 24.95 -05 44 42.6 13.8 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.82,0.05,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 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:24.95 -05:44:42.6 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 48 38.60 -14 03 40.0 13.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.87,0.05,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 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:38.60 -14:03:40.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 57 05.95 -05 03 13.2 13.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.93,0.05,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
target 20260222.1474 13.93CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:05.95 -05:03:13.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 06.88 -04 52 12.9 13.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.88,0.05,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
target 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:06.88 -04:52:12.9 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 46 47.65 -10 56 48.2 13.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5115741219918972160,2461093.6474,13.93,0.05,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 5115741219918972160 20260222.1474 13.93CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:47.65 -10:56:48.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 52 04.14 -05 16 08.8 13.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1474 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:04.14 -05:16:08.8 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 07.04 -05 18 05.7 14.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1474 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:07.04 -05:18:05.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 44.24 -05 12 59.0 14.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3246078764115230080,2461093.6474,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3246078764115230080 20260222.1474 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:44.24 -05:12:59.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 54 46.08 -06 19 35.2 14.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1474 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:46.08 -06:19:35.2 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 55 30.03 -05 33 14.0 14.0 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1474 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:30.03 -05:33:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 50 07.49 -05 30 36.3 13.9 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,13.93,0.05,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
target 20260222.1474 13.93CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:07.49 -05:30:36.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 03 45 24.39 -13 46 57.7 14.1 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6474,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1474 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:24.39 -13:46:57.7 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 04 20 19.44 -10 24 25.3 11.5 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AF Eri,2461093.6474,11.53,0.05,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
AF Eri 20260222.1474 11.53CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:20:19.44 -10:24:25.3 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1474 2461093.6474 13.56 04:26:52.04 -08:40:15.7
203.56492 -35.99097 galactic Eri Second-epoch detections are separated by 5.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3197858685246280192 | 04:26:53.38 -08:39:52.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 04 26 52.04 -08 40 15.7 13.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3197858685246280192,2461093.6474,13.56,0.05,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 3197858685246280192 20260222.1474 13.56CV 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:52.04 -08:40:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1474* 04 12 38.53 -07 47 54.1 11.6 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J041239-0747.8,2461093.6474,11.62,0.05,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
ASAS J041239-0747.8 20260222.1474 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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:38.53 -07:47:54.1 ;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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20_00sec_-14_90C_LIGHT_0076_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: 2461032.72253780 23.12.2025 05:20:17.266 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461032.72253780 23.12.2025 05:20:17.266 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461093.64766487 22.02.2026 03:32:28.245 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 143
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
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: 8 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): 8606
Objects passed selection criteria: 8585
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: 7512.5
Average stars matched: 7284.75 (96.9684 %)
Memory usage VmPeak: 114044 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 02:38:10 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: 2461032.72253780 23.12.2025 05:20:17.266 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461032.72253780 23.12.2025 05:20:17.266 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461093.64766487 22.02.2026 03:32:28.245 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 753
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.48
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 25 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 46010
Objects passed selection criteria: 45902
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 38250.5
Average stars matched: 36202.5 (94.6458 %)
Memory usage VmPeak: 146388 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 02:41:22 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:
Eri-04-Q2b1x1
#######################################
########### Starting Eri-04-Q2b1x1 ###########
Processing Eri-04-Q2b1x1
server tau has sufficient free disk space available: 1057305 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1057305 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.png' -> 'transient_report/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits_preview.png'
Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
renamed 'Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.png' -> 'transient_report/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits_preview.png'
Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.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= 842.2740
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 596.5114
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1499.6121
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 622.6686
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1499.6898
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 622.5437
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.78043
INFO: SECOND_EPOCH__SD_ratio= 0.000
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
SExtractor catalog cache: saved Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.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: 2461093.64714064
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits exists and is non-empty
Saving wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits to local_wcs_cache/
'wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits' -> 'local_wcs_cache/wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits'
wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits exists and is non-empty
Saving wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits to local_wcs_cache/
'wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits' -> 'local_wcs_cache/wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits'
wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits exists and is non-empty
Saving wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits to local_wcs_cache/
'wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits' -> 'local_wcs_cache/wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:17:07.501 -10:00:16.95
Second-epoch image center 04:17:07.470 -10:00:14.32
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:17:07.501 -10:00:16.95
Second-epoch image center 04:17:05.417 -10:00:17.04
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:17:07.470 -10:00:14.32
Second-epoch second image center 04:17:05.417 -10:00:17.04
Angular distance between the image centers 0.00846 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.DxXH96hGxc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits &> /tmp/tmp.3N49I4H6FL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits &> /tmp/tmp.SFzlP7xa4X
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits &> /tmp/tmp.gfxUymMHNL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
Calibrating the magnitude scale
Found non-empty wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.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 5198 out of 8407 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.911064
a=0.000000 b=1.000000 c=22.911064
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.18
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.18
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 125 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
3.6 pix Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
3.5 pix Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
Limiting magnitude estimates:
15.2 mag. Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
15.2 mag. Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
14.5 mag. Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
14.5 mag. Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.9 (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.DxXH96hGxc (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/util/wcs_image_calibration.sh: line 129: echo: write error: Broken pipe
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=684, passed=8407
Got 8407 stars (including 7713 good ones) from the SExtractor catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 8407 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.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.3N49I4H6FL (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits' -> 'wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
Checking if the catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
WCS catalog name: wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=669, passed=8399
Got 8399 stars (including 7713 good ones) from the SExtractor catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 8399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits -region wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.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.SFzlP7xa4X (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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
WCS-calibrated image found: wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
Checking if the catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
WCS catalog name: wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=703, passed=6738
Got 6738 stars (including 6032 good ones) from the SExtractor catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat
util/solve_plate_with_UCAC5 got 6738 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits -region wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.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.gfxUymMHNL (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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
WCS-calibrated image found: wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
Checking if the catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
WCS catalog name: wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=701, passed=6703
Got 6703 stars (including 6000 good ones) from the SExtractor catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat
util/solve_plate_with_UCAC5 got 6703 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits -region wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.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 Eri-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20519.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 43s
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: 20s
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Considering the candidate 20323_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20323_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:13.40 -11:05:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.989 5114943764752159744 057.80555605211 -11.08425942110 11.1921 10.6975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20325_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20325_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:12.06 -06:05:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.266 3245164455774285824 058.80035185016 -06.08586448011 11.0643 10.6158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20326_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20326_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:01.01 -06:14:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.435 3245140743257978496 058.50436879635 -06.23739307636 11.1457 10.5550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20327_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20327_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:56:58.08 -05:27:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 1.132 3245319418193796608 059.24206310970 -05.45214137185 10.8648 10.3471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20332_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20332_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:00.87 -07:05:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 5.022 3243391424554884736 057.75225396650 -07.09869136389 10.6290 10.2197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20333_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20333_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:17.63 -06:20:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.271 3243692518942374016 057.82284963524 -06.34762684814 10.5971 10.1001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20334_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20334_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 20335_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20335_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:58:08.35 -05:02:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.931 3245711772046131200 059.53467327181 -05.04939681621 10.7549 10.2285 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 20336_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20336_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 20337_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20337_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 20338_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20338_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 20339_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20339_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:43.37 -05:26:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 0.939 3245345875192288256 058.93052682268 -05.44138257675 10.5732 10.1557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20340_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20340_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 20343_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20343_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 20344_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20344_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:54.98 -06:32:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 5.838 3243624692818901632 058.22746694284 -06.54794081182 10.4219 9.8969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20346_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20346_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 20347_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20347_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:12.30 -11:20:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 2.024 5114920571928813568 057.30155379053 -11.33930086873 10.1284 9.4975 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 20350_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20350_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:56:20.31 -06:10:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 3.751 3244977263918998528 059.08371623814 -06.16842522807 10.3669 9.9614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20351_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20351_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 20352_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20352_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20353_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20353_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20354_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20354_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:48.28 -13:45:15.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)
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Considering the candidate 20355_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20355_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20356_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20356_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 20357_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20357_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 20358_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20358_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 20359_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20359_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:57:38.16 -06:01:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 3.969 3245063197624691584 059.40832866349 -06.01740028189 9.8663 9.4082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20360_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20360_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20361_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20361_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:09.44 -08:37:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 4.644 3195050227608805376 058.29062942053 -08.62450974467 9.7561 9.3067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20362_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20362_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 20363_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20363_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 20365_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20365_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 20367_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20367_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 20373_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20373_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:30.48 -05:03:11.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20384_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20384_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:49.16 -07:01:30.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20386_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20386_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:52.63 -08:04:14.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20387_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20387_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:38.65 -06:48:55.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20390_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20390_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:07.30 -11:29:22.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20394_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20394_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:05.30 -08:02:45.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20402_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20402_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:14.36 -06:35:53.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20410_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20410_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:32.66 -06:20:04.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20413_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20413_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:28.93 -08:14:02.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20419_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20419_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:00.15 -08:21:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.04, MAG_FAINT_SEARCH_LIMIT=11.02)GAIADR2_OUTPUT=# 5.101 3242817032807582336 056.75199587655 -08.36421529037 9.1949 9.1647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20425_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20425_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:50.35 -07:31:23.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20427_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20427_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:01.46 -06:03:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.13, MAG_FAINT_SEARCH_LIMIT=11.11)GAIADR2_OUTPUT=# 5.163 3245214341816910848 057.75738653744 -06.06205910360 9.1804 8.8749 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20436_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20436_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 20438_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20438_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:45:38.00 -10:17:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.32, MAG_FAINT_SEARCH_LIMIT=11.30)GAIADR2_OUTPUT=# 3.630 5116002457009356160 056.40934142436 -10.28920701381 9.0642 8.6783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20439_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20439_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:50.52 -09:23:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.39, MAG_FAINT_SEARCH_LIMIT=11.37)GAIADR2_OUTPUT=# 4.078 3194560360817840384 056.71163471101 -09.38804985890 9.1857 8.7803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20441_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20441_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:36.50 -08:46:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.46, MAG_FAINT_SEARCH_LIMIT=11.44)GAIADR2_OUTPUT=# 1.009 3242740238792397952 056.90227796650 -08.78243515021 9.7163 9.5872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20442_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20442_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20444_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20444_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20445_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20445_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20451_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20451_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20461_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20461_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20481_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20481_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20487_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20487_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20489_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20489_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:29.85 -07:10:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.17, MAG_FAINT_SEARCH_LIMIT=12.15)GAIADR2_OUTPUT=# 2.819 3243495534561114880 057.12509846555 -07.17184063429 10.0483 9.6549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20493_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20493_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:40.95 -06:16:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 0.775 3244442110993327488 056.92040881476 -06.26804062873 9.9863 9.5477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20509_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20509_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20510_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20510_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:18.06 -08:57:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 3.141 3242639908355990784 056.82587624950 -08.95535683843 10.0538 9.5727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20519_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 20519_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20531_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20531_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:24.52 -04:53:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 3.956 3246198374661254912 057.85302098471 -04.88947290586 10.3405 9.8910 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 20532_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20532_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:20:19.44 -10:24:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 1.292 3191258767916828416 065.08109272233 -10.40737495456 10.3320 8.8830 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20549_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20549_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:12:38.52 -07:47:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.184 3195949387601330944 063.16003854484 -07.79790694452 10.9580 9.5696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20560_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20560_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:04.56 -07:26:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 1.348 3243460762505919104 056.76866174914 -07.43411156622 10.5697 10.1475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20569_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20569_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:43.74 -05:12:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 2.034 3246069456923323392 057.43275212466 -05.20229103830 10.5861 10.0703 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20578_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20578_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:23:06.98 -08:05:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 0.411 3198704798101299968 065.77899198647 -08.09712487906 12.0169 11.4960 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20586_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20586_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:19:25.93 -09:13:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.326 3192505854622682368 064.85796608258 -09.21711546624 12.0120 11.5152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20588_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20588_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:16:38.63 -10:11:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.229 3191317106457151104 064.16095620051 -10.19692475869 12.0100 11.4462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20594_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20594_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:22:09.54 -08:28:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 0.927 3192683833770560128 065.53949067042 -08.47746679038 11.9248 11.1699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20598_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20598_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:39.66 -04:51:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 4.695 3246108867543204480 057.66622386578 -04.85931572651 10.8611 10.4346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20605_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20605_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:22:21.63 -11:03:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.794 3190957291276886016 065.59028541110 -11.05193235698 12.8233 11.8908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20613_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20613_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:23:24.32 -08:36:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.595 3191916718251509120 065.85132830020 -08.60638754773 12.1184 11.6620 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 20614_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20614_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:27:07.65 -09:51:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.679 3191530725247536000 066.78194961678 -09.85581245503 12.1356 11.6132 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 20615_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20615_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:27:34.71 -07:32:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.112 3198835605625708928 066.89461221502 -07.54527843558 12.0170 11.3332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20616_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20616_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:21:00.34 -09:57:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.368 3191663315181711872 065.25131289239 -09.96541917169 12.1492 11.5409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20619_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20619_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:21:22.67 -10:59:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.631 3190969080963976832 065.34434871774 -10.99938824634 12.3218 11.8289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20625_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20625_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:18:32.39 -10:33:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.103 3191230726074794368 064.63493310033 -10.56329135990 12.2326 11.7129 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#
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Considering the candidate 20626_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20626_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:29:08.74 -10:17:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.831 3179480902439166720 067.28618378159 -10.29166622919 12.1317 11.5874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20627_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20627_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:24:53.84 -10:07:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.288 3191424072619700736 066.22426880299 -10.12488185445 12.1849 11.5720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20629_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20629_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:26:02.66 -08:39:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.125 3197861129085367936 066.51111559965 -08.65709695669 12.0785 11.4059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20630_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20630_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:26:29.26 -10:24:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.395 3179391360962749568 066.62184512159 -10.40194532914 12.1475 11.5739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20631_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20631_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:22:34.36 -08:01:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.513 3192751595471676416 065.64302368096 -08.01701678848 12.2191 11.7050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20632_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20632_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:13:41.91 -11:33:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.415 3189563041813384960 063.42456554581 -11.56026607241 12.2364 11.6527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20635_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20635_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:23:30.32 -10:54:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.238 3190986157753977600 065.87627232321 -10.90544483365 12.2309 11.8241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20638_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20638_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:25:26.81 -09:57:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.678 3191479838475051392 066.36178250102 -09.96042363568 12.2026 11.7162 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20643_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20643_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:24:49.56 -09:05:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.523 3191815975499418496 066.20650557149 -09.08633970171 12.2630 11.7896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20644_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20644_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:14:43.81 -09:16:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.293 3192196067221485696 063.68247232877 -09.26815054738 11.9843 11.1223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20646_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20646_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:23:34.15 -08:30:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.951 3192674182981219456 065.89224203474 -08.50217619482 12.2486 11.7185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20647_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20647_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:27:42.42 -07:09:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.241 3198880616882929408 066.92646583446 -07.15269056217 12.0976 11.4363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20649_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20649_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:13:48.09 -11:27:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.085 3189588437957049856 063.45035419829 -11.45476582623 12.2182 11.8213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20650_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20650_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:30:16.96 -07:51:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.921 3198011620445534976 067.57079955107 -07.86685826978 12.3164 11.8444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20651_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20651_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:23:41.07 -05:59:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.958 3202246153255915776 065.92105757440 -05.99778526182 12.1014 11.5509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20652_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20652_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:27:42.53 -09:05:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.604 3197644800172549248 066.92709376478 -09.08742939094 12.2245 11.5621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20653_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20653_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:38:11.83 -09:07:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.172 3185448948476544640 069.54929224304 -09.12459103362 12.0830 11.5301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20654_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20654_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:25:30.09 -07:45:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.334 3198738397628617728 066.37530314895 -07.75792079828 12.1015 11.4001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20656_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20656_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:22:17.91 -08:57:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.473 3191880090770584448 065.57450086931 -08.96628598631 12.1796 11.4942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20658_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20658_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:34:29.83 -08:18:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.530 3197758840144150016 068.62419391493 -08.30497202629 12.2442 11.7867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20660_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20660_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:09:13.62 -10:12:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.181 3190708496708331904 062.30669908654 -10.21066257716 12.0623 11.3684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20661_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20661_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:20:56.02 -11:03:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.332 3190965503254356224 065.23333503011 -11.06298215273 12.2128 11.6499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20662_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20662_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:23:46.23 -09:08:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.296 3191817697782545408 065.94259683270 -09.13950605352 12.2540 11.7554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20663_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20663_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:26:53.38 -08:39:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.186 3197858685246280192 066.72242325328 -08.66453209985 12.3079 11.8077 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 20664_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20664_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:32:55.52 -10:02:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.379 3185455987927130368 068.23122939375 -10.03683692031 12.2383 11.7409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20666_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20666_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:30:08.63 -10:23:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.365 3179428808781009536 067.53585529977 -10.38524401711 12.3029 11.7716 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20668_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20668_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:31:46.35 -11:51:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.165 3178234606011094016 067.94314271328 -11.85326317942 12.2440 11.7668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20669_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20669_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:35:24.80 -11:38:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.789 3178302500854081920 068.85335418353 -11.64835697600 11.9859 11.0955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20671_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20671_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:17:23.64 -11:31:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.457 3190877507964619648 064.34841726823 -11.53229114289 12.2705 11.8119 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 20678_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20678_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:32:22.26 -09:53:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.145 3185473446972045696 068.09270939852 -09.89071667245 12.3307 11.8825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20679_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20679_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:24:14.90 -06:43:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.645 3199135394342700032 066.06196714966 -06.72347048664 12.1877 11.5162 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#
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Considering the candidate 20681_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20681_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:28:25.64 -08:33:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.284 3197877342584208768 067.10675377226 -08.56282834356 12.3033 11.7814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20682_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20682_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:31:09.18 -08:54:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.120 3197618686771427200 067.78825946983 -08.91605979689 12.2535 11.6717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20683_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20683_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:31:27.81 -08:14:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.119 3197795330186235904 067.86587618231 -08.24900517003 12.2841 11.7308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20684_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20684_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:34:13.33 -11:29:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.662 3178352185035856512 068.55537262972 -11.49641303259 12.2950 11.7151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20686_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20686_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:27:57.86 -10:00:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.311 3191513029982275328 066.99099878756 -10.00738455262 12.1890 11.4624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20687_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20687_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:28:41.39 -09:01:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.880 3197634595330230528 067.17266399703 -09.02311397083 12.1538 11.4458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20690_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20690_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:35:02.04 -09:55:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.343 3185295875843753088 068.75842540736 -09.92428277844 12.4047 12.1832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20692_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20692_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:26:22.93 -11:00:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.360 3179285979645279488 066.59563743582 -11.00427152988 12.2866 11.6588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20693_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20693_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:29:40.10 -08:38:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.264 3197682939482071552 067.41704505724 -08.64731277988 12.2949 11.8222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20695_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20695_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:31:45.01 -10:39:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.544 3179218600198615680 067.93739784560 -10.65852558832 12.3584 11.9151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20696_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20696_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:25:07.84 -08:07:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.886 3198692291156597632 066.28248738677 -08.12480957309 12.3388 11.8507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20697_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20697_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:17:33.57 -12:39:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.331 3177233500673296128 064.38992155885 -12.65078115788 12.2494 11.7553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20701_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20701_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:30:45.47 -09:15:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.570 3197571270332526720 067.68955528297 -09.26495956522 12.4866 11.9913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20703_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20703_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:33:35.29 -10:58:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.286 3179160081266769408 068.39710680753 -10.97401926893 12.2007 11.4185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20704_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 20704_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:34:04.21 -08:39:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.095 3197708537487243520 068.51755553206 -08.65894955649 12.1575 11.4181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 02828_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 02828_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 65s
Prepared the HTML report for the field Eri-04-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 ####
04:41:47.76 -07:57:19.9
03:45:21.20 -12:52:15.0
03:52:56.16 -13:11:42.3
03:48:30.58 -13:35:22.9
03:51:34.57 -13:32:15.7
03:48:00.50 -12:21:47.2
03:53:10.14 -07:27:50.1
03:49:10.33 -12:53:58.7
03:51:25.28 -08:54:10.4
03:52:48.28 -08:47:49.8
03:52:07.70 -06:14:37.1
03:51:31.61 -07:38:15.7
03:52:55.77 -09:10:07.5
03:51:48.95 -06:40:42.4
03:46:35.21 -12:25:42.8
03:53:12.75 -06:57:12.8
03:51:56.87 -05:44:37.7
03:46:46.49 -13:48:31.4
03:51:08.68 -05:53:04.4
03:50:41.76 -07:03:58.4
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/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
SExtractor catalog cache: saved Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
Creating symlink local_wcs_cache/wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
Creating symlink local_wcs_cache/wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.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_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits exists and is non-empty
wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits exists and is non-empty
wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:17:07.501 -10:00:16.95
Second-epoch image center 04:17:07.470 -10:00:14.32
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:17:07.501 -10:00:16.95
Second-epoch image center 04:17:05.417 -10:00:17.04
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:17:07.470 -10:00:14.32
Second-epoch second image center 04:17:05.417 -10:00:17.04
Angular distance between the image centers 0.00846 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.MJxCMynZuM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits &> /tmp/tmp.fC83pHq6do
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits &> /tmp/tmp.lEgr4CeKaT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits &> /tmp/tmp.OMT4u3YgZh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
Calibrating the magnitude scale
Found non-empty wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.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 5347 out of 47663 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.800288
a=0.000000 b=1.000000 c=22.800288
From vast_summary.log: estimated ref. image limiting mag.: -7.48
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 640 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
1.9 pix Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
3.5 pix Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
3.4 pix Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
Limiting magnitude estimates:
15.3 mag. Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
15.3 mag. Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
14.6 mag. Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
14.7 mag. Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 13.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.MJxCMynZuM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2447, passed=47647
Got 47647 stars (including 45108 good ones) from the SExtractor catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 47647 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-20-17_20.00sec_-15.00C_LIGHT_0232.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.fC83pHq6do (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits' -> 'wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
Checking if the catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits
WCS catalog name: wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2386, passed=47753
Got 47753 stars (including 45282 good ones) from the SExtractor catalog wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 47753 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits -region wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-04-Q2b1x1_2025-12-22_23-21-11_20.00sec_-15.00C_LIGHT_0233.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.lEgr4CeKaT (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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
WCS-calibrated image found: wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
Checking if the catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits
WCS catalog name: wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=49, blended=3461, passed=29586
Got 29586 stars (including 26101 good ones) from the SExtractor catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat
util/solve_plate_with_UCAC5 got 29586 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits -region wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-31-42_20.00sec_-14.90C_LIGHT_0076.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.OMT4u3YgZh (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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
WCS-calibrated image found: wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
Checking if the catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat corresponding to the image wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.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_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits
WCS catalog name: wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=50, blended=3609, passed=29676
Got 29676 stars (including 26033 good ones) from the SExtractor catalog wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat
util/solve_plate_with_UCAC5 got 29676 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 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: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
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 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Eri-04-Q2b1x1_213458_TTUQ2b1x1_19317_CO6fqdnq/Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits -region wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077.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 Eri-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out53342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53395.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53432.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out53697.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out53974.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out54173.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out14856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55846.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 330s
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: 124s
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Considering the candidate 53342_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53342_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:07.28 -12:27:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.483 5114509148421372416 057.77991679905 -12.45323188735 13.0806 12.5907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53348_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53348_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53349_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53349_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:21.87 -12:56:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 3.235 5114423833191067264 057.34029978855 -12.93431743036 12.7813 12.0753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53352_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53352_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:57:45.83 -13:09:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.959 5111261053633429248 059.44050327335 -13.16376767058 13.3300 12.8966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53353_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53353_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53354_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53354_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:22.51 -14:11:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 5.303 5110860487804789248 057.09235517593 -14.18799269135 12.5276 11.9112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53355_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53355_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53356_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53356_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:45:38.47 -06:04:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 2.421 3199990711308658560 071.41094569900 -06.06880134088 13.4403 12.7518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53357_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53357_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:38.41 -10:16:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 4.474 5115806705284040704 056.91089403422 -10.28052826030 12.6259 12.1331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53359_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53359_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:14.73 -10:27:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 4.302 3194199785426928512 057.56218889644 -10.46535943986 12.7262 12.1473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53360_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53360_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:06.70 -09:08:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.683 3194632241391487232 057.52814985146 -09.14359317088 12.8284 12.3263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53361_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53361_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:35.16 -10:13:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 2.183 3194227002637461632 058.14671863930 -10.22246071231 12.9527 12.3597 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 53362_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53362_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53366_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53366_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:57:06.37 -05:21:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 3.622 3245322334474910848 059.27721988331 -05.35238473257 12.9384 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53367_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53367_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53370_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53370_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:57:24.80 -14:12:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.653 5111033798324141824 059.35375738398 -14.20518432910 13.0543 12.6092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53371_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53371_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:36.60 -14:08:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.173 5110908385279611008 057.65270367177 -14.14182432408 12.5212 11.9713 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53372_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53372_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:56:15.35 -08:17:33.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)
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Considering the candidate 53373_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53373_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:53.76 -06:40:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.597 3244920948307844224 058.72476776015 -06.67364575670 12.9639 12.4813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53374_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53374_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:35.92 -14:20:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 2.827 5110802419846955136 057.15046649260 -14.34734521031 12.7255 12.2026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53375_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53375_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:56:59.48 -07:24:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.772 3195285042060365696 059.24803812674 -07.41284689311 13.1571 12.6114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53376_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53376_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:19.64 -12:13:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.516 5114712931732328320 056.83112609802 -12.21845278472 12.7246 12.3160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53378_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53378_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:05.62 -14:04:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 3.079 5110736758386161024 058.27343405200 -14.08363295585 12.9890 12.4355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53381_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53381_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53384_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53384_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:17.51 -12:46:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.280 5114474376366197888 057.32346763145 -12.77252373806 12.5749 12.0452 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53385_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53385_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:16.61 -11:39:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.657 5114858312083006336 058.06915397639 -11.66474211582 12.9520 12.4726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53386_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53386_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:30.70 -07:55:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.314 3243242642590405120 057.12756080453 -07.92617838080 12.6348 12.1155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53387_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53387_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:00.44 -10:07:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.889 3194240883971693056 058.00166645564 -10.12819604388 12.9653 12.4636 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 53388_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53388_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:46.32 -10:58:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.476 5115705000458356096 057.44303126067 -10.97111896410 12.8657 12.3981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53389_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53389_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:36.78 -14:16:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.330 5110703704317823872 057.90472228073 -14.27043773158 12.8541 12.3733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53392_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53392_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:42.54 -12:54:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.398 5114107620519180288 056.67764631932 -12.90687768560 12.5740 12.0926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53393_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53393_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:42.33 -10:33:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 3.523 3194186423786428544 057.67540988263 -10.55599019330 13.0976 12.5590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53395_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53395_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:31.68 -12:02:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 3.731 5114766532925112064 056.63101605571 -12.03997609174 12.4777 11.9410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53399_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53399_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:59.52 -12:41:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.674 5114446785496308224 058.24858865612 -12.68761007004 12.8802 12.4136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53400_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53400_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:36.35 -10:51:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.760 5114962800047207040 057.65072042892 -10.86405570101 12.7563 12.2715 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53401_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53401_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:47.86 -14:04:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.169 5110918658841370368 057.94911455759 -14.06969588662 12.5961 12.1106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53402_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53402_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:57.47 -09:52:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.482 3194472296808457472 057.23917316999 -09.87341186840 12.7427 12.1969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53403_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53403_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:41.71 -06:43:59.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)
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Considering the candidate 53404_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53404_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:46.49 -08:24:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.085 3195113449527344128 057.94425087150 -08.40168992963 12.7923 12.2281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53405_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53405_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:02.60 -14:13:22.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 53406_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53406_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:28.90 -05:05:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.806 3246121649365610240 058.62066828128 -05.09782344206 12.7444 12.2886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53407_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53407_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:28.80 -06:50:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.423 3244867999951093504 058.86948139220 -06.85032218733 12.9313 12.3906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53408_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53408_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:29.64 -11:28:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.366 5115568935894535936 056.62373348986 -11.47636386146 12.5584 11.9221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53410_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53410_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:19.95 -13:49:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.900 5111117734868253696 058.58179698516 -13.82093567237 12.9609 12.4289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53412_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53412_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:25.52 -12:30:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.284 5114543198922164096 058.35602955539 -12.50089273601 12.8929 12.4054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53413_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53413_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:01.95 -13:54:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.511 5110880691330892928 057.00826964167 -13.91174290288 12.4811 11.8567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53414_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53414_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:18.00 -13:04:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.283 5114043367808464512 057.32435874156 -13.08291818703 12.5695 12.0797 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 53416_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53416_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:26.89 -07:26:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.562 3243275804035448960 057.86272770240 -07.44954042778 12.4219 11.9357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53417_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53417_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:57.65 -09:54:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.165 3194295275437516160 057.98959927859 -09.90790172335 12.6317 12.2023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53418_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53418_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:21.40 -12:41:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.464 5114489803888640000 057.08955166049 -12.69926703998 12.4966 11.8829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53419_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53419_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:56:24.49 -05:00:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.908 3245398651750387456 059.10257350160 -05.00031835144 12.5814 12.0569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53420_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53420_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:00:37.68 -04:53:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.879 3245730291945050368 060.15626179180 -04.88518591145 12.6675 12.1655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53422_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53422_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:26.58 -05:44:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.388 3245284676201397248 058.86087163357 -05.74806065358 12.5825 12.1224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53424_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53424_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:31.95 -06:02:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.269 3245180020735705088 058.63343759401 -06.03835395495 12.6886 12.1764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53426_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53426_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:58:49.40 -05:36:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.176 3245117589090486784 059.70668396165 -05.61516468464 12.8890 12.3365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53427_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53427_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:13.57 -07:56:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 5.235 3243227219365453952 057.30674026050 -07.94058684328 12.4676 11.8719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53428_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53428_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:03.64 -11:38:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.271 5114894114930294144 057.26487552828 -11.64973595084 12.6383 12.0904 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 53431_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53431_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:04.21 -13:13:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.473 5111400897769217280 058.01909105076 -13.22233021304 12.4947 11.8265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53432_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53432_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:59.37 -07:48:49.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 53433_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53433_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:10.04 -08:05:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.712 3195151412741158272 058.04240404081 -08.08489047918 12.4395 11.9184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53434_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53434_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:32.93 -07:45:49.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)
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Considering the candidate 53435_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53435_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53436_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53436_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:40.63 -09:23:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.260 3194574478373962624 057.16974922866 -09.38576940916 12.5499 12.1133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53437_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53437_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:17.79 -09:02:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.353 3194654747020096768 057.82506872974 -09.04988144156 12.6947 12.2124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53438_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53438_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:11.62 -06:29:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.990 3243637818238902400 057.79762104161 -06.48785625904 12.2220 11.5440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53439_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53439_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:42.37 -06:05:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.896 3245167135833818880 058.67706694998 -06.09057094375 12.6528 12.0297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53440_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53440_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53442_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53442_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:40.76 -10:26:10.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 53443_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53443_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:25.97 -10:51:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 2.168 5115745613669285120 056.60839408818 -10.86067597861 12.4477 11.9298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53444_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53444_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:16.82 -09:51:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.381 3194480916806397440 056.82011230281 -09.86063301380 12.1996 11.6814 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 53445_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53445_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:08.16 -05:13:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.837 3246078046857969664 057.78378529632 -05.22996338516 12.3690 11.6922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53446_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53446_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:32.27 -07:32:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.387 3243302948228734848 058.38410401155 -07.54804749381 12.7069 12.2487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53447_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53447_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53448_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53448_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:26.59 -12:13:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.442 5114712656854421760 056.86135471294 -12.23309089372 12.2845 11.8099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53450_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53450_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:28.27 -05:21:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 4.636 3245350101440105088 058.86802471780 -05.36726664787 12.1115 11.4251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53451_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53451_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53452_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53452_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53453_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53453_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:11.85 -14:22:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 2.023 5110661476199400192 058.54928519516 -14.37547185537 12.6536 12.1783 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#
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Considering the candidate 53454_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53454_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:10.23 -06:58:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.929 3243407260097052544 058.29223495900 -06.98271546327 12.5929 12.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53456_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53456_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:56.12 -05:59:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 1.797 3245174759398359680 058.73384676048 -05.98791561979 12.5403 12.0238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53458_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53458_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53459_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53459_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:57:15.87 -05:20:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.963 3245322678072293888 059.31563202984 -05.33956812533 12.7463 12.2577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53460_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53460_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53461_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53461_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:12.60 -09:20:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.727 3194529437053337216 057.30293294048 -09.34427375654 12.4446 11.7984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53462_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53462_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:05.48 -11:34:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.134 5114854528214112000 057.52177664430 -11.57680271077 12.6974 12.2355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53463_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53463_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:22.91 -08:45:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.055 3242750851655145216 056.84485445448 -08.75779475176 12.2476 11.7622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53464_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53464_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53465_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53465_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:02.35 -11:00:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.728 5115703767804186880 057.25887290223 -11.00820351800 12.6229 12.1529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53466_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53466_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:03.73 -11:51:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 5.348 5114781552426843264 056.76443138370 -11.86287413045 12.2248 11.6002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53468_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53468_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:39.02 -10:49:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 0.794 5114963178004324352 057.66246429183 -10.83122964056 12.4981 11.8366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53470_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53470_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:29.27 -13:07:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.224 5111403234231412608 058.12230420540 -13.13259166705 12.4995 11.9969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53471_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53471_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:37.25 -08:56:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.791 3194657186561510272 057.90568934732 -08.94685955616 12.7516 12.2324 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 53472_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53472_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53473_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53473_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:02.60 -08:54:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.854 3194651551564470400 058.26083456705 -08.90840395054 12.6025 12.0827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53474_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53474_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:45.67 -10:55:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.852 5114958298921483520 057.69023461056 -10.93096462144 12.7744 12.2564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53475_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53475_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53476_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53476_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:08.03 -10:16:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.733 3194232328396862592 057.78268701119 -10.26823913223 12.5142 11.9285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53478_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53478_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:00.71 -14:23:14.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 53479_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53479_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:52.42 -06:58:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.101 3243584182687433856 057.71754980408 -06.96896080186 12.2293 11.7364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53480_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53480_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:45.67 -06:09:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.454 3245162222391295488 058.69023010643 -06.16452859857 12.4259 11.7564 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 53481_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53481_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:25.03 -14:04:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.464 5110734005310068864 058.35419982555 -14.07824007853 12.5904 12.0949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53483_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53483_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:17.15 -11:22:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 4.990 3193146869901789568 058.57243066654 -11.37697850781 12.5764 11.9459 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 53484_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53484_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:57.51 -06:01:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.418 3245203900753825792 057.98951696032 -06.02043283221 12.4706 11.7983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53485_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53485_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:09.54 -13:30:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.751 5114013784073810304 057.29078621772 -13.50276269749 12.2611 11.6325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53487_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53487_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:50.21 -11:22:19.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 53488_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53488_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:08.71 -10:41:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.202 5115768256736866304 056.53568667242 -10.69772682220 12.1184 11.3334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53492_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53492_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:08.10 -09:06:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.153 3194629904929262464 057.78393149895 -09.11323780189 12.6558 12.2237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53494_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53494_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:47.79 -11:57:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 4.023 5114787874618748928 056.94807714998 -11.95533399767 12.1217 11.6386 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 53496_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53496_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:44.59 -09:40:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.372 3194504899903621504 057.43557868937 -09.66912465215 12.5735 12.0762 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 53497_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53497_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:31.96 -09:41:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.346 3194512733924122368 057.13250572033 -09.68995207235 12.2542 11.6945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53498_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53498_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:57.39 -11:52:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.837 5114649473592897792 058.48989474209 -11.88081538935 12.7307 12.2659 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 53501_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53501_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:39.14 -10:48:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.058 3193417865158130816 058.16309991914 -10.80826575663 12.3727 11.6677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53502_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53502_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53503_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53503_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53504_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53504_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53505_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53505_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:57:51.03 -06:05:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.718 3245058833937920128 059.46300716014 -06.08904458492 12.6476 12.1851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53508_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53508_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:00:00.53 -05:02:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.378 3245700948728497152 060.00123829797 -05.04423395647 12.7516 12.2761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53510_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53510_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:14.59 -09:47:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.613 3194300910434529152 057.81096167868 -09.79791477141 12.4494 11.9314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53511_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53511_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53512_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53512_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53514_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53514_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:37.70 -10:37:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.578 5115781489532298880 057.15768309548 -10.61793441062 12.1525 11.4902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53515_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53515_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:30.54 -10:26:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.858 3194194086008065792 057.87650408217 -10.43447046635 12.4640 12.0993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53516_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53516_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:50.94 -06:26:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.941 3243643521955536768 057.96360099745 -06.43998006133 12.4181 11.9456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53517_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53517_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:28.79 -06:50:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.391 3243427570999670272 058.36957780690 -06.84349764739 12.6433 12.2125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53518_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53518_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53519_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53519_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53520_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53520_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:25.39 -13:42:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.591 5113981073602896512 057.10554430128 -13.70824037326 12.2610 11.7038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53522_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53522_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53524_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53524_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:40.36 -13:01:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.316 5111407426119446016 057.91848878053 -13.02506262772 12.3211 11.6855 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#
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Considering the candidate 53525_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53525_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:39.31 -07:16:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.068 3243372320540421120 057.91358037547 -07.28001542589 12.0721 11.5372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53528_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53528_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:30.94 -10:52:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.936 5115715411459080960 057.37808465675 -10.86742091529 12.3423 11.9055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53530_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53530_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:12.61 -10:53:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.774 5115709265362318848 057.30154037181 -10.89783607302 12.2544 11.6337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53531_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53531_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:33.57 -13:14:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.399 5111388627045336960 058.14054323506 -13.24633911038 12.3507 11.8673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53532_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53532_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:56:40.60 -05:55:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.302 3245078723929921024 059.16961446058 -05.92426430754 12.6300 12.1592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53533_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53533_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:17.47 -08:14:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.909 3195122653639748864 058.07144016258 -08.24904308161 12.2421 11.7450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.909#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53535_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53535_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:01.47 -09:53:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.138 3194339840017983232 058.25632548099 -09.89402459315 12.6911 12.1479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53537_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53537_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:35.23 -10:50:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.079 5115748504183492992 056.89601770569 -10.83835777185 12.1839 11.7074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53539_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53539_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53540_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53540_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53541_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53541_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:20.08 -10:48:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 3.136 5115757845736142976 056.58278614944 -10.80631261767 12.1574 11.4978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53542_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53542_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53543_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53543_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:54.61 -11:15:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.748 5114924592018130944 057.22600295047 -11.26446614382 12.2656 11.6692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53548_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53548_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:22.64 -06:24:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.216 3244946237075413376 058.59436120315 -06.40771846616 12.4609 11.8277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53549_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53549_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53550_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53550_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:29.66 -06:45:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.850 3244918714924857984 058.62409818645 -06.75996733953 12.4811 12.0428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53553_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53553_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53554_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53554_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53555_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53555_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:58:22.84 -05:56:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.385 3245070138291828224 059.59565479664 -05.94705528128 12.5923 12.0724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53556_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53556_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:57:14.15 -05:31:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 1.508 3245306602011386880 059.30910212143 -05.52658817549 12.4928 11.9411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53557_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53557_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53558_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53558_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:09.00 -09:02:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.595 3194646466323195648 058.28722699436 -09.04468495882 12.4286 11.9458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53559_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53559_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53560_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53560_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53561_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53561_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:36.33 -05:51:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.826 3245177473817685888 058.90171908180 -05.85834670854 12.4597 11.9956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53563_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53563_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:43.23 -06:35:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.142 3243623039254604160 058.18037980990 -06.58785776781 12.2441 11.6698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53564_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53564_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:32.66 -08:51:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.271 3194696902121702144 057.13616718988 -08.85939869584 12.2586 11.7843 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 53565_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53565_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53566_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53566_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:05.81 -12:25:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.624 5114515848570353024 057.77425049377 -12.42546754714 12.2209 11.6437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53567_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53567_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:40.78 -07:09:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.763 3243485565940703488 057.42054098519 -07.16653652304 12.1666 11.7232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53568_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53568_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53570_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53570_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:11.58 -06:27:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 4.212 3243675717030285952 057.29707276966 -06.45642686860 12.1770 11.6998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53571_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53571_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:34.63 -12:00:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 5.289 5114632568601583104 057.89569906177 -12.00845785602 12.4065 11.9847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53573_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53573_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53575_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53575_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:41.10 -07:15:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.080 3243481550147656448 057.42071866071 -07.25979214207 12.1567 11.6463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53576_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53576_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53577_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53577_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:49.13 -07:21:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.195 3243370357738057344 057.95357302057 -07.36475565854 12.1531 11.6615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53578_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53578_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:59.11 -14:16:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 0.801 5110704082274944640 057.99609384907 -14.27874830599 12.2822 11.7999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53579_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53579_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:01:41.29 -04:59:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.571 3245539938994239744 060.42115076122 -04.99116786427 12.4239 11.9802 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 53581_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53581_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:59:03.51 -06:13:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.087 3245011142621110272 059.76491970955 -06.22244457126 12.5549 12.0375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53583_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53583_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:04:18.25 -06:10:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.448 3197305154158095104 061.07597442349 -06.17632719104 12.7986 12.3955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53584_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53584_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53585_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53585_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53586_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53586_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53587_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53587_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:31.66 -07:32:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.988 3243270031599408000 057.88112181953 -07.53785014359 12.1848 11.6515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53588_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53588_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53590_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53590_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 53591_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53591_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:54.88 -09:30:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.638 3194511737491555328 057.47799579607 -09.51203713251 12.2129 11.7064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53592_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53592_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:29.32 -12:56:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.111 5114423661392373632 057.37305288445 -12.93469493136 12.1153 11.5219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53593_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53593_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53594_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53594_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53595_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53595_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:22:37.26 -10:48:38.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 53596_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53596_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:16.76 -09:44:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.268 3194498375849868800 057.31990741843 -09.73676268471 12.2182 11.7051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53597_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53597_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:49.31 -09:30:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.095 3194601214545908992 057.70650867020 -09.51055318781 12.2259 11.5743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53598_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53598_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 53599_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53599_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:19.92 -07:04:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.977 3243391729495313536 057.83202741475 -07.07876837072 12.0824 11.6637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53600_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53600_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:30.86 -11:35:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.889 5114860545465999488 058.12791866651 -11.58727450280 12.4150 11.9388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53601_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53601_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:14.20 -10:48:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.054 3193426656954270080 057.80814350102 -10.81520274837 12.2925 11.8034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53602_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53602_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53603_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53603_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:07.70 -13:03:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.803 5114406722041422080 057.53228764063 -13.05753846107 12.1214 11.6327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53604_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53604_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:11.49 -09:38:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.161 3194408284616755328 057.79771048511 -09.64342224810 12.3907 11.9056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53606_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53606_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:54.79 -13:09:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.406 5111402409597701632 057.97868120239 -13.15082402041 12.1693 11.6052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53608_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53608_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:40.03 -11:02:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.197 5115694559394265216 056.91652570035 -11.04209879088 12.2298 11.8482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53609_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53609_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:53.98 -11:20:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.806 5114920743727509504 057.22335230437 -11.33591463113 12.0917 11.6495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53610_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53610_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:11.19 -08:51:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.079 3242644409481714432 056.79585647440 -08.85974511212 11.9900 11.3643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53611_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53611_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:31.95 -09:34:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.568 3194600523055498624 057.63306190681 -09.56957730771 12.2959 11.7744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53612_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53612_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:11.05 -08:30:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.702 3194738516062215296 057.54571720106 -08.50056938825 12.2121 11.7169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53613_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53613_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:05.86 -11:46:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.989 5115537260511511296 056.52463806152 -11.77670257433 11.9475 11.4409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53614_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53614_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:43.14 -06:45:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.411 3244918882426703104 058.68069637028 -06.75247847856 12.1097 11.4937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53616_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53616_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53617_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53617_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 53618_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53618_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53620_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53620_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:08.39 -06:44:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.169 3243418534388463232 058.53379230162 -06.73339539327 12.1600 11.6438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53621_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53621_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53622_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53622_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:48.38 -06:06:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 4.089 3244981799404464512 058.95190166646 -06.10797964075 12.2576 11.6635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53623_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53623_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53624_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53624_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:05.66 -09:59:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.779 3194246656407729152 058.02234376783 -09.99320056949 12.3456 11.8784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53625_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53625_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53626_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53626_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:38.97 -06:47:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.730 3244915485109451264 058.66190939298 -06.78672973423 12.1199 11.6812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53627_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53627_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53628_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53628_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:36.69 -05:47:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.363 3245283546626911232 058.90302518862 -05.79092208600 12.1689 11.6875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53629_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53629_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53630_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53630_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53631_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53631_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:25.65 -05:17:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.290 3245361027836856192 058.60750086870 -05.30014061529 12.1422 11.5775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53632_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53632_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:40.19 -07:27:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.197 3195290127301664896 058.91656343185 -07.46143364076 12.2780 11.8086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53633_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53633_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:07.81 -10:13:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.693 3194221706940000768 058.03211991425 -10.22402905653 12.2721 11.7963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53634_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53634_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53637_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53637_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:04.16 -08:41:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.851 3195043527459829120 058.26615489891 -08.68740607546 13.2542 12.4846 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53639_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53639_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:02.38 -10:04:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.576 3194279744835746432 057.25955664747 -10.07118405484 11.8725 11.4594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53640_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53640_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53641_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53641_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53642_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53642_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:57:32.10 -05:49:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.833 3245086420511343744 059.38268855022 -05.81722579096 12.1253 11.6051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53643_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53643_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:56.82 -11:56:49.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 53644_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53644_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:23.22 -13:03:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.487 5114043505247415808 057.34653512613 -13.06321719456 11.7692 11.2603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53647_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53647_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:33.49 -06:17:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.671 3244968772766802176 058.88844705592 -06.29857091578 12.0711 11.6230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53650_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53650_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53652_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53652_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53653_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53653_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:48.53 -10:46:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.992 3193392542031010944 058.45276358748 -10.77956461493 12.2589 11.7575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53657_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53657_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:00.88 -14:00:56.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)
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Considering the candidate 53659_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53659_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53661_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53661_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:46:49.70 -13:01:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.156 3180675109507907584 071.70685790820 -13.02634530223 12.9735 12.3051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53662_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53662_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53663_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53663_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:13.07 -07:19:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.468 3243327171844273536 058.30541915068 -07.32252569841 12.0601 11.5871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53664_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53664_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 53667_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53667_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53668_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53668_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53670_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53670_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:19.93 -13:32:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 2.014 5111008921873975680 057.58249043183 -13.54020094167 11.6866 11.0945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53671_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53671_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53673_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53673_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53674_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53674_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 53675_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53675_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:58.60 -09:38:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 5.026 3194397667457590400 057.99275544181 -09.63892256450 11.7991 11.4025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53676_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53676_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53677_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53677_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53679_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53679_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:58.05 -07:39:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.035 3243298172225103104 058.49256642520 -07.65401884189 11.9880 11.5516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53681_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53681_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53682_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53682_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:56:41.31 -06:28:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.530 3244951425395809536 059.17148636759 -06.47683007493 12.0349 11.5145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53683_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53683_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:31.43 -11:35:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.156 5114863225525546624 057.88007365066 -11.59896538942 12.0225 11.5462 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 53684_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53684_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53685_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53685_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53688_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53688_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 53689_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53689_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53690_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53690_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53691_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53691_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53692_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53692_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53693_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53693_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53694_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53694_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:04.81 -09:16:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.670 3194445874170492672 058.26946366391 -09.26991478302 11.9486 11.5042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53696_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53696_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53697_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53697_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:56:27.77 -06:23:44.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
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Considering the candidate 53698_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53698_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53699_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53699_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:05.56 -10:58:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.378 3193406079767888128 058.02360041178 -10.97764390032 11.8810 11.4074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53700_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53700_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:00.80 -13:50:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.438 5110964735250461824 057.50212456046 -13.84898809289 11.4568 10.8114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53701_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53701_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53702_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53702_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53703_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53703_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:16.00 -12:02:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.681 5114631159852317696 057.81653368418 -12.04658195905 11.7571 11.2778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53704_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53704_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53705_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53705_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53706_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53706_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53707_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53707_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:28.27 -14:13:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 3.393 5110810322586761088 057.36682879003 -14.22640837089 11.3030 10.6664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53708_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53708_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53709_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53709_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53710_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53710_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53711_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53711_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53712_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53712_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53713_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53713_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:56:48.29 -06:30:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.876 3244904215115292800 059.20052264578 -06.50663834883 11.7560 11.3454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53715_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53715_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:19.48 -07:23:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.381 3243311774384141056 058.58205646843 -07.39278253466 11.7600 11.3227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53717_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53717_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53719_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53719_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53721_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53721_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53723_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53723_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:38.95 -08:11:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.452 3195132209944523264 058.41218541395 -08.18981852173 11.8859 11.3421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53724_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53724_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53725_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53725_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53727_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53727_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:57.37 -07:46:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 4.369 3243202411634364672 058.23782679356 -07.76726297991 11.6214 11.1938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53731_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53731_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53733_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53733_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53734_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53734_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53736_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53736_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53737_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53737_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53738_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53738_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53739_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53739_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53740_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53740_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53741_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53741_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 53742_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53742_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53743_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53743_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53744_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53744_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:50.58 -08:51:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 4.792 3194652719795574784 058.20940360005 -08.86301222878 11.4328 10.9337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53745_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53745_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53746_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53746_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:07.77 -13:24:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.555 5114053710089702656 056.53258118530 -13.40775621518 10.8916 10.2043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53747_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53747_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53749_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53749_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53750_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53750_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53751_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53751_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53752_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53752_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53754_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53754_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53756_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53756_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53757_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53757_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:36.28 -07:01:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 2.826 3243395135406669952 058.15195270511 -07.02258036585 11.2101 10.6476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53758_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53758_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53760_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53760_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53761_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53761_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 53762_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53762_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 53763_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53763_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 53764_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53764_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53765_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53765_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53766_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53766_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53767_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53767_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53768_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53768_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:59:20.97 -06:22:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 2.564 3244988602632744320 059.83683848569 -06.37172232024 11.4265 10.9557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53769_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53769_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:54.10 -13:24:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.314 5111017271290380288 057.72558179136 -13.41453325822 11.0302 10.5634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53770_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53770_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:59:55.80 -05:49:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.174 3245051446594128512 059.98228703968 -05.83275212629 11.3600 10.9050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53771_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53771_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53772_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53772_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:43.13 -08:03:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.302 3195184608545236224 058.92907530280 -08.05959602397 11.3721 10.9032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53773_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53773_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53774_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53774_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53775_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53775_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53776_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53776_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:27.31 -11:03:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 4.065 5114955687581382656 057.61494131898 -11.05045714712 10.9787 10.4423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53777_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53777_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 53778_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53778_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53779_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53779_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 53783_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53783_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53784_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53784_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53785_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53785_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53786_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53786_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53787_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53787_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53788_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53788_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 53789_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53789_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53790_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53790_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:56:07.32 -07:02:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 3.453 3244848685481222400 059.02956616851 -07.03797502413 11.0576 10.6011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53791_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53791_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53792_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53792_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53793_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53793_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 53794_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53794_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53795_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53795_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 53797_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53797_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 53798_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53798_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53799_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53799_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:32.50 -10:16:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 4.389 3194231572482613376 057.88665383991 -10.27670576546 10.7703 10.2959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53800_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53800_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53801_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53801_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:50.18 -09:07:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 5.462 3194630351605867392 057.70773958207 -09.13256929957 10.6838 10.2342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53802_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53802_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53803_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53803_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53805_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53805_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 53806_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53806_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53807_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53807_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53808_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53808_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53809_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53809_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:57:03.77 -06:28:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 2.967 3244904696151624320 059.26491326710 -06.47115379279 10.5075 10.0019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53811_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53811_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 53812_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53812_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53813_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53813_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53814_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53814_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53815_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53815_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53816_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53816_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 53817_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53817_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53819_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53819_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 53820_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53820_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:26.35 -08:54:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 5.422 3194660553815869696 057.85871581312 -08.90337756842 9.9334 9.4534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53821_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53821_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53822_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53822_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53823_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53823_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53824_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53824_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 53826_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53826_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53827_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53827_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53828_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53828_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 53829_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53829_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:53.66 -06:10:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.45, MAG_FAINT_SEARCH_LIMIT=11.43)GAIADR2_OUTPUT=# 5.362 3244979978338332928 058.97484465196 -06.18102580747 9.4195 8.9487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53830_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53830_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:18.90 -07:46:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.26, MAG_FAINT_SEARCH_LIMIT=11.24)GAIADR2_OUTPUT=# 5.420 3195254874210130176 058.58024180443 -07.77806428588 9.4299 8.9564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53831_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53831_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:44.31 -13:53:06.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53833_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53833_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53835_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53835_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 53836_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53836_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 53837_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53837_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:41.39 -05:21:36.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53841_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53841_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:30.29 -05:03:09.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53848_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53848_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:55:08.77 -04:58:22.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53854_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53854_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:49.18 -07:01:30.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53859_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53859_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:38.66 -06:48:54.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53863_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53863_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:05.60 -08:02:46.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53865_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53865_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:07.18 -11:29:23.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53875_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53875_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:14.50 -06:35:53.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53879_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53879_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:32.84 -06:20:05.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53886_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53886_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:28.96 -08:14:01.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53892_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53892_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:00.28 -08:21:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.06, MAG_FAINT_SEARCH_LIMIT=11.04)GAIADR2_OUTPUT=# 2.977 3242817032807582336 056.75199587655 -08.36421529037 9.1949 9.1647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53893_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53893_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53896_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53896_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:50.46 -07:31:25.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53901_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53901_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:42.59 -05:17:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.21, MAG_FAINT_SEARCH_LIMIT=11.19)GAIADR2_OUTPUT=# 3.905 3246056778179870720 057.42649228022 -05.28736006458 8.9353 8.2611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53904_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53904_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:31.56 -07:38:17.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53905_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53905_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:07.66 -06:14:36.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53908_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53908_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:45:37.99 -10:17:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.27, MAG_FAINT_SEARCH_LIMIT=11.25)GAIADR2_OUTPUT=# 3.794 5116002457009356160 056.40934142436 -10.28920701381 9.0642 8.6783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53910_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53910_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53917_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53917_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:48.97 -06:40:42.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53918_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53918_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:36.40 -08:46:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.49, MAG_FAINT_SEARCH_LIMIT=11.47)GAIADR2_OUTPUT=# 2.265 3242740238792397952 056.90227796650 -08.78243515021 9.7163 9.5872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53936_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53936_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:12.80 -06:57:13.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53955_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53955_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:56.67 -05:44:35.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53963_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 53963_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 53973_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53973_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:46.41 -13:48:32.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53974_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53974_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:29.63 -07:10:17.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)
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Considering the candidate 53982_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53982_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:20.57 -11:08:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 5.112 5115596526764439680 056.58701366829 -11.13469249942 9.9514 9.4701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53995_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53995_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 53998_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 53998_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:40.83 -06:16:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 1.075 3244442110993327488 056.92040881476 -06.26804062873 9.9863 9.5477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54004_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54004_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:08.44 -05:53:03.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54010_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54010_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54015_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54015_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:34.39 -05:15:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.847 3246068804088298496 057.39196764018 -05.25275469589 10.1363 9.4590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54028_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54028_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:41.84 -07:03:58.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54031_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54031_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54037_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54037_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:10.91 -06:45:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 4.162 3243594284448341120 057.79655959362 -06.76170852218 10.5455 10.1723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54038_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54038_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54040_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54040_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54044_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54044_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:24.44 -04:53:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 5.155 3246198374661254912 057.85302098471 -04.88947290586 10.3405 9.8910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54045_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54045_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54054_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54054_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54056_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54056_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:45:14.23 -12:31:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 2.728 5114367689377291648 056.30887764728 -12.51824783313 10.3525 9.9482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54058_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54058_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:45:15.72 -13:39:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 3.776 5113947160539780736 056.31630808913 -13.65991591470 10.3523 9.9252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54065_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54065_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54066_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54066_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54071_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54071_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:04.23 -07:26:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 3.767 3243460762505919104 056.76866174914 -07.43411156622 10.5697 10.1475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54076_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54076_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:00.17 -07:05:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 5.535 3243391424554884736 057.75225396650 -07.09869136389 10.6290 10.2197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54083_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54083_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:02.16 -07:33:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 4.010 3243259551879179264 057.26003162091 -07.55447548118 10.5615 10.0762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54088_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54088_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54110_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54110_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:10.34 -09:41:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 4.153 3194539126499539712 056.79424764565 -09.68972872898 10.8162 10.4655 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54112_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54112_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54114_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54114_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54116_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54116_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:54:52.65 -05:22:58.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)
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Considering the candidate 54118_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54118_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:56.14 -12:16:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 5.084 5114708812860779776 056.98520280089 -12.26896724002 10.6471 10.1267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54124_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54124_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:43.50 -05:12:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 5.551 3246069456923323392 057.43275212466 -05.20229103830 10.5861 10.0703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54127_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54127_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54132_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54132_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54145_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54145_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54146_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54146_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54148_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54148_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54157_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54157_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54162_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54162_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54163_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54163_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:53.43 -10:23:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 5.319 5115985998694719872 056.72412286880 -10.39675108289 10.8813 10.3680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54166_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54166_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:08.38 -07:04:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 1.704 3243523773970016384 056.78449297148 -07.06786599936 10.8934 10.2033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54173_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54173_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:15.58 -11:15:08.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)
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Considering the candidate 54174_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54174_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54178_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54178_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:13.62 -12:28:30.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)
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Considering the candidate 54185_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54185_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54191_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54191_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54201_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54201_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:45:15.52 -13:50:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 2.339 5113895895810195584 056.31521453114 -13.84437677793 10.7651 10.2924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54207_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54207_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54211_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54211_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:45:19.02 -12:10:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 4.408 5114395383326348800 056.33050259239 -12.16776068969 10.9277 10.5170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54214_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54214_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54217_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54217_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:14.22 -06:36:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 4.015 3243631702205562496 057.81032072028 -06.60836356930 10.8836 10.3643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54226_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54226_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:59.09 -06:12:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 3.359 3244448364465706752 056.99707087935 -06.21411753515 11.0410 10.6567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54228_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54228_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54230_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54230_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54236_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54236_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54238_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54238_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54249_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54249_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54253_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54253_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:42.29 -05:52:02.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)
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Considering the candidate 54255_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54255_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54267_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54267_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54268_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54268_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:38.33 -06:00:55.2 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 54273_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54273_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:30.91 -13:51:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 5.269 5113887168436637568 056.62989423275 -13.86183510176 11.0465 10.6033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54274_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54274_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54279_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54279_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54295_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54295_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54298_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54298_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54302_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54302_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:28.87 -05:31:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 4.741 3244556185323514496 057.12108344965 -05.52980599686 11.1903 10.4676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54305_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54305_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54314_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54314_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54316_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54316_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:45:17.68 -11:17:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 3.483 5115634464211304832 056.32457233336 -11.28339435775 11.0823 10.6296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54327_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54327_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54329_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54329_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:53.95 -05:24:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.394 3246060042355026560 057.22531549805 -05.40510713645 11.3870 10.8415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54330_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54330_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54344_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54344_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54367_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54367_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54373_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54373_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54374_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54374_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:57:28.16 -04:50:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 5.501 3245766438389782016 059.36878680280 -04.84557059901 11.4420 10.9382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54383_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54383_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:39.35 -04:52:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 5.815 3246296265555006976 057.41548852703 -04.86850556844 11.2557 10.8215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54385_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54385_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:21.44 -06:06:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 5.185 3244460321654642176 057.34076998743 -06.10046224738 11.2782 10.8268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54388_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54388_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54393_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54393_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54400_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54400_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:20.21 -06:38:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 4.022 3244325562760530816 056.83320334915 -06.64302626245 11.4052 10.7954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54405_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54405_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54409_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54409_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54419_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54419_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54421_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54421_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:32.32 -06:22:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.965 3244429294810920064 056.88512566822 -06.36921360995 11.4330 10.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.965#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54425_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54425_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:36.27 -13:35:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 5.515 5114000452495303296 056.65228159387 -13.58782053929 11.4680 11.0296 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54429_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54429_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54432_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54432_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:55.42 -05:50:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 4.548 3244474065549969152 057.48214779969 -05.84583750861 11.5890 11.1084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54451_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54451_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54453_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54453_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54455_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54455_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54461_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54461_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54469_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54469_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54478_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54478_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54488_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54488_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54493_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54493_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54494_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54494_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54497_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54497_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54500_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54500_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54502_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54502_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:46.67 -06:09:05.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 54506_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54506_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54509_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54509_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54514_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54514_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54523_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54523_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54525_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54525_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54527_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54527_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54533_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54533_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54563_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54563_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54567_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54567_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54571_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54571_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54572_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54572_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:35.69 -06:32:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.028 3243671593861686144 057.14966997782 -06.54763785287 11.3520 10.7728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54575_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54575_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54578_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54578_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54581_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54581_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:09.78 -05:01:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 5.088 3246286576108802304 057.29184273425 -05.02387376080 11.5164 10.9986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54604_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54604_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54608_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54608_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54612_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54612_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54613_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54613_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54632_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54632_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54641_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54641_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54644_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54644_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54645_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54645_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54649_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54649_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:34.74 -06:11:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.177 3244437609867591808 057.14483457984 -06.19953829982 11.7229 11.1588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54657_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54657_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54660_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54660_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:48.03 -05:41:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.933 3244539104238526592 057.20094250580 -05.68948765595 12.0546 11.4880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54673_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54673_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54675_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54675_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:23.27 -05:25:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 3.586 3246059320800526208 057.09786261938 -05.42737104463 11.7354 11.1839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54679_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54679_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:03.37 -13:57:27.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 54686_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54686_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54691_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54691_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54703_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54703_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:28.07 -11:51:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.744 5114785194559113472 056.61794144106 -11.85357753366 11.8415 11.3910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54704_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54704_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54712_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54712_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54717_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54717_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54720_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54720_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54724_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54724_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54727_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54727_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54738_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54738_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54741_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54741_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:12.06 -07:46:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.995 3243061601129443456 056.79885218084 -07.77188938806 11.8574 11.4076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54745_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54745_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:56.05 -10:00:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.329 3194478202387067904 056.73438736756 -10.00804249395 12.0682 11.5984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54748_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54748_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54751_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54751_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:46.06 -06:04:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.998 3244474787104498176 057.19164545447 -06.06912404880 11.8359 11.2988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54769_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54769_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54775_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54775_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54776_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54776_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:41.94 -11:28:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 5.223 5115568798455582720 056.67619606159 -11.48277291358 11.7275 11.1911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54800_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54800_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:21.21 -06:27:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.103 3243638127476622464 057.83958264121 -06.46147684846 12.0359 11.5076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54801_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54801_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:46.64 -04:59:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.893 3246267089841310080 057.19543725779 -04.99357668663 11.9999 11.4740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54803_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54803_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54806_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54806_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54824_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54824_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54841_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54841_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54847_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54847_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:57.20 -08:58:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.781 3242641175370309504 056.73755750709 -08.96668118108 12.3369 11.8004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54852_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54852_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54853_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54853_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54864_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54864_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54865_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54865_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54869_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54869_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:23.91 -07:18:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.631 3243475159236325760 057.35023480875 -07.30225644459 12.2998 11.7741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54877_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54877_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54878_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54878_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54886_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54886_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:30:39.68 -12:54:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.407 3177727456272499584 067.66570745926 -12.90861301550 13.8824 13.3840 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#
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Considering the candidate 54889_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54889_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:34.82 -08:05:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 2.713 3242850396113513344 057.14577011792 -08.09588022994 12.4248 12.2242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54890_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54890_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:10.84 -06:36:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.150 3243658640240373632 057.54500615882 -06.61347320181 12.1061 11.5549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54893_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54893_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54904_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54904_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54914_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54914_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:10.01 -06:12:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 5.854 3245152773463210368 058.29273334866 -06.20712843756 12.2585 11.6725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54918_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54918_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:21.87 -04:51:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 5.551 3246293551135678336 057.34255281888 -04.85656670056 12.2363 11.7900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54922_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54922_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54944_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54944_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54949_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54949_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:21.00 -05:04:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.855 3246265066912592768 057.08868642017 -05.06901086995 12.1376 11.6454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54952_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54952_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:45:19.98 -11:08:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.604 5115645390608096896 056.33424588855 -11.13613062773 12.0154 11.4218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54956_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54956_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54967_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54967_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54968_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 54968_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 54977_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54977_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:11:51.25 -08:48:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.179 3192448989255117952 062.96323373787 -08.81319890928 13.6315 13.0980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54990_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54990_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 54991_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 54991_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:46:03.24 -10:45:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.223 5115759185765938048 056.51429281854 -10.76630260016 12.2746 11.8028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55003_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55003_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:13.41 -04:51:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.679 3246199371093668096 057.80727915717 -04.86508998874 12.2870 11.8186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55009_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55009_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55020_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55020_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:43.70 -06:03:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.517 3244466502111365376 057.43249663203 -06.06398132581 12.1518 11.6488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55023_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55023_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55031_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55031_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55050_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55050_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55052_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55052_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55087_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55087_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55095_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55095_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55106_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55106_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55139_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55139_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55149_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55149_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:51:36.15 -04:56:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.394 3246186176954217472 057.90138989755 -04.94369397541 12.5200 12.0407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55155_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55155_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55164_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55164_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55173_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55173_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55200_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55200_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55213_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55213_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:43.36 -05:24:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.945 3246004310859458688 057.68095821823 -05.41353714683 12.1986 11.6953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55228_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55228_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:45:48.48 -10:54:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.539 5115755169972693888 056.45352699783 -10.91348409843 12.7020 12.3253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55235_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55235_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55237_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55237_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:01.34 -08:49:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 3.733 3194702434039579136 057.25601603987 -08.82133356855 12.4419 11.7778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55238_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55238_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55248_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55248_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:35.47 -05:09:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.979 3246260600146607360 057.14881449829 -05.15637642617 12.1125 11.6330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55261_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55261_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:07.94 -05:06:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.986 3246095913921856896 057.53444280932 -05.10309610094 12.5275 11.9463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55275_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55275_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55278_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55278_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55301_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55301_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:23.98 -06:41:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.463 3243609505814508928 057.60056636289 -06.68780033600 12.9060 12.3952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55306_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55306_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55316_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55316_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:07.76 -05:15:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 5.377 3246068219972749440 057.28314070898 -05.24985226252 12.2913 11.8005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55346_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55346_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55347_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55347_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55384_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55384_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:45:12.50 -13:04:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.631 5114263334555765376 056.30196181319 -13.07959032190 12.2635 11.7655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55385_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55385_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:53.73 -07:32:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.103 3243444544709405184 056.97376851235 -07.53499011499 12.4942 11.8898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55393_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55393_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55416_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55416_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:53:13.96 -06:03:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 5.649 3245159198734274560 058.30942531105 -06.06130767764 12.8573 12.3493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55436_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55436_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55437_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55437_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:59.51 -08:06:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 5.594 3242852320258866432 056.99737562302 -08.11150147271 12.8265 12.2729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55455_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55455_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55463_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55463_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:30.19 -06:07:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 5.277 3244459978057257984 057.37675733831 -06.12480219027 12.6845 12.2525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55474_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55474_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:30:42.84 -06:42:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 4.817 3199297366148705280 067.67818487877 -06.71396751414 14.4329 13.9199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55522_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55522_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
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Considering the candidate 55527_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55527_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55528_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55528_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55529_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55529_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55534_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55534_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55551_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55551_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55580_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55580_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55582_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55582_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:19.02 -10:27:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 4.374 3194248649272544896 057.33023486078 -10.45076634888 13.0987 12.6205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55586_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55586_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55590_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55590_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 55622_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55622_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55629_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55629_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:48:09.13 -08:49:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 5.109 3242736317485816192 057.03944286582 -08.82108840223 12.7722 12.1014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55639_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55639_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55646_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55646_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55661_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55661_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55665_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55665_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:47:01.23 -08:12:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 4.858 3242855893671669376 056.75465472013 -08.20789997759 12.5497 12.0622 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55675_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55675_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55679_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55679_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 55697_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55697_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:49:03.97 -07:41:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.124 3243252989169155200 057.26701456842 -07.69366942408 13.0361 12.6480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55706_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55706_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55774_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55774_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55781_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55781_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:42:16.05 -10:50:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 0.624 3184276147526710784 070.56705090303 -10.84809813133 14.6329 14.1280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55824_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55824_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 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 55826_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 55826_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:50:19.87 -06:25:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 3.866 3243687742938758144 057.58379336657 -06.43081935440 12.9503 12.3731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55846_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 55846_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27638_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 27638_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19518_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 19518_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16250_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 16250_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:41:47.77 -07:57:19.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 14856_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
Preparing report for the candidate 14856_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45711_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 45711_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (32.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21158_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 21158_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 03:52:55.80 -09:10:07.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 26170_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077
The candidate 26170_Eri-04-Q2b1x1_2026-02-21_21-32-28_20.00sec_-15.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:14:23.82 -10:15:22.0 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 21s
make_report_in_HTML.sh TOTAL: 475s
Prepared the HTML report for the field Eri-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:41:47.76 -07:57:19.9
03:45:21.20 -12:52:15.0
03:52:56.16 -13:11:42.3
03:48:30.58 -13:35:22.9
03:51:34.57 -13:32:15.7
03:48:00.50 -12:21:47.2
03:53:10.14 -07:27:50.1
03:49:10.33 -12:53:58.7
03:51:25.28 -08:54:10.4
03:52:48.28 -08:47:49.8
03:52:07.70 -06:14:37.1
03:51:31.61 -07:38:15.7
03:52:55.77 -09:10:07.5
03:51:48.95 -06:40:42.4
03:46:35.21 -12:25:42.8
03:53:12.75 -06:57:12.8
03:51:56.87 -05:44:37.7
03:46:46.49 -13:48:31.4
03:51:08.68 -05:53:04.4
03:50:41.76 -07:03:58.4
04:12:38.53 -07:47:54.1
04:26:52.04 -08:40:15.7
04:20:19.44 -10:24:25.3
03:49:47.68 -12:16:26.3
03:49:41.50 -11:33:32.2
04:12:28.79 -05:30:31.5
03:49:12.64 -14:15:07.9
03:52:05.12 -08:40:27.9
03:49:49.13 -05:52:27.9
03:52:19.44 -14:23:31.9
03:52:49.64 -09:19:03.8
03:46:40.94 -12:35:00.2
03:48:21.63 -13:50:06.3
03:51:50.60 -10:33:01.9
03:51:59.07 -09:28:04.2
03:54:37.54 -13:32:56.3
03:56:30.38 -05:02:09.5
03:50:56.66 -11:54:48.6
03:48:35.69 -11:10:40.2
03:46:36.75 -14:18:13.1
03:48:29.20 -11:38:15.8
03:49:45.92 -12:28:55.9
03:49:06.17 -08:19:44.2
03:54:31.19 -08:43:08.0
03:50:44.63 -10:26:14.9
03:51:14.76 -10:24:29.6
03:50:00.70 -10:34:43.1
03:49:32.40 -06:18:35.8
04:07:32.82 -08:34:19.4
03:47:21.53 -10:48:12.4
03:58:44.77 -05:09:21.5
03:50:20.84 -12:37:48.3
03:58:28.09 -05:02:42.7
03:56:30.44 -05:57:19.0
03:55:08.87 -06:37:09.2
03:51:12.34 -07:41:37.3
03:50:08.56 -11:25:14.2
03:51:54.10 -12:51:39.5
03:54:06.99 -07:37:21.1
03:51:10.25 -11:50:47.4
03:56:19.91 -05:59:00.8
03:56:41.54 -05:19:18.0
03:50:27.79 -07:27:33.2
03:48:47.95 -10:42:27.6
03:49:58.65 -11:44:51.0
03:49:23.79 -13:34:19.4
03:50:31.72 -10:23:04.2
03:51:20.43 -14:16:46.7
03:53:53.64 -08:40:06.7
03:50:48.88 -11:10:50.2
03:58:16.87 -05:57:10.0
03:51:17.37 -13:32:08.3
04:00:43.79 -05:06:38.2
03:51:07.41 -09:49:54.7
03:51:13.85 -11:05:04.6
03:53:11.71 -05:59:11.3
03:54:22.86 -07:06:03.4
03:57:55.22 -05:38:11.8
03:50:22.18 -10:38:01.2
03:48:11.53 -13:54:28.0
03:56:58.38 -05:27:12.1
03:51:01.64 -13:39:45.3
03:52:39.60 -08:27:33.9
03:58:07.97 -05:02:51.9
03:48:29.45 -13:38:59.4
03:51:01.28 -06:03:40.1
03:46:50.24 -09:23:17.5
03:56:14.05 -04:59:47.0
03:47:17.61 -08:57:18.8
03:53:38.64 -06:06:30.3
03:47:15.12 -11:04:31.1
03:53:09.70 -05:59:11.9
03:48:04.92 -10:12:38.2
03:52:53.79 -06:32:50.3
03:51:42.07 -05:02:28.9
03:55:42.76 -05:26:22.7
03:54:51.91 -06:50:12.3
03:51:16.97 -06:20:49.9
03:54:59.77 -05:12:33.3
03:56:36.47 -05:21:11.7
03:47:30.11 -09:29:34.2
03:45:20.32 -12:52:19.7
03:53:28.67 -05:39:12.4
03:54:40.31 -05:39:20.5
03:54:47.91 -05:35:42.9
03:49:55.70 -05:29:45.7
03:52:10.18 -06:23:21.0
03:51:06.92 -07:35:27.9
03:47:24.78 -10:47:34.8
03:50:39.84 -04:53:12.3
03:53:25.75 -06:06:09.0
03:53:35.11 -05:57:30.5
03:54:00.28 -06:14:11.3
03:48:24.18 -07:39:24.9
03:53:12.76 -06:55:24.3
03:46:38.86 -10:32:48.7
03:49:52.35 -06:40:42.8
03:57:40.59 -05:12:07.6
03:53:53.55 -05:56:24.4
03:52:58.61 -05:51:53.9
03:49:45.41 -09:22:03.7
03:53:57.80 -05:02:32.7
03:47:33.56 -09:33:17.3
03:56:32.99 -04:52:02.6
03:50:23.30 -05:41:52.9
03:48:28.71 -08:05:35.8
03:50:52.66 -04:59:02.1
03:54:16.16 -05:34:06.2
03:51:00.45 -10:28:37.6
03:49:13.07 -06:44:31.1
03:45:42.04 -10:21:56.1
03:52:21.39 -06:29:02.3
03:50:43.83 -06:06:51.7
03:48:54.77 -07:15:38.7
03:54:57.51 -06:07:57.3
03:52:51.64 -04:58:03.3
03:45:29.41 -12:19:17.7
03:52:27.23 -06:36:05.1
03:51:03.18 -07:59:49.9
03:53:09.15 -05:20:16.3
03:53:16.85 -07:58:02.8
03:51:12.61 -07:26:09.0
03:49:16.30 -12:08:49.6
03:46:42.80 -12:29:04.6
03:54:29.15 -06:23:45.2
03:53:13.71 -05:17:15.6
03:48:35.63 -05:20:32.1
03:54:00.85 -05:50:16.1
03:51:47.94 -06:46:27.0
03:51:05.65 -05:43:06.9
03:53:18.55 -05:36:01.7
03:49:05.67 -10:23:58.4
03:49:13.92 -11:31:15.1
03:52:54.55 -10:44:44.4
03:53:36.18 -05:19:55.9
03:54:53.27 -05:16:25.5
03:48:37.69 -06:41:51.0
03:50:22.16 -05:07:34.8
03:48:05.25 -05:33:39.4
03:49:29.23 -08:49:23.1
03:46:46.74 -12:06:13.6
03:53:23.28 -08:03:23.7
03:52:02.44 -07:25:59.2
03:49:10.95 -09:54:26.1
03:48:41.59 -12:05:57.5
03:55:44.62 -05:29:04.3
03:51:14.16 -06:52:12.2
03:56:23.12 -05:37:39.4
03:51:14.97 -06:55:24.5
03:45:57.50 -13:00:00.6
03:49:30.50 -05:57:56.4
03:48:22.35 -13:59:10.0
03:46:47.29 -14:12:46.3
03:52:39.44 -06:27:58.6
03:50:11.46 -05:40:10.7
03:45:58.17 -13:42:45.1
03:53:35.22 -07:11:51.7
03:46:47.74 -12:06:34.6
03:46:17.90 -09:16:18.0
03:49:31.78 -06:21:59.4
03:49:09.21 -04:53:26.6
03:48:47.37 -07:04:15.4
03:51:19.53 -07:01:56.8
03:47:52.61 -07:39:54.1
03:51:58.89 -05:21:18.0
03:50:42.21 -05:24:56.6
03:45:58.57 -13:00:19.2
03:50:24.95 -05:44:42.6
03:48:38.60 -14:03:40.0
03:57:05.95 -05:03:13.2
03:52:06.88 -04:52:12.9
03:46:47.65 -10:56:48.2
03:52:04.14 -05:16:08.8
03:50:07.04 -05:18:05.7
03:50:44.24 -05:12:59.0
03:54:46.08 -06:19:35.2
03:55:30.03 -05:33:14.0
03:50:07.49 -05:30:36.3
03:45:24.39 -13:46:57.7
########### Completed Eri-04-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 ####
03:45:21.20 -12:52:15.0
03:52:56.16 -13:11:42.3
03:48:30.58 -13:35:22.9
03:51:34.57 -13:32:15.7
03:48:00.50 -12:21:47.2
03:53:10.14 -07:27:50.1
03:49:10.33 -12:53:58.7
03:51:25.28 -08:54:10.4
03:52:48.28 -08:47:49.8
03:52:07.70 -06:14:37.1
03:51:31.61 -07:38:15.7
03:52:55.77 -09:10:07.5
03:51:48.95 -06:40:42.4
03:46:35.21 -12:25:42.8
03:53:12.75 -06:57:12.8
03:51:56.87 -05:44:37.7
03:46:46.49 -13:48:31.4
03:51:08.68 -05:53:04.4
03:50:41.76 -07:03:58.4
04:41:47.76 -07:57:19.9
03:49:47.68 -12:16:26.3
03:49:41.50 -11:33:32.2
04:12:28.79 -05:30:31.5
03:49:12.64 -14:15:07.9
03:52:05.12 -08:40:27.9
03:49:49.13 -05:52:27.9
03:52:19.44 -14:23:31.9
03:52:49.64 -09:19:03.8
03:46:40.94 -12:35:00.2
03:48:21.63 -13:50:06.3
03:51:50.60 -10:33:01.9
03:51:59.07 -09:28:04.2
03:54:37.54 -13:32:56.3
03:56:30.38 -05:02:09.5
03:50:56.66 -11:54:48.6
03:48:35.69 -11:10:40.2
03:46:36.75 -14:18:13.1
03:48:29.20 -11:38:15.8
03:49:45.92 -12:28:55.9
03:49:06.17 -08:19:44.2
03:54:31.19 -08:43:08.0
03:50:44.63 -10:26:14.9
03:51:14.76 -10:24:29.6
03:50:00.70 -10:34:43.1
03:49:32.40 -06:18:35.8
04:07:32.82 -08:34:19.4
03:47:21.53 -10:48:12.4
03:58:44.77 -05:09:21.5
03:50:20.84 -12:37:48.3
03:58:28.09 -05:02:42.7
03:56:30.44 -05:57:19.0
03:55:08.87 -06:37:09.2
03:51:12.34 -07:41:37.3
03:50:08.56 -11:25:14.2
03:51:54.10 -12:51:39.5
03:54:06.99 -07:37:21.1
03:51:10.25 -11:50:47.4
03:56:19.91 -05:59:00.8
03:56:41.54 -05:19:18.0
03:50:27.79 -07:27:33.2
03:48:47.95 -10:42:27.6
03:49:58.65 -11:44:51.0
03:49:23.79 -13:34:19.4
03:50:31.72 -10:23:04.2
03:51:20.43 -14:16:46.7
03:53:53.64 -08:40:06.7
03:50:48.88 -11:10:50.2
03:58:16.87 -05:57:10.0
03:51:17.37 -13:32:08.3
04:00:43.79 -05:06:38.2
03:51:07.41 -09:49:54.7
03:51:13.85 -11:05:04.6
03:53:11.71 -05:59:11.3
03:54:22.86 -07:06:03.4
03:57:55.22 -05:38:11.8
03:50:22.18 -10:38:01.2
03:48:11.53 -13:54:28.0
03:56:58.38 -05:27:12.1
03:51:01.64 -13:39:45.3
03:52:39.60 -08:27:33.9
03:58:07.97 -05:02:51.9
03:48:29.45 -13:38:59.4
03:51:01.28 -06:03:40.1
03:46:50.24 -09:23:17.5
03:56:14.05 -04:59:47.0
03:47:17.61 -08:57:18.8
03:53:38.64 -06:06:30.3
03:47:15.12 -11:04:31.1
03:53:09.70 -05:59:11.9
03:48:04.92 -10:12:38.2
03:52:53.79 -06:32:50.3
03:51:42.07 -05:02:28.9
03:55:42.76 -05:26:22.7
03:54:51.91 -06:50:12.3
03:51:16.97 -06:20:49.9
03:54:59.77 -05:12:33.3
03:56:36.47 -05:21:11.7
03:47:30.11 -09:29:34.2
03:45:20.32 -12:52:19.7
03:53:28.67 -05:39:12.4
03:54:40.31 -05:39:20.5
03:54:47.91 -05:35:42.9
03:49:55.70 -05:29:45.7
03:52:10.18 -06:23:21.0
03:51:06.92 -07:35:27.9
03:47:24.78 -10:47:34.8
03:50:39.84 -04:53:12.3
03:53:25.75 -06:06:09.0
03:53:35.11 -05:57:30.5
03:54:00.28 -06:14:11.3
03:48:24.18 -07:39:24.9
03:53:12.76 -06:55:24.3
03:46:38.86 -10:32:48.7
03:49:52.35 -06:40:42.8
03:57:40.59 -05:12:07.6
03:53:53.55 -05:56:24.4
03:52:58.61 -05:51:53.9
03:49:45.41 -09:22:03.7
03:53:57.80 -05:02:32.7
03:47:33.56 -09:33:17.3
03:56:32.99 -04:52:02.6
03:50:23.30 -05:41:52.9
03:48:28.71 -08:05:35.8
03:50:52.66 -04:59:02.1
03:54:16.16 -05:34:06.2
03:51:00.45 -10:28:37.6
03:49:13.07 -06:44:31.1
03:45:42.04 -10:21:56.1
03:52:21.39 -06:29:02.3
03:50:43.83 -06:06:51.7
03:48:54.77 -07:15:38.7
03:54:57.51 -06:07:57.3
03:52:51.64 -04:58:03.3
03:45:29.41 -12:19:17.7
03:52:27.23 -06:36:05.1
03:51:03.18 -07:59:49.9
03:53:09.15 -05:20:16.3
03:53:16.85 -07:58:02.8
03:51:12.61 -07:26:09.0
03:49:16.30 -12:08:49.6
03:46:42.80 -12:29:04.6
03:54:29.15 -06:23:45.2
03:53:13.71 -05:17:15.6
03:48:35.63 -05:20:32.1
03:54:00.85 -05:50:16.1
03:51:47.94 -06:46:27.0
03:51:05.65 -05:43:06.9
03:53:18.55 -05:36:01.7
03:49:05.67 -10:23:58.4
03:49:13.92 -11:31:15.1
03:52:54.55 -10:44:44.4
03:53:36.18 -05:19:55.9
03:54:53.27 -05:16:25.5
03:48:37.69 -06:41:51.0
03:50:22.16 -05:07:34.8
03:48:05.25 -05:33:39.4
03:49:29.23 -08:49:23.1
03:46:46.74 -12:06:13.6
03:53:23.28 -08:03:23.7
03:52:02.44 -07:25:59.2
03:49:10.95 -09:54:26.1
03:48:41.59 -12:05:57.5
03:55:44.62 -05:29:04.3
03:51:14.16 -06:52:12.2
03:56:23.12 -05:37:39.4
03:51:14.97 -06:55:24.5
03:45:57.50 -13:00:00.6
03:49:30.50 -05:57:56.4
03:48:22.35 -13:59:10.0
03:46:47.29 -14:12:46.3
03:52:39.44 -06:27:58.6
03:50:11.46 -05:40:10.7
03:45:58.17 -13:42:45.1
03:53:35.22 -07:11:51.7
03:46:47.74 -12:06:34.6
03:46:17.90 -09:16:18.0
03:49:31.78 -06:21:59.4
03:49:09.21 -04:53:26.6
03:48:47.37 -07:04:15.4
03:51:19.53 -07:01:56.8
03:47:52.61 -07:39:54.1
03:51:58.89 -05:21:18.0
03:50:42.21 -05:24:56.6
03:45:58.57 -13:00:19.2
03:50:24.95 -05:44:42.6
03:48:38.60 -14:03:40.0
03:57:05.95 -05:03:13.2
03:52:06.88 -04:52:12.9
03:46:47.65 -10:56:48.2
03:52:04.14 -05:16:08.8
03:50:07.04 -05:18:05.7
03:50:44.24 -05:12:59.0
03:54:46.08 -06:19:35.2
03:55:30.03 -05:33:14.0
03:50:07.49 -05:30:36.3
03:45:24.39 -13:46:57.7
04:20:19.44 -10:24:25.3
04:26:52.04 -08:40:15.7
04:12:38.53 -07:47:54.1
###################################################################################
03:45:21.20 -12:52:15.0 -- not an asteroid (will add it to exclusion list)
03:52:56.16 -13:11:42.3 -- not an asteroid (will add it to exclusion list)
03:48:30.58 -13:35:22.9 -- not an asteroid (will add it to exclusion list)
03:51:34.57 -13:32:15.7 -- not an asteroid (will add it to exclusion list)
03:48:00.50 -12:21:47.2 -- not an asteroid (will add it to exclusion list)
03:53:10.14 -07:27:50.1 -- not an asteroid (will add it to exclusion list)
03:49:10.33 -12:53:58.7 -- not an asteroid (will add it to exclusion list)
03:51:25.28 -08:54:10.4 -- not an asteroid (will add it to exclusion list)
03:52:48.28 -08:47:49.8 -- not an asteroid (will add it to exclusion list)
03:52:07.70 -06:14:37.1 -- not an asteroid (will add it to exclusion list)
03:51:31.61 -07:38:15.7 -- not an asteroid (will add it to exclusion list)
03:52:55.77 -09:10:07.5 -- not an asteroid (will add it to exclusion list)
03:51:48.95 -06:40:42.4 -- not an asteroid (will add it to exclusion list)
03:46:35.21 -12:25:42.8 -- not an asteroid (will add it to exclusion list)
03:53:12.75 -06:57:12.8 -- not an asteroid (will add it to exclusion list)
03:51:56.87 -05:44:37.7 -- not an asteroid (will add it to exclusion list)
03:46:46.49 -13:48:31.4 -- not an asteroid (will add it to exclusion list)
03:51:08.68 -05:53:04.4 -- not an asteroid (will add it to exclusion list)
03:50:41.76 -07:03:58.4 -- not an asteroid (will add it to exclusion list)
04:41:47.76 -07:57:19.9 -- not an asteroid (will add it to exclusion list)
03:49:47.68 -12:16:26.3 -- not an asteroid (will add it to exclusion list)
03:49:41.50 -11:33:32.2 -- not an asteroid (will add it to exclusion list)
04:12:28.79 -05:30:31.5 -- not an asteroid (will add it to exclusion list)
03:49:12.64 -14:15:07.9 -- not an asteroid (will add it to exclusion list)
03:52:05.12 -08:40:27.9 -- not an asteroid (will add it to exclusion list)
03:49:49.13 -05:52:27.9 -- not an asteroid (will add it to exclusion list)
03:52:19.44 -14:23:31.9 -- not an asteroid (will add it to exclusion list)
03:52:49.64 -09:19:03.8 -- not an asteroid (will add it to exclusion list)
03:46:40.94 -12:35:00.2 -- not an asteroid (will add it to exclusion list)
03:48:21.63 -13:50:06.3 -- not an asteroid (will add it to exclusion list)
03:51:50.60 -10:33:01.9 -- not an asteroid (will add it to exclusion list)
03:51:59.07 -09:28:04.2 -- not an asteroid (will add it to exclusion list)
03:54:37.54 -13:32:56.3 -- not an asteroid (will add it to exclusion list)
03:56:30.38 -05:02:09.5 -- not an asteroid (will add it to exclusion list)
03:50:56.66 -11:54:48.6 -- not an asteroid (will add it to exclusion list)
03:48:35.69 -11:10:40.2 -- not an asteroid (will add it to exclusion list)
03:46:36.75 -14:18:13.1 -- not an asteroid (will add it to exclusion list)
03:48:29.20 -11:38:15.8 -- not an asteroid (will add it to exclusion list)
03:49:45.92 -12:28:55.9 -- not an asteroid (will add it to exclusion list)
03:49:06.17 -08:19:44.2 -- not an asteroid (will add it to exclusion list)
03:54:31.19 -08:43:08.0 -- not an asteroid (will add it to exclusion list)
03:50:44.63 -10:26:14.9 -- not an asteroid (will add it to exclusion list)
03:51:14.76 -10:24:29.6 -- not an asteroid (will add it to exclusion list)
03:50:00.70 -10:34:43.1 -- not an asteroid (will add it to exclusion list)
03:49:32.40 -06:18:35.8 -- not an asteroid (will add it to exclusion list)
04:07:32.82 -08:34:19.4 -- not an asteroid (will add it to exclusion list)
03:47:21.53 -10:48:12.4 -- not an asteroid (will add it to exclusion list)
03:58:44.77 -05:09:21.5 -- not an asteroid (will add it to exclusion list)
03:50:20.84 -12:37:48.3 -- not an asteroid (will add it to exclusion list)
03:58:28.09 -05:02:42.7 -- not an asteroid (will add it to exclusion list)
03:56:30.44 -05:57:19.0 -- not an asteroid (will add it to exclusion list)
03:55:08.87 -06:37:09.2 -- not an asteroid (will add it to exclusion list)
03:51:12.34 -07:41:37.3 -- not an asteroid (will add it to exclusion list)
03:50:08.56 -11:25:14.2 -- not an asteroid (will add it to exclusion list)
03:51:54.10 -12:51:39.5 -- not an asteroid (will add it to exclusion list)
03:54:06.99 -07:37:21.1 -- not an asteroid (will add it to exclusion list)
03:51:10.25 -11:50:47.4 -- not an asteroid (will add it to exclusion list)
03:56:19.91 -05:59:00.8 -- not an asteroid (will add it to exclusion list)
03:56:41.54 -05:19:18.0 -- not an asteroid (will add it to exclusion list)
03:50:27.79 -07:27:33.2 -- not an asteroid (will add it to exclusion list)
03:48:47.95 -10:42:27.6 -- not an asteroid (will add it to exclusion list)
03:49:58.65 -11:44:51.0 -- not an asteroid (will add it to exclusion list)
03:49:23.79 -13:34:19.4 -- not an asteroid (will add it to exclusion list)
03:50:31.72 -10:23:04.2 -- not an asteroid (will add it to exclusion list)
03:51:20.43 -14:16:46.7 -- not an asteroid (will add it to exclusion list)
03:53:53.64 -08:40:06.7 -- not an asteroid (will add it to exclusion list)
03:50:48.88 -11:10:50.2 -- not an asteroid (will add it to exclusion list)
03:58:16.87 -05:57:10.0 -- not an asteroid (will add it to exclusion list)
03:51:17.37 -13:32:08.3 -- not an asteroid (will add it to exclusion list)
04:00:43.79 -05:06:38.2 -- not an asteroid (will add it to exclusion list)
03:51:07.41 -09:49:54.7 -- not an asteroid (will add it to exclusion list)
03:51:13.85 -11:05:04.6 -- not an asteroid (will add it to exclusion list)
03:53:11.71 -05:59:11.3 -- not an asteroid (will add it to exclusion list)
03:54:22.86 -07:06:03.4 -- not an asteroid (will add it to exclusion list)
03:57:55.22 -05:38:11.8 -- not an asteroid (will add it to exclusion list)
03:50:22.18 -10:38:01.2 -- not an asteroid (will add it to exclusion list)
03:48:11.53 -13:54:28.0 -- not an asteroid (will add it to exclusion list)
03:56:58.38 -05:27:12.1 -- not an asteroid (will add it to exclusion list)
03:51:01.64 -13:39:45.3 -- not an asteroid (will add it to exclusion list)
03:52:39.60 -08:27:33.9 -- not an asteroid (will add it to exclusion list)
03:58:07.97 -05:02:51.9 -- not an asteroid (will add it to exclusion list)
03:48:29.45 -13:38:59.4 -- not an asteroid (will add it to exclusion list)
03:51:01.28 -06:03:40.1 -- not an asteroid (will add it to exclusion list)
03:46:50.24 -09:23:17.5 -- not an asteroid (will add it to exclusion list)
03:56:14.05 -04:59:47.0 -- not an asteroid (will add it to exclusion list)
03:47:17.61 -08:57:18.8 -- not an asteroid (will add it to exclusion list)
03:53:38.64 -06:06:30.3 -- not an asteroid (will add it to exclusion list)
03:47:15.12 -11:04:31.1 -- not an asteroid (will add it to exclusion list)
03:53:09.70 -05:59:11.9 -- not an asteroid (will add it to exclusion list)
03:48:04.92 -10:12:38.2 -- not an asteroid (will add it to exclusion list)
03:52:53.79 -06:32:50.3 -- not an asteroid (will add it to exclusion list)
03:51:42.07 -05:02:28.9 -- not an asteroid (will add it to exclusion list)
03:55:42.76 -05:26:22.7 -- not an asteroid (will add it to exclusion list)
03:54:51.91 -06:50:12.3 -- not an asteroid (will add it to exclusion list)
03:51:16.97 -06:20:49.9 -- not an asteroid (will add it to exclusion list)
03:54:59.77 -05:12:33.3 -- not an asteroid (will add it to exclusion list)
03:56:36.47 -05:21:11.7 -- not an asteroid (will add it to exclusion list)
03:47:30.11 -09:29:34.2 -- not an asteroid (will add it to exclusion list)
03:45:20.32 -12:52:19.7 -- not an asteroid (will add it to exclusion list)
03:53:28.67 -05:39:12.4 -- not an asteroid (will add it to exclusion list)
03:54:40.31 -05:39:20.5 -- not an asteroid (will add it to exclusion list)
03:54:47.91 -05:35:42.9 -- not an asteroid (will add it to exclusion list)
03:49:55.70 -05:29:45.7 -- not an asteroid (will add it to exclusion list)
03:52:10.18 -06:23:21.0 -- not an asteroid (will add it to exclusion list)
03:51:06.92 -07:35:27.9 -- not an asteroid (will add it to exclusion list)
03:47:24.78 -10:47:34.8 -- not an asteroid (will add it to exclusion list)
03:50:39.84 -04:53:12.3 -- not an asteroid (will add it to exclusion list)
03:53:25.75 -06:06:09.0 -- not an asteroid (will add it to exclusion list)
03:53:35.11 -05:57:30.5 -- not an asteroid (will add it to exclusion list)
03:54:00.28 -06:14:11.3 -- not an asteroid (will add it to exclusion list)
03:48:24.18 -07:39:24.9 -- not an asteroid (will add it to exclusion list)
03:53:12.76 -06:55:24.3 -- not an asteroid (will add it to exclusion list)
03:46:38.86 -10:32:48.7 -- not an asteroid (will add it to exclusion list)
03:49:52.35 -06:40:42.8 -- not an asteroid (will add it to exclusion list)
03:57:40.59 -05:12:07.6 -- not an asteroid (will add it to exclusion list)
03:53:53.55 -05:56:24.4 -- not an asteroid (will add it to exclusion list)
03:52:58.61 -05:51:53.9 -- not an asteroid (will add it to exclusion list)
03:49:45.41 -09:22:03.7 -- not an asteroid (will add it to exclusion list)
03:53:57.80 -05:02:32.7 -- not an asteroid (will add it to exclusion list)
03:47:33.56 -09:33:17.3 -- not an asteroid (will add it to exclusion list)
03:56:32.99 -04:52:02.6 -- not an asteroid (will add it to exclusion list)
03:50:23.30 -05:41:52.9 -- not an asteroid (will add it to exclusion list)
03:48:28.71 -08:05:35.8 -- not an asteroid (will add it to exclusion list)
03:50:52.66 -04:59:02.1 -- not an asteroid (will add it to exclusion list)
03:54:16.16 -05:34:06.2 -- not an asteroid (will add it to exclusion list)
03:51:00.45 -10:28:37.6 -- not an asteroid (will add it to exclusion list)
03:49:13.07 -06:44:31.1 -- not an asteroid (will add it to exclusion list)
03:45:42.04 -10:21:56.1 -- not an asteroid (will add it to exclusion list)
03:52:21.39 -06:29:02.3 -- not an asteroid (will add it to exclusion list)
03:50:43.83 -06:06:51.7 -- not an asteroid (will add it to exclusion list)
03:48:54.77 -07:15:38.7 -- not an asteroid (will add it to exclusion list)
03:54:57.51 -06:07:57.3 -- not an asteroid (will add it to exclusion list)
03:52:51.64 -04:58:03.3 -- not an asteroid (will add it to exclusion list)
03:45:29.41 -12:19:17.7 -- not an asteroid (will add it to exclusion list)
03:52:27.23 -06:36:05.1 -- not an asteroid (will add it to exclusion list)
03:51:03.18 -07:59:49.9 -- not an asteroid (will add it to exclusion list)
03:53:09.15 -05:20:16.3 -- not an asteroid (will add it to exclusion list)
03:53:16.85 -07:58:02.8 -- not an asteroid (will add it to exclusion list)
03:51:12.61 -07:26:09.0 -- not an asteroid (will add it to exclusion list)
03:49:16.30 -12:08:49.6 -- not an asteroid (will add it to exclusion list)
03:46:42.80 -12:29:04.6 -- not an asteroid (will add it to exclusion list)
03:54:29.15 -06:23:45.2 -- not an asteroid (will add it to exclusion list)
03:53:13.71 -05:17:15.6 -- not an asteroid (will add it to exclusion list)
03:48:35.63 -05:20:32.1 -- not an asteroid (will add it to exclusion list)
03:54:00.85 -05:50:16.1 -- not an asteroid (will add it to exclusion list)
03:51:47.94 -06:46:27.0 -- not an asteroid (will add it to exclusion list)
03:51:05.65 -05:43:06.9 -- not an asteroid (will add it to exclusion list)
03:53:18.55 -05:36:01.7 -- not an asteroid (will add it to exclusion list)
03:49:05.67 -10:23:58.4 -- not an asteroid (will add it to exclusion list)
03:49:13.92 -11:31:15.1 -- not an asteroid (will add it to exclusion list)
03:52:54.55 -10:44:44.4 -- not an asteroid (will add it to exclusion list)
03:53:36.18 -05:19:55.9 -- not an asteroid (will add it to exclusion list)
03:54:53.27 -05:16:25.5 -- not an asteroid (will add it to exclusion list)
03:48:37.69 -06:41:51.0 -- not an asteroid (will add it to exclusion list)
03:50:22.16 -05:07:34.8 -- not an asteroid (will add it to exclusion list)
03:48:05.25 -05:33:39.4 -- not an asteroid (will add it to exclusion list)
03:49:29.23 -08:49:23.1 -- not an asteroid (will add it to exclusion list)
03:46:46.74 -12:06:13.6 -- not an asteroid (will add it to exclusion list)
03:53:23.28 -08:03:23.7 -- not an asteroid (will add it to exclusion list)
03:52:02.44 -07:25:59.2 -- not an asteroid (will add it to exclusion list)
03:49:10.95 -09:54:26.1 -- not an asteroid (will add it to exclusion list)
03:48:41.59 -12:05:57.5 -- not an asteroid (will add it to exclusion list)
03:55:44.62 -05:29:04.3 -- not an asteroid (will add it to exclusion list)
03:51:14.16 -06:52:12.2 -- not an asteroid (will add it to exclusion list)
03:56:23.12 -05:37:39.4 -- not an asteroid (will add it to exclusion list)
03:51:14.97 -06:55:24.5 -- not an asteroid (will add it to exclusion list)
03:45:57.50 -13:00:00.6 -- not an asteroid (will add it to exclusion list)
03:49:30.50 -05:57:56.4 -- not an asteroid (will add it to exclusion list)
03:48:22.35 -13:59:10.0 -- not an asteroid (will add it to exclusion list)
03:46:47.29 -14:12:46.3 -- not an asteroid (will add it to exclusion list)
03:52:39.44 -06:27:58.6 -- not an asteroid (will add it to exclusion list)
03:50:11.46 -05:40:10.7 -- not an asteroid (will add it to exclusion list)
03:45:58.17 -13:42:45.1 -- not an asteroid (will add it to exclusion list)
03:53:35.22 -07:11:51.7 -- not an asteroid (will add it to exclusion list)
03:46:47.74 -12:06:34.6 -- not an asteroid (will add it to exclusion list)
03:46:17.90 -09:16:18.0 -- not an asteroid (will add it to exclusion list)
03:49:31.78 -06:21:59.4 -- not an asteroid (will add it to exclusion list)
03:49:09.21 -04:53:26.6 -- not an asteroid (will add it to exclusion list)
03:48:47.37 -07:04:15.4 -- not an asteroid (will add it to exclusion list)
03:51:19.53 -07:01:56.8 -- not an asteroid (will add it to exclusion list)
03:47:52.61 -07:39:54.1 -- not an asteroid (will add it to exclusion list)
03:51:58.89 -05:21:18.0 -- not an asteroid (will add it to exclusion list)
03:50:42.21 -05:24:56.6 -- not an asteroid (will add it to exclusion list)
03:45:58.57 -13:00:19.2 -- not an asteroid (will add it to exclusion list)
03:50:24.95 -05:44:42.6 -- not an asteroid (will add it to exclusion list)
03:48:38.60 -14:03:40.0 -- not an asteroid (will add it to exclusion list)
03:57:05.95 -05:03:13.2 -- not an asteroid (will add it to exclusion list)
03:52:06.88 -04:52:12.9 -- not an asteroid (will add it to exclusion list)
03:46:47.65 -10:56:48.2 -- not an asteroid (will add it to exclusion list)
03:52:04.14 -05:16:08.8 -- not an asteroid (will add it to exclusion list)
03:50:07.04 -05:18:05.7 -- not an asteroid (will add it to exclusion list)
03:50:44.24 -05:12:59.0 -- not an asteroid (will add it to exclusion list)
03:54:46.08 -06:19:35.2 -- not an asteroid (will add it to exclusion list)
03:55:30.03 -05:33:14.0 -- not an asteroid (will add it to exclusion list)
03:50:07.49 -05:30:36.3 -- not an asteroid (will add it to exclusion list)
03:45:24.39 -13:46:57.7 -- not an asteroid (will add it to exclusion list)
04:20:19.44 -10:24:25.3 -- not an asteroid (will add it to exclusion list)
04:26:52.04 -08:40:15.7 -- not an asteroid (will add it to exclusion list)
04:12:38.53 -07:47:54.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:45:20.32 -12:52:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:21.20 -12:52:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:24.39 -13:46:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:29.41 -12:19:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:42.04 -10:21:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:57.50 -13:00:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:58.17 -13:42:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:58.57 -13:00:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:17.90 -09:16:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:35.21 -12:25:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:36.75 -14:18:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:38.86 -10:32:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:40.94 -12:35:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:42.80 -12:29:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:46.49 -13:48:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:46.74 -12:06:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:47.29 -14:12:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:47.65 -10:56:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:47.74 -12:06:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:50.24 -09:23:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:15.12 -11:04:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:17.61 -08:57:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:21.53 -10:48:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:24.78 -10:47:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:30.11 -09:29:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:33.56 -09:33:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:52.61 -07:39:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:00.50 -12:21:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:04.92 -10:12:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:05.25 -05:33:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:11.53 -13:54:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:21.63 -13:50:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:22.35 -13:59:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:24.18 -07:39:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:28.71 -08:05:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:29.20 -11:38:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:29.45 -13:38:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:30.58 -13:35:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:35.63 -05:20:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:35.69 -11:10:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:37.69 -06:41:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:38.60 -14:03:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:41.59 -12:05:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:47.37 -07:04:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:47.95 -10:42:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:54.77 -07:15:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:05.67 -10:23:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:06.17 -08:19:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:09.21 -04:53:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:10.33 -12:53:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:10.95 -09:54:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:12.64 -14:15:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:13.07 -06:44:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:13.92 -11:31:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:16.30 -12:08:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:23.79 -13:34:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:29.23 -08:49:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:30.50 -05:57:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:31.78 -06:21:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:32.40 -06:18:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:41.50 -11:33:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:45.41 -09:22:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:45.92 -12:28:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:47.68 -12:16:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:49.13 -05:52:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:52.35 -06:40:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:55.70 -05:29:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:58.65 -11:44:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:00.70 -10:34:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:07.04 -05:18:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:07.49 -05:30:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:08.56 -11:25:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:11.46 -05:40:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:20.84 -12:37:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:22.16 -05:07:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:22.18 -10:38:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:23.30 -05:41:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:24.95 -05:44:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:27.79 -07:27:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:31.72 -10:23:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:39.84 -04:53:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:41.76 -07:03:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:42.21 -05:24:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:43.83 -06:06:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:44.24 -05:12:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:44.63 -10:26:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:48.88 -11:10:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:52.66 -04:59:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:56.66 -11:54:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:00.45 -10:28:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:01.28 -06:03:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:01.64 -13:39:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:03.18 -07:59:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:05.65 -05:43:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:06.92 -07:35:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:07.41 -09:49:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:08.68 -05:53:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:10.25 -11:50:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:12.34 -07:41:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:12.61 -07:26:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:13.85 -11:05:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:14.16 -06:52:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:14.76 -10:24:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:14.97 -06:55:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:16.97 -06:20:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:17.37 -13:32:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:19.53 -07:01:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:20.43 -14:16:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:25.28 -08:54:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:31.61 -07:38:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:34.57 -13:32:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:42.07 -05:02:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:47.94 -06:46:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:48.95 -06:40:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:50.60 -10:33:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:54.10 -12:51:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:56.87 -05:44:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:58.89 -05:21:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:59.07 -09:28:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:02.44 -07:25:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:04.14 -05:16:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:05.12 -08:40:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:06.88 -04:52:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:07.70 -06:14:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:10.18 -06:23:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:19.44 -14:23:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:21.39 -06:29:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:27.23 -06:36:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:39.44 -06:27:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:39.60 -08:27:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:48.28 -08:47:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:49.64 -09:19:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:51.64 -04:58:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:53.79 -06:32:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:54.55 -10:44:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:55.77 -09:10:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:56.16 -13:11:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:58.61 -05:51:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:09.15 -05:20:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:09.70 -05:59:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:10.14 -07:27:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:11.71 -05:59:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:12.75 -06:57:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:12.76 -06:55:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:13.71 -05:17:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:16.85 -07:58:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:18.55 -05:36:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:23.28 -08:03:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:25.75 -06:06:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:28.67 -05:39:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:35.11 -05:57:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:35.22 -07:11:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:36.18 -05:19:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:38.64 -06:06:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:53.55 -05:56:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:53.64 -08:40:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:57.80 -05:02:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:00.28 -06:14:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:00.85 -05:50:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:06.99 -07:37:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:16.16 -05:34:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:22.86 -07:06:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:29.15 -06:23:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:31.19 -08:43:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:37.54 -13:32:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:40.31 -05:39:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:46.08 -06:19:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:47.91 -05:35:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:51.91 -06:50:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:53.27 -05:16:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:57.51 -06:07:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:59.77 -05:12:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:08.87 -06:37:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:30.03 -05:33:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:42.76 -05:26:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:44.62 -05:29:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:14.05 -04:59:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:19.91 -05:59:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:23.12 -05:37:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:30.38 -05:02:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:30.44 -05:57:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:32.99 -04:52:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:36.47 -05:21:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:41.54 -05:19:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:58.38 -05:27:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:05.95 -05:03:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:40.59 -05:12:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:55.22 -05:38:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:07.97 -05:02:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:16.87 -05:57:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:28.09 -05:02:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:44.77 -05:09:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:43.79 -05:06:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:07:32.82 -08:34:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:28.79 -05:30:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:38.53 -07:47:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:19.44 -10:24:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:52.04 -08:40:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:47.76 -07:57:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
03:45:20.32 -12:52:19.7 -- not a known variable star
03:45:21.20 -12:52:15.0 -- not a known variable star
03:45:24.39 -13:46:57.7 -- not a known variable star
03:45:29.41 -12:19:17.7 -- not a known variable star
03:45:42.04 -10:21:56.1 -- not a known variable star
03:45:57.50 -13:00:00.6 -- not a known variable star
03:45:58.17 -13:42:45.1 -- a known variable star
03:45:58.57 -13:00:19.2 -- not a known variable star
03:46:17.90 -09:16:18.0 -- not a known variable star
03:46:35.21 -12:25:42.8 -- not a known variable star
03:46:36.75 -14:18:13.1 -- not a known variable star
03:46:38.86 -10:32:48.7 -- not a known variable star
03:46:40.94 -12:35:00.2 -- not a known variable star
03:46:42.80 -12:29:04.6 -- not a known variable star
03:46:46.49 -13:48:31.4 -- not a known variable star
03:46:46.74 -12:06:13.6 -- not a known variable star
03:46:47.29 -14:12:46.3 -- not a known variable star
03:46:47.65 -10:56:48.2 -- a known variable star
03:46:47.74 -12:06:34.6 -- not a known variable star
03:46:50.24 -09:23:17.5 -- not a known variable star
03:47:15.12 -11:04:31.1 -- not a known variable star
03:47:17.61 -08:57:18.8 -- not a known variable star
03:47:21.53 -10:48:12.4 -- not a known variable star
03:47:24.78 -10:47:34.8 -- not a known variable star
03:47:30.11 -09:29:34.2 -- not a known variable star
03:47:33.56 -09:33:17.3 -- not a known variable star
03:47:52.61 -07:39:54.1 -- not a known variable star
03:48:00.50 -12:21:47.2 -- not a known variable star
03:48:04.92 -10:12:38.2 -- not a known variable star
03:48:05.25 -05:33:39.4 -- not a known variable star
03:48:11.53 -13:54:28.0 -- not a known variable star
03:48:21.63 -13:50:06.3 -- not a known variable star
03:48:22.35 -13:59:10.0 -- a known variable star
03:48:24.18 -07:39:24.9 -- not a known variable star
03:48:28.71 -08:05:35.8 -- not a known variable star
03:48:29.20 -11:38:15.8 -- not a known variable star
03:48:29.45 -13:38:59.4 -- not a known variable star
03:48:30.58 -13:35:22.9 -- not a known variable star
03:48:35.63 -05:20:32.1 -- a known variable star
03:48:35.69 -11:10:40.2 -- not a known variable star
03:48:37.69 -06:41:51.0 -- a known variable star
03:48:38.60 -14:03:40.0 -- not a known variable star
03:48:41.59 -12:05:57.5 -- not a known variable star
03:48:47.37 -07:04:15.4 -- not a known variable star
03:48:47.95 -10:42:27.6 -- not a known variable star
03:48:54.77 -07:15:38.7 -- not a known variable star
03:49:05.67 -10:23:58.4 -- a known variable star
03:49:06.17 -08:19:44.2 -- not a known variable star
03:49:09.21 -04:53:26.6 -- not a known variable star
03:49:10.33 -12:53:58.7 -- not a known variable star
03:49:10.95 -09:54:26.1 -- not a known variable star
03:49:12.64 -14:15:07.9 -- not a known variable star
03:49:13.07 -06:44:31.1 -- not a known variable star
03:49:13.92 -11:31:15.1 -- not a known variable star
03:49:16.30 -12:08:49.6 -- not a known variable star
03:49:23.79 -13:34:19.4 -- not a known variable star
03:49:29.23 -08:49:23.1 -- not a known variable star
03:49:30.50 -05:57:56.4 -- not a known variable star
03:49:31.78 -06:21:59.4 -- not a known variable star
03:49:32.40 -06:18:35.8 -- not a known variable star
03:49:41.50 -11:33:32.2 -- not a known variable star
03:49:45.41 -09:22:03.7 -- not a known variable star
03:49:45.92 -12:28:55.9 -- not a known variable star
03:49:47.68 -12:16:26.3 -- a known variable star
03:49:49.13 -05:52:27.9 -- a known variable star
03:49:52.35 -06:40:42.8 -- not a known variable star
03:49:55.70 -05:29:45.7 -- not a known variable star
03:49:58.65 -11:44:51.0 -- not a known variable star
03:50:00.70 -10:34:43.1 -- not a known variable star
03:50:07.04 -05:18:05.7 -- not a known variable star
03:50:07.49 -05:30:36.3 -- not a known variable star
03:50:08.56 -11:25:14.2 -- not a known variable star
03:50:11.46 -05:40:10.7 -- not a known variable star
03:50:20.84 -12:37:48.3 -- not a known variable star
03:50:22.16 -05:07:34.8 -- not a known variable star
03:50:22.18 -10:38:01.2 -- not a known variable star
03:50:23.30 -05:41:52.9 -- not a known variable star
03:50:24.95 -05:44:42.6 -- not a known variable star
03:50:27.79 -07:27:33.2 -- not a known variable star
03:50:31.72 -10:23:04.2 -- not a known variable star
03:50:39.84 -04:53:12.3 -- not a known variable star
03:50:41.76 -07:03:58.4 -- not a known variable star
03:50:42.21 -05:24:56.6 -- not a known variable star
03:50:43.83 -06:06:51.7 -- not a known variable star
03:50:44.24 -05:12:59.0 -- a known variable star
03:50:44.63 -10:26:14.9 -- not a known variable star
03:50:48.88 -11:10:50.2 -- not a known variable star
03:50:52.66 -04:59:02.1 -- not a known variable star
03:50:56.66 -11:54:48.6 -- a known variable star
03:51:00.45 -10:28:37.6 -- not a known variable star
03:51:01.28 -06:03:40.1 -- not a known variable star
03:51:01.64 -13:39:45.3 -- not a known variable star
03:51:03.18 -07:59:49.9 -- not a known variable star
03:51:05.65 -05:43:06.9 -- not a known variable star
03:51:06.92 -07:35:27.9 -- not a known variable star
03:51:07.41 -09:49:54.7 -- not a known variable star
03:51:08.68 -05:53:04.4 -- not a known variable star
03:51:10.25 -11:50:47.4 -- not a known variable star
03:51:12.34 -07:41:37.3 -- not a known variable star
03:51:12.61 -07:26:09.0 -- a known variable star
03:51:13.85 -11:05:04.6 -- not a known variable star
03:51:14.16 -06:52:12.2 -- not a known variable star
03:51:14.76 -10:24:29.6 -- not a known variable star
03:51:14.97 -06:55:24.5 -- not a known variable star
03:51:16.97 -06:20:49.9 -- not a known variable star
03:51:17.37 -13:32:08.3 -- not a known variable star
03:51:19.53 -07:01:56.8 -- not a known variable star
03:51:20.43 -14:16:46.7 -- not a known variable star
03:51:25.28 -08:54:10.4 -- not a known variable star
03:51:31.61 -07:38:15.7 -- a known variable star
03:51:34.57 -13:32:15.7 -- not a known variable star
03:51:42.07 -05:02:28.9 -- not a known variable star
03:51:47.94 -06:46:27.0 -- not a known variable star
03:51:48.95 -06:40:42.4 -- not a known variable star
03:51:50.60 -10:33:01.9 -- not a known variable star
03:51:54.10 -12:51:39.5 -- not a known variable star
03:51:56.87 -05:44:37.7 -- not a known variable star
03:51:58.89 -05:21:18.0 -- a known variable star
03:51:59.07 -09:28:04.2 -- not a known variable star
03:52:02.44 -07:25:59.2 -- not a known variable star
03:52:04.14 -05:16:08.8 -- not a known variable star
03:52:05.12 -08:40:27.9 -- not a known variable star
03:52:06.88 -04:52:12.9 -- not a known variable star
03:52:07.70 -06:14:37.1 -- not a known variable star
03:52:10.18 -06:23:21.0 -- not a known variable star
03:52:19.44 -14:23:31.9 -- not a known variable star
03:52:21.39 -06:29:02.3 -- not a known variable star
03:52:27.23 -06:36:05.1 -- not a known variable star
03:52:39.44 -06:27:58.6 -- not a known variable star
03:52:39.60 -08:27:33.9 -- not a known variable star
03:52:48.28 -08:47:49.8 -- not a known variable star
03:52:49.64 -09:19:03.8 -- not a known variable star
03:52:51.64 -04:58:03.3 -- not a known variable star
03:52:53.79 -06:32:50.3 -- not a known variable star
03:52:54.55 -10:44:44.4 -- not a known variable star
03:52:55.77 -09:10:07.5 -- a known variable star
03:52:56.16 -13:11:42.3 -- not a known variable star
03:52:58.61 -05:51:53.9 -- not a known variable star
03:53:09.15 -05:20:16.3 -- not a known variable star
03:53:09.70 -05:59:11.9 -- a known variable star
03:53:10.14 -07:27:50.1 -- not a known variable star
03:53:11.71 -05:59:11.3 -- a known variable star
03:53:12.75 -06:57:12.8 -- not a known variable star
03:53:12.76 -06:55:24.3 -- not a known variable star
03:53:13.71 -05:17:15.6 -- not a known variable star
03:53:16.85 -07:58:02.8 -- not a known variable star
03:53:18.55 -05:36:01.7 -- not a known variable star
03:53:23.28 -08:03:23.7 -- not a known variable star
03:53:25.75 -06:06:09.0 -- not a known variable star
03:53:28.67 -05:39:12.4 -- not a known variable star
03:53:35.11 -05:57:30.5 -- a known variable star
03:53:35.22 -07:11:51.7 -- not a known variable star
03:53:36.18 -05:19:55.9 -- a known variable star
03:53:38.64 -06:06:30.3 -- not a known variable star
03:53:53.55 -05:56:24.4 -- not a known variable star
03:53:53.64 -08:40:06.7 -- not a known variable star
03:53:57.80 -05:02:32.7 -- not a known variable star
03:54:00.28 -06:14:11.3 -- not a known variable star
03:54:00.85 -05:50:16.1 -- not a known variable star
03:54:06.99 -07:37:21.1 -- a known variable star
03:54:16.16 -05:34:06.2 -- a known variable star
03:54:22.86 -07:06:03.4 -- not a known variable star
03:54:29.15 -06:23:45.2 -- not a known variable star
03:54:31.19 -08:43:08.0 -- not a known variable star
03:54:37.54 -13:32:56.3 -- not a known variable star
03:54:40.31 -05:39:20.5 -- not a known variable star
03:54:46.08 -06:19:35.2 -- not a known variable star
03:54:47.91 -05:35:42.9 -- not a known variable star
03:54:51.91 -06:50:12.3 -- not a known variable star
03:54:53.27 -05:16:25.5 -- not a known variable star
03:54:57.51 -06:07:57.3 -- not a known variable star
03:54:59.77 -05:12:33.3 -- not a known variable star
03:55:08.87 -06:37:09.2 -- not a known variable star
03:55:30.03 -05:33:14.0 -- not a known variable star
03:55:42.76 -05:26:22.7 -- a known variable star
03:55:44.62 -05:29:04.3 -- not a known variable star
03:56:14.05 -04:59:47.0 -- not a known variable star
03:56:19.91 -05:59:00.8 -- not a known variable star
03:56:23.12 -05:37:39.4 -- not a known variable star
03:56:30.38 -05:02:09.5 -- not a known variable star
03:56:30.44 -05:57:19.0 -- not a known variable star
03:56:32.99 -04:52:02.6 -- not a known variable star
03:56:36.47 -05:21:11.7 -- not a known variable star
03:56:41.54 -05:19:18.0 -- not a known variable star
03:56:58.38 -05:27:12.1 -- not a known variable star
03:57:05.95 -05:03:13.2 -- not a known variable star
03:57:40.59 -05:12:07.6 -- not a known variable star
03:57:55.22 -05:38:11.8 -- not a known variable star
03:58:07.97 -05:02:51.9 -- not a known variable star
03:58:16.87 -05:57:10.0 -- not a known variable star
03:58:28.09 -05:02:42.7 -- not a known variable star
03:58:44.77 -05:09:21.5 -- not a known variable star
04:00:43.79 -05:06:38.2 -- a known variable star
04:07:32.82 -08:34:19.4 -- not a known variable star
04:12:28.79 -05:30:31.5 -- a known variable star
04:12:38.53 -07:47:54.1 -- a known variable star
04:20:19.44 -10:24:25.3 -- a known variable star
04:26:52.04 -08:40:15.7 -- not a known variable star
04:41:47.76 -07:57:19.9 -- a known variable star
Found 173 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
199 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)2461093.64714064 -observatory 500
23:23:23.55 -01:59:28.7 Mercury (-0.1mag)
23:04:22.11 -07:30:26.0 Venus (-3.9mag)
21:42:44.90 -14:53:09.7 Mars (1.1mag)
07:06:06.31 +22:54:19.5 Jupiter (-2.5mag)
00:05:25.65 -01:44:31.5 Saturn (1.0mag)
03:39:59.41 +19:21:43.4 Uranus (5.7mag)
00:03:40.74 -01:01:38.4 Neptune (7.8mag)
20:29:06.89 -22:59:34.5 Pluto (14.5mag)
01:53:08.87 +16:08:18.7 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 22 02:38 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461093.64714064:
07:06:10.17 +22:54:14.5 Io (5.4mag)
07:06:17.71 +22:53:58.6 Europa (5.5mag)
07:05:56.89 +22:54:45.4 Ganymede (4.9mag)
07:06:25.21 +22:53:54.3 Callisto (6.2mag)
07:09:15.21 +23:10:42.8 Himalia (15.0mag)
07:06:07.36 +22:54:19.9 Thebe (15.9mag)
07:08:40.30 +23:19:10.9 Elara (17.0mag)
07:01:39.82 +24:02:18.2 Pasiphae (17.0mag)
07:15:07.21 +22:42:19.2 Carme (18.1mag)
00:05:37.34 -01:44:36.2 Titan (8.8mag)
00:05:31.10 -01:44:30.2 Rhea (10.1mag)
00:05:21.02 -01:45:52.5 Iapetus (11.5mag)
00:05:26.45 -01:44:34.6 Hyperion (14.8mag)
00:07:29.93 -01:31:31.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 22 02:38 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.64714064:
08:45:43.52 +24:30:42.5 JWST
11:27:36.30 +47:48:29.1 Chandra
15:18:44.20 -60:07:53.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 22 02:38 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)2461093.64714064 at 500
16:59:40.77 -11:03:48.9 17.5mag 10P/Tempel 2
03:37:18.32 +28:57:47.8 18.0mag 123P/West-Hartley
08:23:39.45 +60:43:02.2 18.4mag 124P/Mrkos
21:19:33.15 -07:38:54.5 22.1mag 141P/Machholz
01:21:07.97 +11:54:43.5 17.7mag 145P/Shoemaker-Levy 5
11:02:59.45 +30:34:29.3 17.9mag 164P/Christensen
09:33:08.21 -33:51:49.2 18.0mag 195P/Hill
15:52:03.28 -06:35:55.6 19.2mag 210P/Christensen
18:16:49.40 -21:28:32.3 17.3mag 218P/LINEAR
16:21:33.40 -18:10:56.9 15.2mag 235P/LINEAR
03:56:22.73 +27:44:25.9 17.8mag 240P/NEAT
15:17:37.29 +06:38:27.0 14.8mag 24P/Schaumasse
11:23:31.25 -03:23:10.3 17.4mag 29P/Schwassmann-Wachmann 1
07:03:47.92 +27:24:49.8 19.6mag 407P/PanSTARRS-Fuls
17:07:08.03 -11:19:14.4 17.6mag 40P/Vaisala 1
11:02:13.14 -08:51:54.4 16.6mag 43P/Wolf-Harrington
13:25:29.72 -05:49:37.8 20.0mag 489P/Denning
04:34:21.79 +48:34:36.0 17.8mag 493P/2024 Q2 (LONEOS)
06:04:23.01 +47:31:32.3 17.7mag 63P/Wild 1
23:14:35.68 -02:07:35.5 16.2mag 78P/Gehrels 2
20:01:28.71 -22:18:21.7 15.0mag 88P/Howell
15:27:54.46 -29:00:38.9 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.07 -72:35:55.7 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:50.05 +31:12:54.1 18.2mag C/2017 K2 (PanSTARRS)
20:06:38.03 -65:11:37.4 18.1mag C/2020 V2 (ZTF)
17:21:40.25 +04:21:20.6 16.3mag C/2021 G2 (ATLAS)
03:35:40.70 +24:36:41.8 15.8mag C/2022 N2 (PanSTARRS)
09:08:13.38 +29:49:32.7 15.3mag C/2022 QE78 (ATLAS)
08:35:40.67 -06:33:49.7 16.7mag C/2022 R6 (PanSTARRS)
23:53:01.70 +48:26:44.6 18.0mag C/2023 C2 (ATLAS)
09:51:08.23 -20:46:02.4 17.5mag C/2023 F3 (ATLAS)
20:34:44.57 +61:14:30.9 17.3mag C/2023 H5 (Lemmon)
19:34:30.09 -03:24:15.7 16.1mag C/2023 R1 (PANSTARRS)
02:48:55.16 +35:40:34.4 18.5mag C/2023 RS61 (PanSTARRS)
21:01:26.48 +81:19:56.1 18.0mag C/2023 X2 (Lemmon)
06:39:10.25 +63:49:12.9 17.3mag C/2024 A1 (ATLAS)
01:56:42.80 -24:38:17.4 11.2mag C/2024 E1 (Wierzchos)
11:44:58.96 -02:34:54.8 18.1mag C/2024 G2 (ATLAS)
19:28:18.67 +00:39:11.9 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.74 -01:42:55.4 17.7mag C/2024 G6 (ATLAS)
19:53:27.37 +03:15:03.3 15.6mag C/2024 J3 (ATLAS)
02:47:14.43 -31:34:32.5 15.4mag C/2024 T5 (ATLAS)
16:25:06.92 -58:13:41.4 15.6mag C/2025 A6 (Lemmon)
04:50:29.55 +62:14:38.2 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)
15:56:43.66 -13:01:32.0 14.8mag C/2025 L1 (ATLAS)
02:20:13.81 -19:05:55.5 16.7mag C/2025 Q3 (ATLAS)
02:09:34.11 +17:16:42.3 21.2mag C/2025 R2 (SWAN)
22:20:45.75 +17:39:14.2 16.4mag C/2025 R3 (PANSTARRS)
21:46:00.92 -16:50:21.3 21.5mag C/2025 T1 (ATLAS)
03:06:15.13 -20:34:10.6 18.3mag C/2026 A1 (MAPS)
21:03:00.83 +20:55:29.6 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 22 02:39 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
-rw-r--r-- 1 apache apache 6.2K Feb 22 02:38 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
-rw-r--r-- 1 apache apache 187K Feb 22 02:38 tocp_transients_list.txt