This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386
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 22.1410 2461093.6410 11.33 02:05:34.62 -05:59:47.7
166.10350 -62.47933 galactic Cet Second-epoch detections are separated by 2.3" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2490715340984556928 | 02:05:34.24 -05:59:51.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1951TOYal..23.....B BD-06 401
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 05 34.62 -05 59 47.7 11.3 U Cet 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 2490715340984556928,2461093.6410,11.33,0.05,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 2490715340984556928 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:34.62 -05:59:47.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.68 02:07:59.19 -02:17:33.2
162.61188 -59.13423 galactic Cet Second-epoch detections are separated by 5.0" 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 | ATO J032.0085-02.2891 | 02:07:59.92 -02:17:33.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0p 1945AJ.....51..187G BD-02 366
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 07 59.19 -02 17 33.2 10.7 U Cet 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 J032.0085-02.2891,2461093.6410,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J032.0085-02.2891 20260222.1410 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:59.19 -02:17:33.2 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.28 02:15:16.47 +02:22:34.2
160.63598 -54.24107 galactic Cet Second-epoch detections are separated by 0.5" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2513946617225734784 | 02:15:17.04 +02:22:28.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1949TOYal..20.....B BD+01 398
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 15 16.47 +02 22 34.2 10.3 U Cet 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 2513946617225734784,2461093.6410,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2513946617225734784 20260222.1410 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:15:16.47 +02:22:34.2 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.39 02:06:39.03 +03:06:12.1
156.81855 -54.74285 galactic Cet Second-epoch detections are separated by 0.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2517654823269588480 | 02:06:39.62 +03:06:06.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1949TOYal..20.....B BD+02 332
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 06 39.03 +03 06 12.1 10.4 U Cet 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 2517654823269588480,2461093.6410,10.39,0.05,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 2517654823269588480 20260222.1410 10.39CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:39.03 +03:06:12.1 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.41 02:14:46.59 +02:13:55.3
160.59162 -54.42971 galactic Cet Second-epoch detections are separated by 2.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2513567972908911744 | 02:14:46.51 +02:13:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1949TOYal..20.....B BD+01 396
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 14 46.59 +02 13 55.3 10.4 U Cet 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 2513567972908911744,2461093.6410,10.41,0.05,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 2513567972908911744 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:14:46.59 +02:13:55.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_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 22.1410* 02 13 13.49 +01 07 24.9 10.7 U Cet 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
NSV 754,2461093.6410,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 754 20260222.1410 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:13:13.49 +01:07:24.9 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.68 02:14:51.16 +02:31:17.6
160.34970 -54.17620 galactic Cet Second-epoch detections are separated by 3.1" 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 2514702428390645248 | 02:14:51.67 +02:31:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1958PMcCO..13b....V AG+02 223
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 14 51.16 +02 31 17.6 10.7 U Cet 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 2514702428390645248,2461093.6410,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514702428390645248 20260222.1410 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:14:51.16 +02:31:17.6 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.76 02:05:42.86 +01:53:20.2
157.53305 -55.91088 galactic Cet Second-epoch detections are separated by 6.8" 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 2508416382975736704 | 02:05:43.44 +01:53:16.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949TOYal..20.....B BD+01 367
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 05 42.86 +01 53 20.2 10.8 U Cet 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 2508416382975736704,2461093.6410,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2508416382975736704 20260222.1410 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:42.86 +01:53:20.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.90 02:08:20.95 +03:03:22.5
157.49368 -54.57104 galactic Cet Second-epoch detections are separated by 1.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514643913756089856 | 02:08:20.23 +03:03:32.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3:V 1986AJ.....92..139S StKM 2- 188
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 08 20.95 +03 03 22.5 10.9 U Cet 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 2514643913756089856,2461093.6410,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514643913756089856 20260222.1410 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:08:20.95 +03:03:22.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2517561674019047296,2461093.6410,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2517561674019047296 20260222.1410 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:17.62 +02:57:27.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_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 22.1410* 02 17 51.12 +02 22 28.9 11.0 U Cet 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 J021752+0222.4,2461093.6410,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J021752+0222.4 20260222.1410 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:17:51.12 +02:22:28.9 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.35 02:06:48.57 +02:51:54.0
157.08466 -54.92968 galactic Cet Second-epoch detections are separated by 0.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514552035815705088 | 02:06:49.26 +02:51:46.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1958PMcCO..13b....V AG+02 214
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 06 48.57 +02 51 54.0 11.3 U Cet 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 2514552035815705088,2461093.6410,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514552035815705088 20260222.1410 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:48.57 +02:51:54.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.29 02:08:35.45 -06:11:42.5
167.63330 -62.16965 galactic Cet Second-epoch detections are separated by 4.0" 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 2487666193377847936 | 02:08:36.26 -06:11:36.6 (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 22.1410* 02 08 35.45 -06 11 42.5 13.3 U Cet 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 2487666193377847936,2461093.6410,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2487666193377847936 20260222.1410 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:08:35.45 -06:11:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.04 02:04:58.17 -03:28:45.4
162.72519 -60.53869 galactic Cet Second-epoch detections are separated by 8.9" 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 2492418557511019520 | 02:04:58.56 -03:28:47.2 (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 22.1410* 02 04 58.17 -03 28 45.4 13.0 U Cet 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 2492418557511019520,2461093.6410,13.04,0.05,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 2492418557511019520 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:04:58.17 -03:28:45.4 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.07 02:05:33.28 -05:40:38.6
165.67463 -62.22969 galactic Cet Second-epoch detections are separated by 8.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2490759772421788160 | 02:05:33.29 -05:40:31.1 (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 22.1410* 02 05 33.28 -05 40 38.6 13.1 U Cet 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 2490759772421788160,2461093.6410,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2490759772421788160 20260222.1410 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:33.28 -05:40:38.6 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.88 02:04:01.36 -05:50:56.0
165.24312 -62.59670 galactic Cet Second-epoch detections are separated by 4.5" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2490915387676914816 | 02:04:00.98 -05:51:01.4 (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 22.1410* 02 04 01.36 -05 50 56.0 12.9 U Cet 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 2490915387676914816,2461093.6410,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2490915387676914816 20260222.1410 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:04:01.36 -05:50:56.0 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.05 02:09:34.78 -05:13:27.2
166.75968 -61.25760 galactic Cet Second-epoch detections are separated by 3.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2491162601699088000 | 02:09:35.30 -05:13:32.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 09 34.78 -05 13 27.2 13.1 U Cet 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 2491162601699088000,2461093.6410,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2491162601699088000 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:09:34.78 -05:13:27.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.61 02:03:18.43 -02:52:48.5
161.34816 -60.27648 galactic Cet Second-epoch detections are separated by 7.3" 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 2492711882302183936 | 02:03:17.96 -02:52:55.9 (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 22.1410* 02 03 18.43 -02 52 48.5 12.6 U Cet 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 2492711882302183936,2461093.6410,12.61,0.05,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 2492711882302183936 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:18.43 -02:52:48.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.69 02:02:54.01 -04:34:01.4
163.14176 -61.72576 galactic Cet Second-epoch detections are separated by 4.1" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2492198169854213888 | 02:02:54.65 -04:33:60.0 (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 22.1410* 02 02 54.01 -04 34 01.4 12.7 U Cet 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 2492198169854213888,2461093.6410,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2492198169854213888 20260222.1410 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:02:54.01 -04:34:01.4 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.61 02:03:34.39 -02:32:25.0
161.08279 -59.95642 galactic Cet Second-epoch detections are separated by 6.1" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2492738648538366336 | 02:03:34.61 -02:32:33.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 03 34.39 -02 32 25.0 12.6 U Cet 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 2492738648538366336,2461093.6410,12.61,0.05,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 2492738648538366336 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:34.39 -02:32:25.0 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.44 02:03:15.23 -06:08:28.4
165.29481 -62.94518 galactic Cet Second-epoch detections are separated by 2.6" 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 2490628071544668544 | 02:03:14.86 -06:08:33.9 (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 22.1410* 02 03 15.23 -06 08 28.4 12.4 U Cet 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 2490628071544668544,2461093.6410,12.44,0.05,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 2490628071544668544 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:15.23 -06:08:28.4 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.56 02:06:23.81 -05:41:01.4
166.03879 -62.10710 galactic Cet Second-epoch detections are separated by 3.7" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2490757332880384384 | 02:06:23.36 -05:41:06.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 06 23.81 -05 41 01.4 12.6 U Cet 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 2490757332880384384,2461093.6410,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2490757332880384384 20260222.1410 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:23.81 -05:41:01.4 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.54 02:03:51.42 -04:53:20.5
163.94800 -61.84916 galactic Cet Second-epoch detections are separated by 0.8" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2491051589679761664 | 02:03:50.71 -04:53:23.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 03 51.42 -04 53 20.5 12.5 U Cet 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 2491051589679761664,2461093.6410,12.54,0.05,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 2491051589679761664 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:51.42 -04:53:20.5 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.50 02:07:37.04 -02:04:47.5
162.22960 -59.01117 galactic Cet Second-epoch detections are separated by 3.6" 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 2494267970428658432 | 02:07:37.35 -02:04:41.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 07 37.04 -02 04 47.5 12.5 U Cet 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 2494267970428658432,2461093.6410,12.50,0.05,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 2494267970428658432 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:37.04 -02:04:47.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.38 02:05:07.73 -03:19:24.8
162.61143 -60.38807 galactic Cet Second-epoch detections are separated by 6.5" 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 2492425498178166272 | 02:05:08.01 -03:19:35.4 (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 22.1410* 02 05 07.73 -03 19 24.8 12.4 U Cet 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 2492425498178166272,2461093.6410,12.38,0.05,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 2492425498178166272 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:07.73 -03:19:24.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.43 02:16:21.28 -06:27:26.4
171.08305 -61.11742 galactic Cet Second-epoch detections are separated by 1.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.0818-06.4591 | 02:16:22.02 -06:27:41.4 (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 22.1410* 02 16 21.28 -06 27 26.4 12.4 U Cet 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 J034.0818-06.4591,2461093.6410,12.43,0.05,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 J034.0818-06.4591 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:16:21.28 -06:27:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.20 02:06:38.21 -05:35:47.1
166.02580 -62.00151 galactic Cet Second-epoch detections are separated by 3.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2490764204828234240 | 02:06:37.74 -05:35:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 06 38.21 -05 35 47.1 12.2 U Cet 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 2490764204828234240,2461093.6410,12.20,0.05,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 2490764204828234240 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:38.21 -05:35:47.1 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.02 02:04:57.05 -05:23:32.7
165.04987 -62.09306 galactic Cet Second-epoch detections are separated by 3.3" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2490968404753355648 | 02:04:56.31 -05:23:37.1 (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 22.1410* 02 04 57.05 -05 23 32.7 12.0 U Cet 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 2490968404753355648,2461093.6410,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2490968404753355648 20260222.1410 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:04:57.05 -05:23:32.7 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.22 02:09:52.95 -04:14:07.4
165.63978 -60.42944 galactic Cet Second-epoch detections are separated by 4.2" 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 2491530117756005248 | 02:09:52.57 -04:14:09.9 (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 22.1410* 02 09 52.95 -04 14 07.4 12.2 U Cet 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 2491530117756005248,2461093.6410,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2491530117756005248 20260222.1410 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:09:52.95 -04:14:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.07 02:03:57.98 -03:39:57.3
162.52205 -60.83465 galactic Cet Second-epoch detections are separated by 0.6" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2492318639391975808 | 02:03:57.52 -03:39:59.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 03 57.98 -03 39 57.3 12.1 U Cet 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 2492318639391975808,2461093.6410,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2492318639391975808 20260222.1410 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:57.98 -03:39:57.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.91 02:06:18.17 -01:42:37.2
161.30129 -58.88801 galactic Cet Second-epoch detections are separated by 5.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2506395407589094400 | 02:06:17.77 -01:42:39.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 06 18.17 -01 42 37.2 11.9 U Cet 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 2506395407589094400,2461093.6410,11.91,0.05,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 2506395407589094400 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:18.17 -01:42:37.2 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.98 02:13:23.91 +02:07:14.7
160.19645 -54.70973 galactic Cet Second-epoch detections are separated by 3.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514288049946194432 | 02:13:23.64 +02:07:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 13 23.91 +02 07 14.7 12.0 U Cet 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 2514288049946194432,2461093.6410,11.98,0.05,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 2514288049946194432 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:13:23.91 +02:07:14.7 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.82 02:02:51.98 -04:20:39.0
162.85763 -61.54819 galactic Cet Second-epoch detections are separated by 1.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2492252668694325120 | 02:02:51.37 -04:20:43.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 02 51.98 -04 20 39.0 11.8 U Cet 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 2492252668694325120,2461093.6410,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2492252668694325120 20260222.1410 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:02:51.98 -04:20:39.0 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.66 02:07:05.30 -01:17:37.8
161.17413 -58.43234 galactic Cet Second-epoch detections are separated by 6.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2506447806190228096 | 02:07:05.65 -01:17:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG-01 196
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 07 05.30 -01 17 37.8 11.7 U Cet 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 2506447806190228096,2461093.6410,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2506447806190228096 20260222.1410 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:05.30 -01:17:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.62 02:03:49.71 -03:58:42.0
162.83103 -61.11089 galactic Cet Second-epoch detections are separated by 4.2" 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 2492292044954505216 | 02:03:48.96 -03:58:45.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1945AJ.....51..187G BD-04 325
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 03 49.71 -03 58 42.0 11.6 U Cet 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 2492292044954505216,2461093.6410,11.62,0.05,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 2492292044954505216 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:49.71 -03:58:42.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.51 02:06:50.99 -03:24:13.3
163.41407 -60.20714 galactic Cet Second-epoch detections are separated by 0.7" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2492429861865007360 | 02:06:50.41 -03:24:15.6 (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 22.1410* 02 06 50.99 -03 24 13.3 11.5 U Cet 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 2492429861865007360,2461093.6410,11.51,0.05,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 2492429861865007360 20260222.1410 11.51CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:50.99 -03:24:13.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.36 02:05:43.55 -04:20:49.3
164.07188 -61.13703 galactic Cet Second-epoch detections are separated by 0.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2492217411307171584 | 02:05:42.97 -04:20:51.3 (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 22.1410* 02 05 43.55 -04 20 49.3 11.4 U Cet 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 2492217411307171584,2461093.6410,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2492217411307171584 20260222.1410 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:43.55 -04:20:49.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.42 02:08:53.52 -05:46:32.5
167.19758 -61.79596 galactic Cet Second-epoch detections are separated by 4.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2491071724486457088 | 02:08:53.16 -05:46:35.5 (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 22.1410* 02 08 53.52 -05 46 32.5 11.4 U Cet 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 2491071724486457088,2461093.6410,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2491071724486457088 20260222.1410 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:08:53.52 -05:46:32.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.32 02:08:07.10 -04:50:40.1
165.67905 -61.18038 galactic Cet Second-epoch detections are separated by 2.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2491377766676171008 | 02:08:06.60 -04:50:42.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 08 07.10 -04 50 40.1 11.3 U Cet 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 2491377766676171008,2461093.6410,11.32,0.05,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 2491377766676171008 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:08:07.10 -04:50:40.1 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.50 02:06:46.63 +01:08:57.6
158.62333 -56.40986 galactic Cet Second-epoch detections are separated by 2.8" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2508140302477906304 | 02:06:47.21 +01:08:56.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1950TOYal..21.....B BD+00 351
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 06 46.63 +01 08 57.6 10.5 U Cet 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 2508140302477906304,2461093.6410,10.50,0.05,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 2508140302477906304 20260222.1410 10.50CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:46.63 +01:08:57.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.93 02:12:20.10 +00:32:21.8
161.32615 -56.17974 galactic Cet Second-epoch detections are separated by 2.4" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2507096453626315392 | 02:12:20.91 +00:32:18.4 (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 22.1410* 02 12 20.10 +00 32 21.8 10.9 U Cet 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 2507096453626315392,2461093.6410,10.93,0.05,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 2507096453626315392 20260222.1410 10.93CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:12:20.10 +00:32:21.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.88 02:15:36.88 +02:28:03.1
160.67262 -54.11817 galactic Cet Second-epoch detections are separated by 6.4" 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 2513948919328218368 | 02:15:37.48 +02:27:57.7 (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 22.1410* 02 15 36.88 +02 28 03.1 10.9 U Cet 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 2513948919328218368,2461093.6410,10.88,0.05,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 2513948919328218368 20260222.1410 10.88CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:15:36.88 +02:28:03.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.85 02:08:17.92 -01:43:10.5
162.10935 -58.61759 galactic Cet Second-epoch detections are separated by 7.8" 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 2494376237964265088 | 02:08:18.57 -01:43:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 08 17.92 -01 43 10.5 10.8 U Cet 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 2494376237964265088,2461093.6410,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2494376237964265088 20260222.1410 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:08:17.92 -01:43:10.5 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.87 02:05:38.22 -00:56:42.3
160.23127 -58.33778 galactic Cet Second-epoch detections are separated by 5.3" 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 2506518660265805184 | 02:05:38.92 -00:56:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1950TOYal..21.....B BD-01 289
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 05 38.22 +00 56 42.3 10.9 U Cet 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 2506518660265805184,2461093.6410,10.87,0.05,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 2506518660265805184 20260222.1410 10.87CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:38.22 -00:56:42.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.89 02:03:36.50 -01:03:38.3
159.52925 -58.70672 galactic Cet Second-epoch detections are separated by 5.0" 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 2506680391554435200 | 02:03:37.68 -01:03:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG-01 193
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 03 36.50 -01 03 38.3 10.9 U Cet 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 2506680391554435200,2461093.6410,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2506680391554435200 20260222.1410 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:36.50 -01:03:38.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 10.94 02:11:15.84 +02:37:21.0
158.95522 -54.56820 galactic Cet Second-epoch detections are separated by 4.8" 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 2514399886598935168 | 02:11:16.55 +02:37:17.8 (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 22.1410* 02 11 15.84 +02 37 21.0 10.9 U Cet 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 2514399886598935168,2461093.6410,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514399886598935168 20260222.1410 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:11:15.84 +02:37:21.0 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.01 02:07:05.27 +00:21:09.3
159.50607 -57.04731 galactic Cet Second-epoch detections are separated by 3.4" 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 2507219697712642048 | 02:07:06.03 +00:21:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1950TOYal..21.....B BD-00 319
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 07 05.27 +00 21 09.3 11.0 U Cet 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 2507219697712642048,2461093.6410,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2507219697712642048 20260222.1410 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:05.27 +00:21:09.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.24 02:14:34.82 +02:04:49.4
160.66306 -54.58357 galactic Cet Second-epoch detections are separated by 2.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2513557390109500288 | 02:14:35.42 +02:04:43.2 (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 22.1410* 02 14 34.82 +02 04 49.4 11.2 U Cet 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 2513557390109500288,2461093.6410,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2513557390109500288 20260222.1410 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:14:34.82 +02:04:49.4 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.15 02:03:41.23 -02:12:51.2
160.77457 -59.66815 galactic Cet Second-epoch detections are separated by 1.1" 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 2506259858421109760 | 02:03:41.66 -02:12:50.7 (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 22.1410* 02 03 41.23 -02 12 51.2 11.2 U Cet 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 2506259858421109760,2461093.6410,11.15,0.05,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 2506259858421109760 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:41.23 -02:12:51.2 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.20 02:04:09.82 -01:41:01.3
160.40365 -59.15823 galactic Cet Second-epoch detections are separated by 4.9" 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 2506361155225291904 | 02:04:10.17 -01:40:56.9 (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 22.1410* 02 04 09.82 -01 41 01.3 11.2 U Cet 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 2506361155225291904,2461093.6410,11.20,0.05,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 2506361155225291904 20260222.1410 11.20CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:04:09.82 -01:41:01.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.36 02:10:27.38 -00:39:00.6
161.82052 -57.42970 galactic Cet Second-epoch detections are separated by 2.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2506871156822033408 | 02:10:28.09 -00:39:01.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG-00 227
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 10 27.38 +00 39 00.6 11.4 U Cet 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 2506871156822033408,2461093.6410,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2506871156822033408 20260222.1410 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:10:27.38 -00:39:00.6 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.24 02:18:46.79 +02:41:22.7
161.58267 -53.49732 galactic Cet Second-epoch detections are separated by 8.2" 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 2513970840841542144 | 02:18:47.30 +02:41:17.7 (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 22.1410* 02 18 46.79 +02 41 22.7 11.2 U Cet 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 2513970840841542144,2461093.6410,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2513970840841542144 20260222.1410 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:18:46.79 +02:41:22.7 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.46 02:12:44.89 +02:07:41.5
159.95217 -54.79082 galactic Cet Second-epoch detections are separated by 5.4" 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 2514290970523781376 | 02:12:45.56 +02:07:39.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 12 44.89 +02 07 41.5 11.5 U Cet 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 2514290970523781376,2461093.6410,11.46,0.05,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 2514290970523781376 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:12:44.89 +02:07:41.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.47 02:07:03.66 -01:33:37.0
161.44543 -58.65817 galactic Cet Second-epoch detections are separated by 0.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2506404242337223296 | 02:07:04.26 -01:33:35.1 (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 22.1410* 02 07 03.66 -01 33 37.0 11.5 U Cet 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 2506404242337223296,2461093.6410,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2506404242337223296 20260222.1410 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:03.66 -01:33:37.0 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.51 02:12:53.27 +00:05:38.8
161.98031 -56.47269 galactic Cet Second-epoch detections are separated by 5.6" 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 2507018010343637760 | 02:12:53.73 +00:05:43.7 (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 22.1410* 02 12 53.27 +00 05 38.8 11.5 U Cet 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 2507018010343637760,2461093.6410,11.51,0.05,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 2507018010343637760 20260222.1410 11.51CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:12:53.27 +00:05:38.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.65 02:11:32.52 +01:47:52.9
159.81650 -55.23102 galactic Cet Second-epoch detections are separated by 1.7" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514182153232329216 | 02:11:33.17 +01:47:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 11 32.52 +01 47 52.9 11.7 U Cet 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 2514182153232329216,2461093.6410,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514182153232329216 20260222.1410 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:11:32.52 +01:47:52.9 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_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 22.1410* 02 19 48.46 +02 51 38.4 11.5 U Cet 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 J021949+0251.6,2461093.6410,11.51,0.05,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
ASAS J021949+0251.6 20260222.1410 11.51CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:19:48.46 +02:51:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.68 02:09:15.25 +00:53:28.3
159.81870 -56.30307 galactic Cet Second-epoch detections are separated by 3.4" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2507364459585708288 | 02:09:16.21 +00:53:30.3 (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 22.1410* 02 09 15.25 +00 53 28.3 11.7 U Cet 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 2507364459585708288,2461093.6410,11.68,0.05,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 2507364459585708288 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:09:15.25 +00:53:28.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.62 02:05:38.22 +00:31:20.2
158.77439 -57.09365 galactic Cet Second-epoch detections are separated by 3.5" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2507987436001873408 | 02:05:38.31 +00:31:09.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 05 38.22 +00 31 20.2 11.6 U Cet 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 2507987436001873408,2461093.6410,11.62,0.05,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 2507987436001873408 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:38.22 +00:31:20.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.71 02:10:11.82 +01:25:32.7
159.66526 -55.72521 galactic Cet Second-epoch detections are separated by 3.6" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514144151361843968 | 02:10:12.53 +01:25:31.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 10 11.82 +01 25 32.7 11.7 U Cet 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 2514144151361843968,2461093.6410,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514144151361843968 20260222.1410 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:10:11.82 +01:25:32.7 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.71 02:13:19.41 +03:03:40.5
159.30839 -53.92449 galactic Cet Second-epoch detections are separated by 2.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514795676425538048 | 02:13:19.88 +03:03:39.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1958PMcCO..13b....V AG+02 220
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 22.1410* 02 13 19.41 +03 03 40.5 11.7 U Cet 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 2514795676425538048,2461093.6410,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514795676425538048 20260222.1410 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:13:19.41 +03:03:40.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.66 02:03:50.18 -00:32:25.5
159.09659 -58.23482 galactic Cet Second-epoch detections are separated by 1.2" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2506781580983911296 | 02:03:50.94 -00:32:25.1 (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 22.1410* 02 03 50.18 +00 32 25.5 11.7 U Cet 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 2506781580983911296,2461093.6410,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2506781580983911296 20260222.1410 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:50.18 -00:32:25.5 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.70 02:10:06.73 +02:12:27.4
158.90681 -55.07231 galactic Cet Second-epoch detections are separated by 3.8" 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 | Large-amplitude variable Gaia DR2 2514257293684972032 | 02:10:07.49 +02:12:24.7 (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 22.1410* 02 10 06.73 +02 12 27.4 11.7 U Cet 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 2514257293684972032,2461093.6410,11.70,0.05,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
Large-amplitude variable Gaia DR2 2514257293684972032 20260222.1410 11.70CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:10:06.73 +02:12:27.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.87 02:10:29.04 +02:38:39.4
158.64871 -54.65132 galactic Cet Second-epoch detections are separated by 3.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514567841295419136 | 02:10:29.39 +02:38:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 10 29.04 +02 38 39.4 11.9 U Cet 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 2514567841295419136,2461093.6410,11.87,0.05,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 2514567841295419136 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:10:29.04 +02:38:39.4 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.86 02:05:04.89 -00:54:51.7
159.97660 -58.38655 galactic Cet Second-epoch detections are separated by 6.1" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2506499414516827008 | 02:05:05.36 -00:54:50.9 (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 22.1410* 02 05 04.89 +00 54 51.7 11.9 U Cet 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 2506499414516827008,2461093.6410,11.86,0.05,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 2506499414516827008 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:04.89 -00:54:51.7 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.88 02:11:49.95 +01:43:49.0
159.98766 -55.24937 galactic Cet Second-epoch detections are separated by 3.6" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514180675763582208 | 02:11:50.70 +01:43:44.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 11 49.95 +01 43 49.0 11.9 U Cet 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 2514180675763582208,2461093.6410,11.88,0.05,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 2514180675763582208 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:11:49.95 +01:43:49.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.88 02:06:03.96 +02:18:57.9
157.28553 -55.49770 galactic Cet Second-epoch detections are separated by 8.7" 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 2514495892003378560 | 02:06:05.07 +02:18:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 06 03.96 +02 18 57.9 11.9 U Cet 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 2514495892003378560,2461093.6410,11.88,0.05,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 2514495892003378560 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:03.96 +02:18:57.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.90 02:04:37.54 +00:05:58.9
158.78269 -57.58607 galactic Cet Second-epoch detections are separated by 7.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2507193245009263744 | 02:04:37.73 +00:05:40.1 (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 22.1410* 02 04 37.54 +00 05 58.9 11.9 U Cet 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 2507193245009263744,2461093.6410,11.90,0.05,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 2507193245009263744 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:04:37.54 +00:05:58.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.99 02:09:05.56 +03:05:11.2
157.74284 -54.45088 galactic Cet Second-epoch detections are separated by 4.9" 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 2514666797341840640 | 02:09:06.31 +03:05:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 09 05.56 +03 05 11.2 12.0 U Cet 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 2514666797341840640,2461093.6410,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514666797341840640 20260222.1410 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:09:05.56 +03:05:11.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.91 02:04:35.13 +00:50:27.5
158.05836 -56.95659 galactic Cet Second-epoch detections are separated by 6.9" 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 2508057426788892288 | 02:04:35.95 +00:50:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 04 35.13 +00 50 27.5 11.9 U Cet 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 2508057426788892288,2461093.6410,11.91,0.05,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 2508057426788892288 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:04:35.13 +00:50:27.5 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 11.97 02:13:13.77 +02:28:31.8
159.80644 -54.43311 galactic Cet Second-epoch detections are separated by 5.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514341204461445376 | 02:13:14.16 +02:28:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 13 13.77 +02 28 31.8 12.0 U Cet 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 2514341204461445376,2461093.6410,11.97,0.05,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 2514341204461445376 20260222.1410 11.97CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:13:13.77 +02:28:31.8 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.01 02:08:31.20 -00:12:45.2
160.62371 -57.33161 galactic Cet Second-epoch detections are separated by 7.5" 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 2506947435441181312 | 02:08:32.09 -00:12:48.2 (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 22.1410* 02 08 31.20 +00 12 45.2 12.0 U Cet 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 2506947435441181312,2461093.6410,12.01,0.05,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 2506947435441181312 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:08:31.20 -00:12:45.2 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.04 02:09:42.80 +03:04:57.3
157.97520 -54.37513 galactic Cet Second-epoch detections are separated by 2.1" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514664563958880512 | 02:09:42.31 +03:05:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 09 42.80 +03 04 57.3 12.0 U Cet 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 2514664563958880512,2461093.6410,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514664563958880512 20260222.1410 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:09:42.80 +03:04:57.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.03 02:09:49.97 +01:26:58.4
159.50584 -55.75341 galactic Cet Second-epoch detections are separated by 5.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514147862213588224 | 02:09:50.57 +01:26:56.9 (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 22.1410* 02 09 49.97 +01 26 58.4 12.0 U Cet 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 2514147862213588224,2461093.6410,12.03,0.05,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 2514147862213588224 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:09:49.97 +01:26:58.4 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.12 02:08:44.02 +01:58:36.3
158.60220 -55.44885 galactic Cet Second-epoch detections are separated by 7.8" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514257847735339776 | 02:08:44.59 +01:58:37.7 (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 22.1410* 02 08 44.02 +01 58 36.3 12.1 U Cet 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 2514257847735339776,2461093.6410,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514257847735339776 20260222.1410 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:08:44.02 +01:58:36.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.16 02:14:12.01 +02:43:00.8
159.93573 -54.09944 galactic Cet Second-epoch detections are separated by 4.7" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514721910362246272 | 02:14:12.20 +02:42:54.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 14 12.01 +02 43 00.8 12.2 U Cet 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 2514721910362246272,2461093.6410,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514721910362246272 20260222.1410 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:14:12.01 +02:43:00.8 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.06 02:04:40.32 +01:07:20.2
157.82976 -56.70369 galactic Cet Second-epoch detections are separated by 7.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2508171496824867072 | 02:04:40.98 +01:07:16.8 (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 22.1410* 02 04 40.32 +01 07 20.2 12.1 U Cet 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 2508171496824867072,2461093.6410,12.06,0.05,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 2508171496824867072 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:04:40.32 +01:07:20.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.25 02:09:01.05 +02:47:46.4
157.97048 -54.71006 galactic Cet Second-epoch detections are separated by 3.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514587804303345280 | 02:09:00.48 +02:47:52.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 09 01.05 +02 47 46.4 12.2 U Cet 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 2514587804303345280,2461093.6410,12.25,0.05,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 2514587804303345280 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:09:01.05 +02:47:46.4 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.26 02:06:37.73 +02:56:03.0
156.95659 -54.89228 galactic Cet Second-epoch detections are separated by 1.4" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514556296423238528 | 02:06:38.53 +02:55:55.3 (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 22.1410* 02 06 37.73 +02 56 03.0 12.3 U Cet 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 2514556296423238528,2461093.6410,12.26,0.05,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 2514556296423238528 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:37.73 +02:56:03.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.38 02:20:37.10 +02:50:46.8
162.07273 -53.11059 galactic Cet Second-epoch detections are separated by 4.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514026744135661696 | 02:20:37.68 +02:50:41.7 (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 22.1410* 02 20 37.10 +02 50 46.8 12.4 U Cet 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 2514026744135661696,2461093.6410,12.38,0.05,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 2514026744135661696 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:20:37.10 +02:50:46.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.27 02:10:14.98 +02:23:35.9
158.78876 -54.89604 galactic Cet Second-epoch detections are separated by 2.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514366905545502464 | 02:10:15.39 +02:23:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 10 14.98 +02 23 35.9 12.3 U Cet 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 2514366905545502464,2461093.6410,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514366905545502464 20260222.1410 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:10:14.98 +02:23:35.9 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.33 02:08:36.83 -05:08:56.7
166.26882 -61.34656 galactic Cet Second-epoch detections are separated by 1.2" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2491177960502137600 | 02:08:36.92 -05:09:18.1 (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 22.1410* 02 08 36.83 -05 08 56.7 12.3 U Cet 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 2491177960502137600,2461093.6410,12.33,0.05,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 2491177960502137600 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:08:36.83 -05:08:56.7 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.32 02:03:48.78 -02:03:44.5
160.66287 -59.52374 galactic Cet Second-epoch detections are separated by 4.5" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2506279722645372544 | 02:03:48.91 -02:03:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 03 48.78 -02 03 44.5 12.3 U Cet 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 2506279722645372544,2461093.6410,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2506279722645372544 20260222.1410 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:48.78 -02:03:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.51 02:07:43.23 +00:38:52.4
159.46503 -56.71306 galactic Cet Second-epoch detections are separated by 2.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2507330409084786944 | 02:07:43.40 +00:38:45.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 07 43.23 +00 38 52.4 12.5 U Cet 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 2507330409084786944,2461093.6410,12.51,0.05,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 2507330409084786944 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:43.23 +00:38:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.60 02:06:31.73 +02:57:38.4
156.89600 -54.88175 galactic Cet Second-epoch detections are separated by 6.1" 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 2514556571300675200 | 02:06:32.58 +02:57:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 06 31.73 +02 57 38.4 12.6 U Cet 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 2514556571300675200,2461093.6410,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514556571300675200 20260222.1410 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:31.73 +02:57:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.53 02:11:17.23 +01:39:01.3
159.86068 -55.38986 galactic Cet Second-epoch detections are separated by 6.8" 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 2514172837451032832 | 02:11:17.89 +01:39:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 11 17.23 +01 39 01.3 12.5 U Cet 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 2514172837451032832,2461093.6410,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514172837451032832 20260222.1410 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:11:17.23 +01:39:01.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.69 02:07:42.77 +00:38:29.0
159.46834 -56.71959 galactic Cet Second-epoch detections are separated by 1.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2507330409084786944 | 02:07:43.40 +00:38:45.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 07 42.77 +00 38 29.0 12.7 U Cet 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 2507330409084786944,2461093.6410,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2507330409084786944 20260222.1410 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:42.77 +00:38:29.0 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.76 02:06:58.61 +01:57:34.2
157.95253 -55.68976 galactic Cet Second-epoch detections are separated by 7.4" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514419853902228224 | 02:06:58.98 +01:57:30.7 (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 22.1410* 02 06 58.61 +01 57 34.2 12.8 U Cet 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 2514419853902228224,2461093.6410,12.76,0.05,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 2514419853902228224 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:58.61 +01:57:34.2 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.79 02:06:07.32 +01:24:51.5
158.12354 -56.26744 galactic Cet Second-epoch detections are separated by 8.4" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2508206616772926848 | 02:06:07.89 +01:24:46.0 (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 22.1410* 02 06 07.32 +01 24 51.5 12.8 U Cet 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 2508206616772926848,2461093.6410,12.79,0.05,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 2508206616772926848 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:07.32 +01:24:51.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.79 02:05:50.68 +02:48:36.1
156.76813 -55.09737 galactic Psc Second-epoch detections are separated by 1.9" 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 2514547775208319232 | 02:05:51.25 +02:48:28.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2514547775208319232,2461093.6410,12.79,0.05,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 2514547775208319232 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:50.68 +02:48:36.1 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.71 02:03:02.08 -02:59:47.2
161.36386 -60.41100 galactic Cet Second-epoch detections are separated by 8.2" 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 2492682955697785216 | 02:03:01.96 -03:00:14.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 03 02.08 -02 59 47.2 12.7 U Cet 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 2492682955697785216,2461093.6410,12.71,0.05,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 2492682955697785216 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:03:02.08 -02:59:47.2 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.78 02:15:26.65 +02:36:11.7
160.48587 -54.02747 galactic Cet Second-epoch detections are separated by 2.6" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514707612415577856 | 02:15:27.11 +02:36:10.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 15 26.65 +02 36 11.7 12.8 U Cet 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 2514707612415577856,2461093.6410,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514707612415577856 20260222.1410 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:15:26.65 +02:36:11.7 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.89 02:10:02.88 +02:56:35.3
158.22142 -54.45192 galactic Cet Second-epoch detections are separated by 7.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514611443803367296 | 02:10:02.66 +02:56:42.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 10 02.88 +02 56 35.3 12.9 U Cet 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 2514611443803367296,2461093.6410,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514611443803367296 20260222.1410 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:10:02.88 +02:56:35.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.81 02:06:03.94 +02:51:18.5
156.81267 -55.03081 galactic Psc Second-epoch detections are separated by 2.1" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514553856882000000 | 02:06:04.87 +02:51:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2514553856882000000,2461093.6410,12.81,0.05,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 2514553856882000000 20260222.1410 12.81CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:03.94 +02:51:18.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.80 02:06:03.76 +02:51:15.6
156.81223 -55.03188 galactic Psc Second-epoch detections are separated by 3.4" 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 2514553856882000000 | 02:06:04.87 +02:51:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2514553856882000000,2461093.6410,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514553856882000000 20260222.1410 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:03.76 +02:51:15.6 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.96 02:06:06.20 +02:29:01.2
157.15157 -55.34807 galactic Cet 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 2514502729590676096 | 02:06:07.13 +02:28:52.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 06 06.20 +02 29 01.2 13.0 U Cet 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 2514502729590676096,2461093.6410,12.96,0.05,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 2514502729590676096 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:06.20 +02:29:01.2 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.90 02:08:34.80 +01:08:56.4
159.31538 -56.17415 galactic Cet Second-epoch detections are separated by 6.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2508128684591118848 | 02:08:35.24 +01:08:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 08 34.80 +01 08 56.4 12.9 U Cet 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 2508128684591118848,2461093.6410,12.90,0.05,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 2508128684591118848 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:08:34.80 +01:08:56.4 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.01 02:05:36.73 +01:10:22.4
158.14980 -56.54004 galactic Cet Second-epoch detections are separated by 6.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J031.4050+01.1717 | 02:05:37.21 +01:10:18.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 05 36.73 +01 10 22.4 13.0 U Cet 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 J031.4050+01.1717,2461093.6410,13.01,0.05,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
ATO J031.4050+01.1717 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:36.73 +01:10:22.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.14 02:07:20.07 +03:08:17.6
157.04457 -54.62753 galactic Cet Second-epoch detections are separated by 6.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2514659302624008064 | 02:07:21.02 +03:08:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 07 20.07 +03 08 17.6 13.1 U Cet 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 2514659302624008064,2461093.6410,13.14,0.05,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 2514659302624008064 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:20.07 +03:08:17.6 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.06 02:12:29.28 +00:48:34.9
161.11631 -55.93317 galactic Cet Second-epoch detections are separated by 8.7" 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 2513294396376487552 | 02:12:29.77 +00:48:36.7 (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 22.1410* 02 12 29.28 +00 48 34.9 13.1 U Cet 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 2513294396376487552,2461093.6410,13.06,0.05,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 2513294396376487552 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:12:29.28 +00:48:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.24 02:06:22.17 +02:54:48.0
156.87696 -54.94260 galactic Psc Second-epoch detections are separated by 8.0" 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 2514556021545331968 | 02:06:23.23 +02:54:48.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2514556021545331968,2461093.6410,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2514556021545331968 20260222.1410 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:06:22.17 +02:54:48.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.10 02:13:06.70 +01:58:24.2
160.22966 -54.87247 galactic Cet Second-epoch detections are separated by 6.6" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2513533956767917056 | 02:13:07.11 +01:58:23.4 (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 22.1410* 02 13 06.70 +01 58 24.2 13.1 U Cet 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 2513533956767917056,2461093.6410,13.10,0.05,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 2513533956767917056 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:13:06.70 +01:58:24.2 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.12 02:12:56.14 +01:58:01.7
160.17114 -54.90144 galactic Cet Second-epoch detections are separated by 4.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J033.2359+01.9679 | 02:12:56.63 +01:58:04.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 12 56.14 +01 58 01.7 13.1 U Cet 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 J033.2359+01.9679,2461093.6410,13.12,0.05,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
ATO J033.2359+01.9679 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:12:56.14 +01:58:01.7 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.31 02:07:31.96 +03:03:50.3
157.18283 -54.66702 galactic Cet Second-epoch detections are separated by 8.4" 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 2514651983999998464 | 02:07:33.51 +03:03:45.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 07 31.96 +03 03 50.3 13.3 U Cet 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 2514651983999998464,2461093.6410,13.31,0.05,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 2514651983999998464 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:31.96 +03:03:50.3 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 13.27 02:05:06.46 +02:03:54.6
157.14152 -55.83487 galactic Cet Second-epoch detections are separated by 6.4" 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 2508434486262486784 | 02:05:07.65 +02:03:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1410* 02 05 06.46 +02 03 54.6 13.3 U Cet 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 2508434486262486784,2461093.6410,13.27,0.05,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 2508434486262486784 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:05:06.46 +02:03:54.6 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1410 2461093.6410 12.31 02:12:19.82 +00:21:09.1
161.51074 -56.33597 galactic Cet Second-epoch detections are separated by 1.2" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2507089444239694976 | 02:12:20.11 +00:21:04.5 (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 22.1410* 02 12 19.82 +00 21 09.1 12.3 U Cet 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 2507089444239694976,2461093.6410,12.31,0.05,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 2507089444239694976 20260222.1410 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/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:12:19.82 +00:21:09.1 ;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_Cet-04-Q2b1x1_2025-12-22_22-37-45_20_00sec_-14_90C_LIGHT_0185_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20_00sec_-14_90C_LIGHT_0185_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20_00sec_-14_90C_LIGHT_0185_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20_00sec_-14_90C_LIGHT_0185_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_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 22.1410* 02 42 35.88 -03 04 22.9 11.7 U Cet 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 J024236-0304.4,2461093.6410,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J024236-0304.4 20260222.1410 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:42:35.88 -03:04:22.9 ;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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_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 22.1410* 02 26 02.51 +00 10 43.0 8.2 U Cet 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
R Cet,2461093.6410,8.15,0.05,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
R Cet 20260222.1410 8.15CV 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:26:02.51 -00:10:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20_00sec_-15_00C_LIGHT_0067_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png resample_wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20_00sec_-15_00C_LIGHT_0066_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: 2461032.69191674 23.12.2025 04:36:11.606 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
First image: 2461032.69191674 23.12.2025 04:36:11.606 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
Last image: 2461093.64128155 22.02.2026 03:23:16.726 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 73
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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: 7 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): 6608
Objects passed selection criteria: 6588
Measurements per detected object (mean, median, min, max): 3.0 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 4.0 2 4
Average stars detected per image: 5210.5
Average stars matched: 5064.25 (97.1932 %)
Memory usage VmPeak: 114936 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 04:03:12 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: 2461032.69191674 23.12.2025 04:36:11.606 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
First image: 2461032.69191674 23.12.2025 04:36:11.606 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
Last image: 2461093.64128155 22.02.2026 03:23:16.726 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 414
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 22 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 32941
Objects passed selection criteria: 32847
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 25090.2
Average stars matched: 23625.2 (94.1611 %)
Memory usage VmPeak: 135604 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 04:06:01 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:
Cet-04-Q2b1x1
#######################################
########### Starting Cet-04-Q2b1x1 ###########
Processing Cet-04-Q2b1x1
server tau has sufficient free disk space available: 1030560 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1030560 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.png' -> 'transient_report/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits_preview.png'
Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
renamed 'Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.png' -> 'transient_report/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits_preview.png'
Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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= 699.1073
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 554.9486
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1807.6724
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 587.1852
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1810.6703
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 587.4327
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.58569
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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
SExtractor catalog cache: saved Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat to cache
SExtractor catalog cache: saved Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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: 2461093.64077693
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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits exists and is non-empty
Saving wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits to local_wcs_cache/
'wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits' -> 'local_wcs_cache/wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits'
wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits exists and is non-empty
Saving wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits to local_wcs_cache/
'wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits' -> 'local_wcs_cache/wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits'
wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits exists and is non-empty
Saving wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits to local_wcs_cache/
'wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits' -> 'local_wcs_cache/wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits'
wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
Saving wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits to local_wcs_cache/
'wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits' -> 'local_wcs_cache/wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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 02:34:05.028 -02:00:03.11
Second-epoch image center 02:34:09.005 -02:02:34.68
Angular distance between the image centers 0.05 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 02:34:05.028 -02:00:03.11
Second-epoch image center 02:34:07.482 -02:02:45.72
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 02:34:09.005 -02:02:34.68
Second-epoch second image center 02:34:07.482 -02:02:45.72
Angular distance between the image centers 0.00704 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits &> /tmp/tmp.qQuFHv4Gt9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits &> /tmp/tmp.O1T5rBFkiI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits &> /tmp/tmp.IGkHCJNTDR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.OyuLsEiWkp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits and wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits and wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat
Found non-empty wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits and wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat
The reference image (wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits) and catalog (wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat) found
'wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.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 3587 out of 6819 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.907312
a=0.000000 b=1.000000 c=22.907312
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 67 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
2.0 pix Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
3.8 pix Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
3.8 pix Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
Limiting magnitude estimates:
15.3 mag. Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
15.3 mag. Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
14.0 mag. Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
13.9 mag. Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.6 (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.qQuFHv4Gt9 (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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits' -> 'wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=492, passed=6819
Got 6819 stars (including 6317 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat
util/solve_plate_with_UCAC5 got 6819 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits -region wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.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.O1T5rBFkiI (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/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits' -> 'wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=512, passed=6779
Got 6779 stars (including 6257 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat
util/solve_plate_with_UCAC5 got 6779 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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 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 - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits -region wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.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.IGkHCJNTDR (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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=386, passed=3740
Got 3740 stars (including 3352 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 3740 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 963 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: 0.63"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 963 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits -region wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.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.OyuLsEiWkp (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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=365, passed=3675
Got 3675 stars (including 3307 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 3675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 962 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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 Cet-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20500.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 50s
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: 10s
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Considering the candidate 20338_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20338_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:35.49 -06:02:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 5.898 2490686311301204992 031.89939778334 -06.04506944881 10.2647 9.7541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20339_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20339_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:28.02 -00:39:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 1.079 2506871152526234752 032.61703457952 -00.65045491101 10.4048 10.0126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20342_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20342_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:08.05 -00:36:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 0.980 2506898335374859264 032.28327382653 -00.60684049659 10.1093 9.6858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20343_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20343_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20344_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20344_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:14:35.47 +02:04:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 1.054 2513557390109500288 033.64756755292 +02.07867274762 10.1941 9.7713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20345_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20345_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:44.15 -02:18:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 1.769 2494212750033557120 031.93437055498 -02.31540697200 9.9874 9.5789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20346_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20346_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:15:18.03 +01:51:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 1.292 2513537083504158336 033.82476723772 +01.86580967615 10.1412 9.6870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20347_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20347_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:24.55 +00:41:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 1.293 2507290861025993088 032.85248109282 +00.69516694143 10.0106 9.5864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20348_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20348_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 20349_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20349_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:00.90 +01:27:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 2.472 2513403836438660224 033.00306471424 +01.45112998316 10.0577 9.6272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20350_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20350_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:16:38.70 +01:36:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 1.689 2513468535826170752 034.16089873680 +01.60158888499 10.2990 9.9087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20351_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20351_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:48.55 +00:07:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 2.628 2507067247848720768 032.95262132843 +00.11976523294 10.0197 9.6180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20352_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20352_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:05.15 -01:58:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 2.441 2506290305444813568 031.27208990473 -01.98230316059 9.6044 9.0658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20353_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20353_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:38.66 -00:56:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 5.698 2506518660265805184 031.41214815808 -00.94564321825 9.6979 9.2451 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20354_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20354_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:48.76 -03:50:31.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)
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Considering the candidate 20356_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20356_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 20357_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20357_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:18.42 -01:43:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.08, MAG_FAINT_SEARCH_LIMIT=12.06)GAIADR2_OUTPUT=# 2.522 2494376237964265088 032.07738954606 -01.71936968124 9.8185 9.4559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20359_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20359_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:13.08 -05:44:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 5.140 2491061657083113088 032.30334600710 -05.74370968036 9.6390 9.1907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20360_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20360_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:10.14 -01:57:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 5.467 2494321846498461696 032.29362872436 -01.96519402095 9.7721 9.3696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20361_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20361_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 20362_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20362_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20363_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20363_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 20364_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20364_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:21.25 -01:34:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.32, MAG_FAINT_SEARCH_LIMIT=11.30)GAIADR2_OUTPUT=# 3.266 2494731620738219776 032.83937862360 -01.57260057490 9.3331 8.9332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20365_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20365_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 20366_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20366_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:03:49.19 -04:34:42.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20367_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20367_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:13.37 -00:58:07.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20368_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20368_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:02.33 -04:13:00.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20369_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20369_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:15.18 -04:21:52.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20370_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20370_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 20374_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20374_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:29.73 +00:02:06.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20375_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20375_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:15.80 +02:44:44.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20378_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20378_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:48.67 +01:26:30.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20379_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20379_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:33.53 -00:37:12.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20381_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20381_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:41.52 -00:26:13.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.66, MAG_FAINT_SEARCH_LIMIT=9.64)
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Considering the candidate 20382_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20382_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:16:49.97 +02:34:41.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20387_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20387_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:41.69 +00:55:46.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20393_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20393_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:37.57 +01:55:47.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20394_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20394_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:24.75 +02:01:34.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20395_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20395_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:19.21 +00:19:20.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20399_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20399_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:48.42 +00:49:36.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20400_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20400_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:51.54 +02:30:44.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20408_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20408_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:41.51 +01:42:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.24, MAG_FAINT_SEARCH_LIMIT=11.22)GAIADR2_OUTPUT=# 1.577 2514165243945430272 032.42339098094 +01.70604107952 9.0139 8.7427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20410_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20410_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20416_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20416_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20417_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20417_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20421_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20421_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:37.34 +02:17:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.56, MAG_FAINT_SEARCH_LIMIT=11.54)GAIADR2_OUTPUT=# 5.867 2514353329153444736 032.65688307103 +02.29084877028 9.5560 9.3818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20426_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20426_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:46.98 +01:08:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.66, MAG_FAINT_SEARCH_LIMIT=11.64)GAIADR2_OUTPUT=# 3.543 2508140302477906304 031.69670959659 +01.14913565687 9.3023 8.9620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20427_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20427_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20433_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20433_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:24.67 +02:59:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)GAIADR2_OUTPUT=# 3.716 2514613333588974976 032.60220512603 +02.99068319034 9.5950 8.9189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20434_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20434_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20436_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20436_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20437_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20437_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:25.31 +02:45:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.76, MAG_FAINT_SEARCH_LIMIT=11.74)GAIADR2_OUTPUT=# 3.186 2514569868519950720 032.60494177343 +02.75708013152 9.6618 9.0311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20447_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20447_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20448_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20448_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:25.35 +01:08:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 2.344 2508136591626161408 031.85500644418 +01.13775928368 9.7930 9.1206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20454_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20454_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 20455_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20455_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 20456_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20456_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20459_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20459_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:50.85 +02:08:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 4.904 2514440568528968064 031.46311337422 +02.13568032787 9.6927 8.9522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20460_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20460_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:18.69 +02:57:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 3.154 2517561674019047296 031.32724113655 +02.95550532238 9.2382 8.7138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20462_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20462_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 20463_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20463_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:16.26 +02:37:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 4.375 2514399886598935168 032.81895572423 +02.62161559307 9.7575 9.3331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20467_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20467_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:06.09 +00:21:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 0.853 2507219697712642048 031.77514337591 +00.35249481676 9.8166 9.4146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20469_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20469_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 20472_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20472_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:17.45 +02:37:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 0.938 2514529594611331072 031.57246716175 +02.62782146123 9.5844 9.0520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20482_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20482_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:26.10 +02:13:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 3.188 2514447444772129408 031.60941857933 +02.23008540634 9.9256 9.0853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20500_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20500_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20512_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20512_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:42:35.87 -03:04:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 1.509 2495636965484564608 040.64978267371 -03.07332170816 10.9039 9.5848 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 61s
Prepared the HTML report for the field Cet-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 ####
02:05:34.62 -05:59:47.7
02:07:59.19 -02:17:33.2
02:15:16.47 +02:22:34.2
02:06:39.03 +03:06:12.1
02:14:46.59 +02:13:55.3
02:13:13.49 +01:07:24.9
02:14:51.16 +02:31:17.6
02:05:42.86 +01:53:20.2
02:08:20.95 +03:03:22.5
02:05:17.62 +02:57:27.3
02:17:51.12 +02:22:28.9
02:06:48.57 +02:51:54.0
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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
SExtractor catalog cache: saved Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat to cache
SExtractor catalog cache: saved Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
Creating symlink local_wcs_cache/wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
Creating symlink local_wcs_cache/wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
Creating symlink local_wcs_cache/wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits exists and is non-empty
wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits exists and is non-empty
wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits exists and is non-empty
wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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 02:34:05.028 -02:00:03.11
Second-epoch image center 02:34:09.005 -02:02:34.68
Angular distance between the image centers 0.05 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 02:34:05.028 -02:00:03.11
Second-epoch image center 02:34:07.482 -02:02:45.72
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 02:34:09.005 -02:02:34.68
Second-epoch second image center 02:34:07.482 -02:02:45.72
Angular distance between the image centers 0.00704 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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits &> /tmp/tmp.Ld9bIH0Cso
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits &> /tmp/tmp.DUN5D92O0W
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits &> /tmp/tmp.yXEmyjcXhU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.uAifbHGgNj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits and wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.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_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits and wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat
Found non-empty wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits and wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat
The reference image (wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits) and catalog (wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat) found
'wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.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 3631 out of 34431 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.812498
a=0.000000 b=1.000000 c=22.812498
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 377 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
1.9 pix Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
3.7 pix Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
3.7 pix Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
Limiting magnitude estimates:
15.4 mag. Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
15.4 mag. Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
14.3 mag. Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
14.2 mag. Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.5 (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.Ld9bIH0Cso (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/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits' -> 'wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1543, passed=34418
Got 34418 stars (including 32809 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat
util/solve_plate_with_UCAC5 got 34418 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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 969 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: 0.27"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits -region wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-36-11_20.00sec_-14.90C_LIGHT_0184.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.DUN5D92O0W (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/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits' -> 'wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1533, passed=34584
Got 34584 stars (including 32992 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat
util/solve_plate_with_UCAC5 got 34584 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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits -region wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2025-12-22_22-37-45_20.00sec_-14.90C_LIGHT_0185.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.yXEmyjcXhU (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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=1816, passed=16419
Got 16419 stars (including 14590 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 16419 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 964 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: 0.63"
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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 964 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits -region wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-22-33_20.00sec_-15.00C_LIGHT_0066.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.uAifbHGgNj (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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=61, blended=1727, passed=16133
Got 16133 stars (including 14394 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 16133 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 962 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cet-04-Q2b1x1_212431_TTUQ2b1x1_5712_aL2Rg386/Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067.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 Cet-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out52415.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_local.txt__out11519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52579.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53839.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 207s
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: 65s
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Considering the candidate 52415_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52415_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:46:58.84 -03:19:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.777 5185730460785426176 041.74522274691 -03.31700957619 13.9552 13.4783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52420_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52420_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52421_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52421_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52422_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52422_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52427_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52427_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:35:29.17 -07:02:13.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)
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Considering the candidate 52432_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52432_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:49.93 -03:09:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.673 2493905578268197504 032.70822770537 -03.15072856322 12.3486 11.7974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52433_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52433_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:04.42 -00:16:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 3.882 2506937196238963456 032.51948031147 -00.26787136196 11.9567 11.5514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52434_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52434_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:04:07.41 -03:18:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.471 2492615267013229056 031.03109325272 -03.30843223316 11.7073 11.2952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52435_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52435_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52437_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52437_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:09.87 -02:42:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.065 2494169937799554432 031.54149744421 -02.71476993836 11.9076 11.4124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52438_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52438_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52439_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52439_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:04:07.48 -03:18:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.464 2492615267013229056 031.03109325272 -03.30843223316 11.7073 11.2952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52440_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52440_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:03.64 -03:22:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 0.949 2492435698725131648 031.76541773142 -03.37547061714 12.0048 11.3618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52441_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52441_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:30.31 -04:40:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.846 2491401268737211136 031.87729348900 -04.67378711135 11.9723 11.5182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52443_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52443_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:17.95 -03:38:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.637 2493057781788058624 033.07496266096 -03.64688052579 12.2493 11.7706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52444_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52444_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:50.27 -00:39:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.890 2506894654587768704 031.96009767079 -00.66092671799 11.8023 11.4067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52445_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52445_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:13.67 -05:58:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 3.144 2488041809742159872 032.80693310082 -05.97365086597 11.9884 11.4693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52446_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52446_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:19:00.44 +01:54:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.167 2513672868894609792 034.75253198409 +01.90849246089 12.3197 11.8912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52447_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52447_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:19.01 -05:54:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.269 2491054819495182464 032.32937212882 -05.90410676700 11.9556 11.4615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52448_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52448_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:03:38.57 -04:02:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 0.325 2492290082153813248 030.91074389251 -04.03977740973 11.6192 11.0510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52449_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52449_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:14:09.47 +00:40:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.178 2513095663945245056 033.54004652919 +00.67246942608 12.1994 11.7440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52450_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52450_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52451_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52451_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:25.14 -05:42:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.756 2490749052183457024 031.85559916443 -05.69949898010 11.7857 11.3318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52452_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52452_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:26.35 -02:58:55.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52453_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52453_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52454_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52454_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52457_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52457_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:14.16 -05:10:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 4.359 2490981220935629056 031.30996763307 -05.18071146661 11.6427 11.2538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52458_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52458_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:22.11 -01:26:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 0.961 2494738046009288576 032.84225645170 -01.43521196494 12.0568 11.5696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52460_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52460_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:16:04.95 +02:22:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.364 2513943692353129216 034.02081207413 +02.37622592638 12.2402 11.7469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52461_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52461_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:57.07 -05:53:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.696 2490739122219054336 031.73899349305 -05.88361711734 11.4215 10.8475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52463_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52463_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:26.70 -05:15:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 3.448 2491153118411298688 032.11203287164 -05.25266763985 11.7823 11.2111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52465_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52465_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:47.89 -00:03:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.049 2507131603638678912 031.69976956231 -00.05740364449 11.6440 11.1418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52467_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52467_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:16:00.51 +02:08:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.468 2513549487369695744 034.00171942655 +02.13928954066 11.9677 11.5357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52470_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52470_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52471_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52471_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:13:28.26 +00:56:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 2.730 2513325599314455936 033.36789876068 +00.93908981715 11.8189 11.1389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52472_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52472_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:17:49.83 +01:07:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 4.070 2513183208263476992 034.45865698288 +01.11656574578 12.3935 11.8957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52473_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52473_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:39.48 -05:18:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.287 2491159818560281472 032.41507176591 -05.30328197412 11.8287 11.3044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52474_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52474_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:19:04.02 -06:25:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 2.112 2487074067711342464 034.76733889242 -06.42640139908 12.2393 11.8323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52475_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52475_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52478_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52478_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:17:14.83 +02:30:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 4.676 2513940599975982464 034.31306306593 +02.50489532610 12.0545 11.6431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.676#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52481_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52481_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52483_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52483_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:21:12.95 +02:53:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.392 2514047664921094144 035.30357628147 +02.89217334251 12.2365 11.7872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52484_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52484_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:01.02 -01:05:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.846 2506820849869760256 032.25472510647 -01.08281268179 11.8595 11.3527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52486_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52486_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:16:47.20 +03:02:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.623 2514747916388674304 034.19736533194 +03.03740101400 11.6463 11.0424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52487_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52487_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52488_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52488_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:03:02.14 -03:00:10.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 52489_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52489_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:20.68 -06:01:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.882 2488038103185951616 032.83575085348 -06.02587007409 11.7743 11.3383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52490_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52490_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:18.82 -04:03:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.554 2492324819849200640 031.57887351960 -04.06173823144 11.6074 11.0147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52491_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52491_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:18:44.79 +02:24:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 3.948 2513909538772485376 034.68602723006 +02.40894750121 11.9684 11.5471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52493_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52493_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:53.51 -06:18:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.679 2487661584877364608 032.22362805735 -06.30280811220 11.6531 11.2483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52494_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52494_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:46.69 -02:42:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 1.430 2494172446060455168 031.44438781635 -02.70075503490 11.5014 11.0348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52495_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52495_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 52496_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52496_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:03:28.85 -03:43:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.116 2492316715246627840 030.87134855822 -03.71816704442 11.5129 11.0584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52497_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52497_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:13:44.60 -00:34:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 2.095 2494938633866698880 033.43550736514 -00.57087897176 11.9831 11.5823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52499_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52499_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:13:07.34 +00:58:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.257 2513306250486547328 033.28104771591 +00.97897338976 11.8748 11.4369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52500_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52500_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:41.08 -02:24:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 5.139 2494233885568184960 031.42026299422 -02.41271682615 11.3723 10.9470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52501_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52501_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:58.63 -00:09:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.556 2507134966597424768 031.99480930214 -00.15584718650 11.5806 11.1053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52502_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52502_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:19:18.42 +02:36:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 3.545 2513922011358024576 034.82742165316 +02.59969609262 11.8543 11.4039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52503_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52503_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:14:50.21 +02:11:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 2.400 2513564360841094784 033.70862221039 +02.18915160630 11.9883 11.5870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52505_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52505_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:03:40.47 -04:19:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.373 2492211020395834496 030.91927324917 -04.32287872299 11.3408 10.9107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52506_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52506_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:14:46.91 -00:35:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 0.595 2494935683224347392 033.69530544606 -00.59174255130 12.0108 11.6142 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#
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Considering the candidate 52508_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52508_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52509_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52509_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:38.97 -06:32:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.447 2487769989852289024 033.16192064383 -06.54917476340 11.6304 11.2471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52510_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52510_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:37.03 -04:42:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.840 2491280902278374656 032.90333598413 -04.71253603695 11.8995 11.4193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52512_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52512_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:14:33.37 +01:14:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.127 2513338273762700672 033.63935169652 +01.23626200491 11.8275 11.3846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52513_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52513_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:13:35.35 +01:52:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.312 2513529210829027328 033.39787659379 +01.87820641148 11.8504 11.3719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52514_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52514_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:20:52.62 -04:30:36.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)
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Considering the candidate 52515_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52515_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:08.84 +00:27:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.424 2507279384873364224 032.53727970833 +00.44966005629 11.7412 11.3162 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52516_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52516_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:49.54 -06:12:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 0.750 2487973987914215552 033.20623267578 -06.20237276334 11.7289 11.2825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52517_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52517_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:15:12.20 -06:01:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.257 2487815447785767168 033.80052580481 -06.02886290517 11.6801 11.2200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52518_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52518_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:17:49.05 +01:48:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.535 2513853017002878976 034.45480113424 +01.80798104662 12.1457 11.7588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52519_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52519_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:25.36 -03:37:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.467 2492354717117177984 031.60681890019 -03.63104937332 11.5790 11.1264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52521_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52521_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:00.46 -01:53:27.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)
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Considering the candidate 52522_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52522_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:15:55.52 +00:51:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.809 2513125488198165120 033.98236494048 +00.85690212630 11.9096 11.4791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52523_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52523_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:46.99 -01:46:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.319 2494384415581991168 031.69606859065 -01.77387897387 11.3654 10.9243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52525_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52525_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:56.31 -00:42:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.112 2506893421932252416 031.98490159934 -00.70996194526 11.5527 11.1344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52526_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52526_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:15.09 +00:01:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.125 2507238634223672064 032.31345230868 +00.02932109095 11.6957 11.2939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52528_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52528_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:07.56 -00:11:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.010 2507029555215706368 032.78166541277 -00.19460554666 11.7953 11.4457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52530_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52530_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:03.12 +02:05:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.702 2514295780887120128 033.01280846174 +02.09021328379 11.4498 10.9318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52532_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52532_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:34.93 +00:28:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.251 2507317799060833024 032.14519986841 +00.47814534522 11.4627 10.7386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52534_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52534_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:09.33 -05:41:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 5.395 2491073957869447296 032.28766993097 -05.69520442676 11.2943 10.9561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52537_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52537_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:24.21 -02:51:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.226 2493970621252847104 031.85114315764 -02.85879348973 11.4669 10.9993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52538_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52538_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:57.96 -06:06:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 5.261 2490710637995953664 031.49074320409 -06.10253042661 11.0910 10.6775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52539_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52539_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:13:49.32 +01:44:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.911 2513514715314457216 033.45553064468 +01.74666437136 11.7062 11.2437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52543_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52543_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52544_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52544_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:32:47.67 -00:13:41.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
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Considering the candidate 52545_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52545_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:07.97 +00:02:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.816 2507042508837060992 032.78271285378 +00.04743304989 11.6257 11.2104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52546_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52546_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:06.80 -03:14:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.779 2493153370580581376 032.77863176512 -03.24781081390 11.7402 11.3492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52547_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52547_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52549_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52549_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52550_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52550_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:13:41.74 +01:03:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 1.229 2513328927913868800 033.42390600718 +01.05271426049 11.6412 11.1699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52551_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52551_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52553_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52553_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52554_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52554_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52556_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52556_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:38.92 -03:48:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 4.697 2492356813061245440 031.91331164169 -03.80101882283 11.3333 10.9281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52558_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52558_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:06.16 -00:46:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.359 2506833391173769600 032.52639616625 -00.77849864821 11.5637 11.0051 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 52559_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52559_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:18:27.50 +02:21:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 3.030 2513907752066091136 034.61404434505 +02.35553581594 11.5750 11.1232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52560_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52560_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:27.75 -03:02:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 5.637 2493903070007265664 032.36709420470 -03.03974151912 11.2290 10.8597 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52561_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52561_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:04:52.77 -03:34:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.610 2492411268950929792 031.21997505001 -03.57598064462 11.2932 10.7984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52562_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52562_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:24:29.14 +03:06:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.341 2515361959273052544 036.12161586393 +03.10290866771 11.8921 11.4467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52563_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52563_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:14:02.44 +01:56:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.826 2513530692592793472 033.51039548919 +01.94948320294 11.4392 10.9548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52564_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52564_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:27.50 -01:53:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 2.406 2494379055462818816 031.86523568543 -01.88453564323 11.2140 10.7548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52565_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52565_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:09.84 +00:16:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 2.841 2507249040928810368 032.54140784762 +00.27221337765 11.2775 10.8472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52566_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52566_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:11.20 -02:33:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 4.599 2494181040290578816 031.54769026561 -02.55968229966 11.3059 10.9451 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52567_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52567_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:30.24 -05:49:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 3.243 2488059371863978752 032.62602196969 -05.82981724218 11.1671 10.7642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52568_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52568_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:04:15.26 -04:24:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 3.890 2492196250003968512 031.06460352991 -04.40777460018 11.0386 10.5734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52569_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52569_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52570_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52570_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:15.91 -05:36:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 4.753 2491124638483515392 032.06505051346 -05.60310534101 11.1922 10.7753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52571_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52571_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:26.60 -01:03:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 1.382 2494812400483061888 032.86080721606 -01.05086711855 11.4896 11.0729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52573_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52573_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:12.43 -06:07:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.575 2488030818921420928 032.80107748158 -06.11947072804 11.4181 10.9825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52574_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52574_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:01.45 +00:53:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.007 2513313294232589184 032.75520884632 +00.88420260184 11.4455 10.9383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52575_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52575_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52576_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52576_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:13:51.51 -01:28:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.701 2494560711104118912 033.46454228671 -01.46778485010 11.7025 11.2577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52578_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52578_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52579_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52579_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52581_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52581_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:04.92 -02:51:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 2.100 2494154514572595456 031.52107286056 -02.86622025403 11.0111 10.6131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52582_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52582_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52583_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52583_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:56.29 -00:42:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.932 2506719527296464128 031.48461913931 -00.71677480128 11.0249 10.6190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52585_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52585_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:32.76 -03:24:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 5.181 2492432400190249088 031.63780903847 -03.41375830112 11.0479 10.6897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52589_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52589_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52590_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52590_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52591_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52591_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:36.92 -03:38:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.242 2492365884032169088 032.15417829406 -03.64188382318 11.1071 10.6109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52592_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52592_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:13:47.71 -00:46:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.996 2494927127649471744 033.44904916678 -00.77139852913 11.4397 11.0604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52593_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52593_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:19:04.60 +02:50:07.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)
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Considering the candidate 52594_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52594_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:49.72 -01:34:40.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)
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Considering the candidate 52595_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52595_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52596_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52596_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:18:13.14 +02:31:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 2.539 2513961666791170048 034.55485526810 +02.53250306567 11.2866 10.8313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52597_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52597_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:19:05.26 +02:06:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 1.525 2513865008551566080 034.77185109587 +02.10602953209 11.4060 11.0079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52599_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52599_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:21.76 -05:55:34.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)
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Considering the candidate 52601_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52601_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52602_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52602_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:16:46.99 +02:29:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 4.502 2513952080424145280 034.19485049470 +02.49024108843 11.0653 10.6387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52603_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52603_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52604_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52604_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:58.34 -00:39:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 5.148 2494852841895108608 032.99165319661 -00.65347781009 11.0555 10.6666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52606_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52606_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:44.42 -03:25:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 5.520 2492429449548121856 031.68654098693 -03.42645571481 10.7905 10.3236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52607_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52607_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 52608_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52608_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:03:16.28 -05:18:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 4.521 2490999328517694080 030.81678666318 -05.30720075632 10.2511 9.7808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52609_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52609_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52610_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52610_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52611_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52611_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:03:44.84 -05:47:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 3.905 2490919820083143296 030.93582023983 -05.78937279543 10.1838 9.7013 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 52612_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52612_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52613_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52613_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:38.35 -04:54:55.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)
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Considering the candidate 52614_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52614_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:02:57.95 -05:55:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 4.156 2490823028700229504 030.74053843287 -05.92956492430 10.0793 9.6124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52615_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52615_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52616_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52616_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:58.23 -06:02:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 2.671 2490674766429112064 031.99194851384 -06.04395213326 10.4579 10.0512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52618_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52618_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52619_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52619_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:04:23.17 -03:14:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.67, MAG_FAINT_SEARCH_LIMIT=12.65)GAIADR2_OUTPUT=# 2.813 2492617358661665280 031.09583748067 -03.24935315760 10.3964 9.9421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52621_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52621_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:17:38.91 +02:54:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 2.060 2513993071592030336 034.41218075712 +02.91556951933 10.8240 10.3804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52622_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52622_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:35.92 -06:02:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 3.582 2490686311301204992 031.89939778334 -06.04506944881 10.2647 9.7541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52623_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52623_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52624_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52624_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52626_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52626_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:02.80 -02:03:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 2.146 2494361012304618752 032.01225888170 -02.05601133796 10.4440 9.9950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52627_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52627_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:40.82 -00:40:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 4.100 2506859165273144448 032.67116508522 -00.67888401489 10.5553 10.0632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52628_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52628_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52629_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52629_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52630_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52630_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52631_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52631_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52632_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52632_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:34.67 -05:59:47.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52633_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52633_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:49.03 -03:50:31.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)
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Considering the candidate 52634_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52634_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:21:41.74 +02:40:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 2.695 2514005269298760448 035.42353296229 +02.68078193735 10.1379 9.6682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52636_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52636_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:13.12 -05:44:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.92, MAG_FAINT_SEARCH_LIMIT=11.90)GAIADR2_OUTPUT=# 5.631 2491061657083113088 032.30334600710 -05.74370968036 9.6390 9.1907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52637_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52637_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 52638_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52638_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52639_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52639_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52640_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52640_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:48.41 -01:56:01.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52641_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52641_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:03:49.24 -04:34:42.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52642_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52642_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:02.46 -04:13:00.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52643_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52643_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:15.22 -04:21:51.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52644_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52644_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52649_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52649_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:29.52 +00:02:07.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52650_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52650_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:15.97 +02:44:42.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52652_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52652_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:48.65 +01:26:30.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52654_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52654_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:41.70 -00:26:13.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.41, MAG_FAINT_SEARCH_LIMIT=9.39)
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Considering the candidate 52657_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52657_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:16:49.89 +02:34:42.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52662_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52662_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:41.49 +00:55:47.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52668_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52668_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:37.63 +01:55:46.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52669_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52669_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:24.48 +02:01:37.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52671_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52671_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:19.29 +00:19:20.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52680_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52680_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52684_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52684_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:51.04 +02:30:49.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52685_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52685_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:15:16.55 +02:22:33.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52687_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52687_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:41.25 +01:42:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.11, MAG_FAINT_SEARCH_LIMIT=11.09)GAIADR2_OUTPUT=# 5.483 2514165243945430272 032.42339098094 +01.70604107952 9.0139 8.7427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52694_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52694_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:14:46.43 +02:13:56.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52700_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52700_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:39.02 +03:06:12.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52703_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52703_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:37.37 +02:17:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.47, MAG_FAINT_SEARCH_LIMIT=11.45)GAIADR2_OUTPUT=# 5.267 2514353329153444736 032.65688307103 +02.29084877028 9.5560 9.3818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52708_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52708_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52710_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52710_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52712_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52712_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:13:13.45 +01:07:25.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52722_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52722_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52725_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52725_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:24.69 +02:59:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 4.298 2514613333588974976 032.60220512603 +02.99068319034 9.5950 8.9189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52726_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52726_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:25.34 +02:45:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 3.619 2514569868519950720 032.60494177343 +02.75708013152 9.6618 9.0311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52729_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52729_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:17.78 +02:57:27.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52738_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52738_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52742_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52742_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52745_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52745_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:17:51.03 +02:22:29.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52749_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52749_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:25.27 +01:08:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 1.053 2508136591626161408 031.85500644418 +01.13775928368 9.7930 9.1206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52750_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52750_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52755_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52755_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:19.87 +03:03:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 5.875 2514643913756089856 032.08425899392 +03.05914247784 9.6663 8.9846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52758_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52758_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52759_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52759_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52761_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52761_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52762_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52762_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 52763_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52763_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52774_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52774_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 52781_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52781_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52787_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52787_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:18.48 +02:16:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 0.019 2514349622596507520 032.82700216793 +02.27602293191 10.1947 9.5462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52790_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52790_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:15:17.69 +01:51:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 3.935 2513537083504158336 033.82476723772 +01.86580967615 10.1412 9.6870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52797_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52797_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:16:38.30 +01:36:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 4.782 2513468535826170752 034.16089873680 +01.60158888499 10.2990 9.9087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52798_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52798_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52803_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52803_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:48.19 +02:51:54.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52805_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52805_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52807_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52807_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52810_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52810_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52819_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52819_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52821_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52821_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:04:50.16 -00:15:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 1.800 2506793808755164032 031.20862805489 -00.26233242206 10.2333 9.7330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52823_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52823_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52832_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52832_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 52839_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52839_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52841_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52841_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:35.28 +00:52:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 5.280 2513311030785354112 032.89845134478 +00.87520402723 10.5444 10.1229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52848_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52848_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52870_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52870_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52872_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52872_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52880_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52880_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52889_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52889_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52895_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52895_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52896_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52896_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52899_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52899_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52902_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52902_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52905_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52905_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52909_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52909_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52911_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52911_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52915_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52915_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:36.22 +02:51:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.288 2514411057809316480 033.15140220039 +02.85143841077 10.6815 10.1302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52917_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52917_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52925_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52925_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52927_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52927_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52929_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52929_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 52930_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52930_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52931_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52931_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 52933_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52933_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:22.44 +01:58:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 0.363 2514202391118197120 032.59342051824 +01.96674336467 10.9177 10.2941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52935_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52935_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:09.95 +01:35:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.373 2514205861451762048 032.04181856763 +01.58404209064 10.8188 10.1458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52942_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52942_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:04:41.61 -00:00:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 3.950 2507189087480924160 031.17443203006 -00.00401647586 10.8265 10.7069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52951_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52951_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:24.09 +02:10:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 3.852 2514350069273710976 032.59948746843 +02.17940139774 10.9315 10.2449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52961_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52961_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52965_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52965_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52969_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52969_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52970_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52970_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52978_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52978_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52981_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52981_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52985_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52985_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 52986_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52986_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52987_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52987_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:21.87 +01:05:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 4.326 2513369614139226880 032.84228745966 +01.09227792029 10.9893 10.5382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52991_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 52991_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:48.29 +02:42:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 2.366 2514402296075398784 032.95176250388 +02.71029888444 11.0074 10.6262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52997_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52997_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 52999_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 52999_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53000_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53000_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:20.98 +03:00:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 4.034 2514613604171403648 032.58852891076 +03.01531557169 11.0100 10.6171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53006_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53006_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53013_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53013_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53014_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53014_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53016_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53016_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53018_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53018_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:57.59 +02:55:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 3.373 2514415352776582400 032.98928861020 +02.92437836958 11.1422 10.4688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53022_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53022_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53025_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53025_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53026_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53026_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53029_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53029_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53032_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53032_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53033_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53033_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53048_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53048_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:17.17 +00:52:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 4.032 2508093676312948480 031.82265086658 +00.87859468011 11.0084 10.5405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53054_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53054_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53063_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53063_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53065_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53065_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53071_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53071_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:16:09.54 +03:11:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 5.242 2514766784180562816 034.04099549000 +03.19027041012 11.3016 10.8732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53079_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53079_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53080_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53080_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53081_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53081_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53088_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53088_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53092_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53092_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53098_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53098_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53109_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53109_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53113_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53113_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53126_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53126_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53128_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53128_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:17:29.34 +02:03:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 4.216 2513873014370606720 034.37340071721 +02.05786129002 11.4857 11.0851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53129_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53129_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53130_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53130_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53134_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53134_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53139_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53139_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53151_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53151_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:52.26 +02:12:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 4.540 2514268804197322240 032.46900759202 +02.20450676485 11.4276 11.0394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53153_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53153_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 53161_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53161_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:22.50 +00:54:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.884 2507367582026617600 032.09426731250 +00.90758647336 11.3939 10.9595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53182_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53182_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:04.21 +02:24:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.565 2514498881300436864 031.51774626381 +02.40591982080 10.9582 10.4592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53196_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53196_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:04:31.74 -00:43:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.536 2506728323389445632 031.13217374383 -00.71962799230 11.2464 10.8116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53198_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53198_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:15.10 +01:03:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.684 2508135560834014336 031.81289183209 +01.05411710318 11.4878 11.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53209_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53209_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53213_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53213_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:22.75 +00:54:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.357 2507367582026617600 032.09426731250 +00.90758647336 11.3939 10.9595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53214_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53214_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:00.25 +00:43:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.502 2508085223817316096 031.75063771932 +00.72224369648 11.5615 11.0105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53215_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53215_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53218_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53218_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 53230_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53230_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53235_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53235_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53247_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53247_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:42.69 +02:30:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.326 2514383535658892672 033.17795422917 +02.51343309069 11.7898 11.3510 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#
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Considering the candidate 53251_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53251_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53259_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53259_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53263_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53263_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:38.13 +02:39:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.697 2514401677600717824 032.90933605572 +02.66198344082 11.5190 11.0741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53270_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53270_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:07.71 +02:25:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 3.506 2514360548993901312 032.78208500571 +02.41819372960 11.3227 10.6866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53274_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53274_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:13.19 +00:50:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 3.885 2508102609844928384 031.55588659972 +00.83847744403 11.5342 11.0291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53282_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53282_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53283_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53283_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:08.51 +00:45:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.557 2508088522352199808 031.53503355533 +00.75894262816 11.4382 10.7978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53289_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53289_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53309_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53309_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53329_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53329_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53354_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53354_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53358_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53358_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53371_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53371_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:08.25 +02:45:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.346 2514594092135530496 032.78474080457 +02.76477390487 11.9168 11.5785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53376_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53376_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53377_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53377_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:45.74 +00:20:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.466 2507218361978020352 031.69025016711 +00.33537321375 11.4139 10.7916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53378_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53378_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53379_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53379_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53385_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53385_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:56.26 +02:51:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 3.676 2514595672683493120 032.73348228051 +02.85371984815 11.6800 11.0105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.676#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53420_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53420_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53422_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53422_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:22.13 +02:25:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.727 2514466200894459264 032.09172879603 +02.42599889522 11.5615 11.0563 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 53432_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53432_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:28.61 +02:31:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.713 2514480357106672512 032.11948718622 +02.51983650770 11.6078 11.1960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53436_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53436_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53444_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53444_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53449_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53449_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:25.34 +01:56:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.481 2514237055798613248 031.85467059482 +01.94193197621 11.6913 11.0860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53451_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53451_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:53.92 +01:49:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.729 2514217402028269440 032.22418808638 +01.81737664443 11.9152 11.2118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53453_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53453_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:59.46 -00:53:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 4.628 2506886515624844800 031.99903573620 -00.88453038820 11.9003 11.4480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53459_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53459_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:04.73 +01:58:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.857 2514238022166840576 032.01918170123 +01.97615019493 11.6017 11.2078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53466_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53466_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53476_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53476_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:47.88 +02:00:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 2.313 2514258496275353600 032.20003029949 +02.00663693062 11.6734 11.2979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53488_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53488_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:14.80 +02:27:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.708 2514381675937796096 033.06234713641 +02.46609981052 11.8477 11.3697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53490_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53490_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:05.24 +01:36:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.099 2508217470154704128 031.77226442100 +01.61024608780 11.8579 11.4465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53491_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53491_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53496_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53496_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53500_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53500_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:49.58 +03:08:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 4.154 2514981910502596736 033.20577001239 +03.14320872406 11.9936 11.4361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53507_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53507_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:13:27.47 +02:25:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.865 2514337150012134528 033.36464053071 +02.42028070893 12.2944 11.8402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53509_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53509_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:28.79 +02:31:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.719 2514480357106672512 032.11948718622 +02.51983650770 11.6078 11.1960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53511_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53511_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:50:05.34 -04:42:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.035 5184585594302962304 042.52308799331 -04.71074647415 13.5979 13.0642 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 53515_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53515_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:38.44 +02:39:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.999 2514401677600717824 032.90933605572 +02.66198344082 11.5190 11.0741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53516_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53516_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53520_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53520_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:32.51 +02:24:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 2.926 2514366420213761792 032.63619387220 +02.40195807093 12.1890 11.7303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53522_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53522_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53529_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53529_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:10:40.92 +02:55:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.872 2514600410031871872 032.67028589735 +02.93203025726 11.7206 11.1600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53547_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53547_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:58.92 +01:57:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.948 2514419853902228224 031.74576311790 +01.95853971376 11.6287 11.1549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53554_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53554_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:18.21 +02:33:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.441 2514481460913126784 032.07527922407 +02.55632500354 11.8027 11.2851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53560_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53560_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:05:48.76 +00:11:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.580 2507221072102180224 031.45326873858 +00.19426021121 11.7691 11.3190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53568_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53568_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:53.58 +01:08:02.8 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 53574_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53574_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:12:14.86 +02:28:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.806 2514381675937796096 033.06234713641 +02.46609981052 11.8477 11.3697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53580_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53580_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:04.35 +01:20:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 5.657 2508191395408852864 031.76968621761 +01.34167816369 11.8164 11.4566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53591_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53591_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53594_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53594_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:08:49.80 +00:54:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.350 2507365284219245184 032.20841784237 +00.91259919496 11.8251 11.3792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53595_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53595_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:44.50 +02:08:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.688 2514255339474992128 032.43557638240 +02.14263175963 11.5448 10.9118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53607_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53607_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53638_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53638_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:11:43.78 +01:38:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.659 2513427643442701056 032.93324339484 +01.63689743601 12.3518 11.8773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53642_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53642_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53647_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53647_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53648_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53648_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:09:01.50 +02:21:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.888 2514462558762192896 032.25677477464 +02.35609828922 11.9688 11.4973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53649_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53649_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53677_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53677_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53678_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53678_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53680_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53680_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53689_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53689_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 53712_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53712_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53780_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53780_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 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 53812_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53812_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53839_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 53839_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53847_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53847_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:06.84 +00:14:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 5.425 2507213512959738624 031.77991324833 +00.24705089709 12.1501 11.6651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53886_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53886_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:06:23.08 +02:54:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.616 2514556021545331968 031.59681291740 +02.91350032686 12.0135 11.4614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53985_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53985_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:07:33.37 +03:03:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.465 2514651983999998464 031.88962149643 +03.06262551224 12.1129 11.6858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53999_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 53999_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 13361_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 13361_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:41:14.17 -00:41:47.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 50030_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 50030_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 24116_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 24116_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12910_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 12910_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
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Considering the candidate 11519_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 11519_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14435_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 14435_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:32:09.52 -01:02:05.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 34350_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 34350_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:37:41.81 -03:23:41.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 13840_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 13840_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:22:12.64 -00:53:05.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 09237_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 09237_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:21:56.91 +00:23:44.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20433_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067
The candidate 20433_Cet-04-Q2b1x1_2026-02-21_21-23-16_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 02:19:21.47 -02:58:39.6 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 11s
make_report_in_HTML.sh TOTAL: 283s
Prepared the HTML report for the field Cet-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:05:34.62 -05:59:47.7
02:07:59.19 -02:17:33.2
02:15:16.47 +02:22:34.2
02:06:39.03 +03:06:12.1
02:14:46.59 +02:13:55.3
02:13:13.49 +01:07:24.9
02:14:51.16 +02:31:17.6
02:05:42.86 +01:53:20.2
02:08:20.95 +03:03:22.5
02:05:17.62 +02:57:27.3
02:17:51.12 +02:22:28.9
02:06:48.57 +02:51:54.0
02:26:02.51 -00:10:43.0
02:42:35.88 -03:04:22.9
02:12:19.82 +00:21:09.1
02:08:35.45 -06:11:42.5
02:04:58.17 -03:28:45.4
02:05:33.28 -05:40:38.6
02:04:01.36 -05:50:56.0
02:09:34.78 -05:13:27.2
02:03:18.43 -02:52:48.5
02:02:54.01 -04:34:01.4
02:03:34.39 -02:32:25.0
02:03:15.23 -06:08:28.4
02:06:23.81 -05:41:01.4
02:03:51.42 -04:53:20.5
02:07:37.04 -02:04:47.5
02:05:07.73 -03:19:24.8
02:16:21.28 -06:27:26.4
02:06:38.21 -05:35:47.1
02:04:57.05 -05:23:32.7
02:09:52.95 -04:14:07.4
02:03:57.98 -03:39:57.3
02:06:18.17 -01:42:37.2
02:13:23.91 +02:07:14.7
02:02:51.98 -04:20:39.0
02:07:05.30 -01:17:37.8
02:03:49.71 -03:58:42.0
02:06:50.99 -03:24:13.3
02:05:43.55 -04:20:49.3
02:08:53.52 -05:46:32.5
02:08:07.10 -04:50:40.1
02:06:46.63 +01:08:57.6
02:12:20.10 +00:32:21.8
02:15:36.88 +02:28:03.1
02:08:17.92 -01:43:10.5
02:05:38.22 -00:56:42.3
02:03:36.50 -01:03:38.3
02:11:15.84 +02:37:21.0
02:07:05.27 +00:21:09.3
02:14:34.82 +02:04:49.4
02:03:41.23 -02:12:51.2
02:04:09.82 -01:41:01.3
02:10:27.38 -00:39:00.6
02:18:46.79 +02:41:22.7
02:12:44.89 +02:07:41.5
02:07:03.66 -01:33:37.0
02:12:53.27 +00:05:38.8
02:11:32.52 +01:47:52.9
02:19:48.46 +02:51:38.4
02:09:15.25 +00:53:28.3
02:05:38.22 +00:31:20.2
02:10:11.82 +01:25:32.7
02:13:19.41 +03:03:40.5
02:03:50.18 -00:32:25.5
02:10:06.73 +02:12:27.4
02:10:29.04 +02:38:39.4
02:05:04.89 -00:54:51.7
02:11:49.95 +01:43:49.0
02:06:03.96 +02:18:57.9
02:04:37.54 +00:05:58.9
02:09:05.56 +03:05:11.2
02:04:35.13 +00:50:27.5
02:13:13.77 +02:28:31.8
02:08:31.20 -00:12:45.2
02:09:42.80 +03:04:57.3
02:09:49.97 +01:26:58.4
02:08:44.02 +01:58:36.3
02:14:12.01 +02:43:00.8
02:04:40.32 +01:07:20.2
02:09:01.05 +02:47:46.4
02:06:37.73 +02:56:03.0
02:20:37.10 +02:50:46.8
02:10:14.98 +02:23:35.9
02:08:36.83 -05:08:56.7
02:03:48.78 -02:03:44.5
02:07:43.23 +00:38:52.4
02:06:31.73 +02:57:38.4
02:11:17.23 +01:39:01.3
02:07:42.77 +00:38:29.0
02:06:58.61 +01:57:34.2
02:06:07.32 +01:24:51.5
02:05:50.68 +02:48:36.1
02:03:02.08 -02:59:47.2
02:15:26.65 +02:36:11.7
02:10:02.88 +02:56:35.3
02:06:03.94 +02:51:18.5
02:06:03.76 +02:51:15.6
02:06:06.20 +02:29:01.2
02:08:34.80 +01:08:56.4
02:05:36.73 +01:10:22.4
02:07:20.07 +03:08:17.6
02:12:29.28 +00:48:34.9
02:06:22.17 +02:54:48.0
02:13:06.70 +01:58:24.2
02:12:56.14 +01:58:01.7
02:07:31.96 +03:03:50.3
02:05:06.46 +02:03:54.6
########### Completed Cet-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 ####
02:05:34.62 -05:59:47.7
02:07:59.19 -02:17:33.2
02:15:16.47 +02:22:34.2
02:06:39.03 +03:06:12.1
02:14:46.59 +02:13:55.3
02:13:13.49 +01:07:24.9
02:14:51.16 +02:31:17.6
02:05:42.86 +01:53:20.2
02:08:20.95 +03:03:22.5
02:05:17.62 +02:57:27.3
02:17:51.12 +02:22:28.9
02:06:48.57 +02:51:54.0
02:08:35.45 -06:11:42.5
02:04:58.17 -03:28:45.4
02:05:33.28 -05:40:38.6
02:04:01.36 -05:50:56.0
02:09:34.78 -05:13:27.2
02:03:18.43 -02:52:48.5
02:02:54.01 -04:34:01.4
02:03:34.39 -02:32:25.0
02:03:15.23 -06:08:28.4
02:06:23.81 -05:41:01.4
02:03:51.42 -04:53:20.5
02:07:37.04 -02:04:47.5
02:05:07.73 -03:19:24.8
02:16:21.28 -06:27:26.4
02:06:38.21 -05:35:47.1
02:04:57.05 -05:23:32.7
02:09:52.95 -04:14:07.4
02:03:57.98 -03:39:57.3
02:06:18.17 -01:42:37.2
02:13:23.91 +02:07:14.7
02:02:51.98 -04:20:39.0
02:07:05.30 -01:17:37.8
02:03:49.71 -03:58:42.0
02:06:50.99 -03:24:13.3
02:05:43.55 -04:20:49.3
02:08:53.52 -05:46:32.5
02:08:07.10 -04:50:40.1
02:06:46.63 +01:08:57.6
02:12:20.10 +00:32:21.8
02:15:36.88 +02:28:03.1
02:08:17.92 -01:43:10.5
02:05:38.22 -00:56:42.3
02:03:36.50 -01:03:38.3
02:11:15.84 +02:37:21.0
02:07:05.27 +00:21:09.3
02:14:34.82 +02:04:49.4
02:03:41.23 -02:12:51.2
02:04:09.82 -01:41:01.3
02:10:27.38 -00:39:00.6
02:18:46.79 +02:41:22.7
02:12:44.89 +02:07:41.5
02:07:03.66 -01:33:37.0
02:12:53.27 +00:05:38.8
02:11:32.52 +01:47:52.9
02:19:48.46 +02:51:38.4
02:09:15.25 +00:53:28.3
02:05:38.22 +00:31:20.2
02:10:11.82 +01:25:32.7
02:13:19.41 +03:03:40.5
02:03:50.18 -00:32:25.5
02:10:06.73 +02:12:27.4
02:10:29.04 +02:38:39.4
02:05:04.89 -00:54:51.7
02:11:49.95 +01:43:49.0
02:06:03.96 +02:18:57.9
02:04:37.54 +00:05:58.9
02:09:05.56 +03:05:11.2
02:04:35.13 +00:50:27.5
02:13:13.77 +02:28:31.8
02:08:31.20 -00:12:45.2
02:09:42.80 +03:04:57.3
02:09:49.97 +01:26:58.4
02:08:44.02 +01:58:36.3
02:14:12.01 +02:43:00.8
02:04:40.32 +01:07:20.2
02:09:01.05 +02:47:46.4
02:06:37.73 +02:56:03.0
02:20:37.10 +02:50:46.8
02:10:14.98 +02:23:35.9
02:08:36.83 -05:08:56.7
02:03:48.78 -02:03:44.5
02:07:43.23 +00:38:52.4
02:06:31.73 +02:57:38.4
02:11:17.23 +01:39:01.3
02:07:42.77 +00:38:29.0
02:06:58.61 +01:57:34.2
02:06:07.32 +01:24:51.5
02:05:50.68 +02:48:36.1
02:03:02.08 -02:59:47.2
02:15:26.65 +02:36:11.7
02:10:02.88 +02:56:35.3
02:06:03.94 +02:51:18.5
02:06:03.76 +02:51:15.6
02:06:06.20 +02:29:01.2
02:08:34.80 +01:08:56.4
02:05:36.73 +01:10:22.4
02:07:20.07 +03:08:17.6
02:12:29.28 +00:48:34.9
02:06:22.17 +02:54:48.0
02:13:06.70 +01:58:24.2
02:12:56.14 +01:58:01.7
02:07:31.96 +03:03:50.3
02:05:06.46 +02:03:54.6
02:12:19.82 +00:21:09.1
02:42:35.88 -03:04:22.9
02:26:02.51 -00:10:43.0
###################################################################################
02:05:34.62 -05:59:47.7 -- not an asteroid (will add it to exclusion list)
02:07:59.19 -02:17:33.2 -- not an asteroid (will add it to exclusion list)
02:15:16.47 +02:22:34.2 -- not an asteroid (will add it to exclusion list)
02:06:39.03 +03:06:12.1 -- not an asteroid (will add it to exclusion list)
02:14:46.59 +02:13:55.3 -- not an asteroid (will add it to exclusion list)
02:13:13.49 +01:07:24.9 -- not an asteroid (will add it to exclusion list)
02:14:51.16 +02:31:17.6 -- not an asteroid (will add it to exclusion list)
02:05:42.86 +01:53:20.2 -- not an asteroid (will add it to exclusion list)
02:08:20.95 +03:03:22.5 -- not an asteroid (will add it to exclusion list)
02:05:17.62 +02:57:27.3 -- not an asteroid (will add it to exclusion list)
02:17:51.12 +02:22:28.9 -- not an asteroid (will add it to exclusion list)
02:06:48.57 +02:51:54.0 -- not an asteroid (will add it to exclusion list)
02:08:35.45 -06:11:42.5 -- not an asteroid (will add it to exclusion list)
02:04:58.17 -03:28:45.4 -- not an asteroid (will add it to exclusion list)
02:05:33.28 -05:40:38.6 -- not an asteroid (will add it to exclusion list)
02:04:01.36 -05:50:56.0 -- not an asteroid (will add it to exclusion list)
02:09:34.78 -05:13:27.2 -- not an asteroid (will add it to exclusion list)
02:03:18.43 -02:52:48.5 -- not an asteroid (will add it to exclusion list)
02:02:54.01 -04:34:01.4 -- not an asteroid (will add it to exclusion list)
02:03:34.39 -02:32:25.0 -- not an asteroid (will add it to exclusion list)
02:03:15.23 -06:08:28.4 -- not an asteroid (will add it to exclusion list)
02:06:23.81 -05:41:01.4 -- not an asteroid (will add it to exclusion list)
02:03:51.42 -04:53:20.5 -- not an asteroid (will add it to exclusion list)
02:07:37.04 -02:04:47.5 -- not an asteroid (will add it to exclusion list)
02:05:07.73 -03:19:24.8 -- not an asteroid (will add it to exclusion list)
02:16:21.28 -06:27:26.4 -- not an asteroid (will add it to exclusion list)
02:06:38.21 -05:35:47.1 -- not an asteroid (will add it to exclusion list)
02:04:57.05 -05:23:32.7 -- not an asteroid (will add it to exclusion list)
02:09:52.95 -04:14:07.4 -- not an asteroid (will add it to exclusion list)
02:03:57.98 -03:39:57.3 -- not an asteroid (will add it to exclusion list)
02:06:18.17 -01:42:37.2 -- not an asteroid (will add it to exclusion list)
02:13:23.91 +02:07:14.7 -- not an asteroid (will add it to exclusion list)
02:02:51.98 -04:20:39.0 -- not an asteroid (will add it to exclusion list)
02:07:05.30 -01:17:37.8 -- not an asteroid (will add it to exclusion list)
02:03:49.71 -03:58:42.0 -- not an asteroid (will add it to exclusion list)
02:06:50.99 -03:24:13.3 -- not an asteroid (will add it to exclusion list)
02:05:43.55 -04:20:49.3 -- not an asteroid (will add it to exclusion list)
02:08:53.52 -05:46:32.5 -- not an asteroid (will add it to exclusion list)
02:08:07.10 -04:50:40.1 -- not an asteroid (will add it to exclusion list)
02:06:46.63 +01:08:57.6 -- not an asteroid (will add it to exclusion list)
02:12:20.10 +00:32:21.8 -- not an asteroid (will add it to exclusion list)
02:15:36.88 +02:28:03.1 -- not an asteroid (will add it to exclusion list)
02:08:17.92 -01:43:10.5 -- not an asteroid (will add it to exclusion list)
02:05:38.22 -00:56:42.3 -- not an asteroid (will add it to exclusion list)
02:03:36.50 -01:03:38.3 -- not an asteroid (will add it to exclusion list)
02:11:15.84 +02:37:21.0 -- not an asteroid (will add it to exclusion list)
02:07:05.27 +00:21:09.3 -- not an asteroid (will add it to exclusion list)
02:14:34.82 +02:04:49.4 -- not an asteroid (will add it to exclusion list)
02:03:41.23 -02:12:51.2 -- not an asteroid (will add it to exclusion list)
02:04:09.82 -01:41:01.3 -- not an asteroid (will add it to exclusion list)
02:10:27.38 -00:39:00.6 -- not an asteroid (will add it to exclusion list)
02:18:46.79 +02:41:22.7 -- not an asteroid (will add it to exclusion list)
02:12:44.89 +02:07:41.5 -- not an asteroid (will add it to exclusion list)
02:07:03.66 -01:33:37.0 -- not an asteroid (will add it to exclusion list)
02:12:53.27 +00:05:38.8 -- not an asteroid (will add it to exclusion list)
02:11:32.52 +01:47:52.9 -- not an asteroid (will add it to exclusion list)
02:19:48.46 +02:51:38.4 -- not an asteroid (will add it to exclusion list)
02:09:15.25 +00:53:28.3 -- not an asteroid (will add it to exclusion list)
02:05:38.22 +00:31:20.2 -- not an asteroid (will add it to exclusion list)
02:10:11.82 +01:25:32.7 -- not an asteroid (will add it to exclusion list)
02:13:19.41 +03:03:40.5 -- not an asteroid (will add it to exclusion list)
02:03:50.18 -00:32:25.5 -- not an asteroid (will add it to exclusion list)
02:10:06.73 +02:12:27.4 -- not an asteroid (will add it to exclusion list)
02:10:29.04 +02:38:39.4 -- not an asteroid (will add it to exclusion list)
02:05:04.89 -00:54:51.7 -- not an asteroid (will add it to exclusion list)
02:11:49.95 +01:43:49.0 -- not an asteroid (will add it to exclusion list)
02:06:03.96 +02:18:57.9 -- not an asteroid (will add it to exclusion list)
02:04:37.54 +00:05:58.9 -- not an asteroid (will add it to exclusion list)
02:09:05.56 +03:05:11.2 -- not an asteroid (will add it to exclusion list)
02:04:35.13 +00:50:27.5 -- not an asteroid (will add it to exclusion list)
02:13:13.77 +02:28:31.8 -- not an asteroid (will add it to exclusion list)
02:08:31.20 -00:12:45.2 -- not an asteroid (will add it to exclusion list)
02:09:42.80 +03:04:57.3 -- not an asteroid (will add it to exclusion list)
02:09:49.97 +01:26:58.4 -- not an asteroid (will add it to exclusion list)
02:08:44.02 +01:58:36.3 -- not an asteroid (will add it to exclusion list)
02:14:12.01 +02:43:00.8 -- not an asteroid (will add it to exclusion list)
02:04:40.32 +01:07:20.2 -- not an asteroid (will add it to exclusion list)
02:09:01.05 +02:47:46.4 -- not an asteroid (will add it to exclusion list)
02:06:37.73 +02:56:03.0 -- not an asteroid (will add it to exclusion list)
02:20:37.10 +02:50:46.8 -- not an asteroid (will add it to exclusion list)
02:10:14.98 +02:23:35.9 -- not an asteroid (will add it to exclusion list)
02:08:36.83 -05:08:56.7 -- not an asteroid (will add it to exclusion list)
02:03:48.78 -02:03:44.5 -- not an asteroid (will add it to exclusion list)
02:07:43.23 +00:38:52.4 -- not an asteroid (will add it to exclusion list)
02:06:31.73 +02:57:38.4 -- not an asteroid (will add it to exclusion list)
02:11:17.23 +01:39:01.3 -- not an asteroid (will add it to exclusion list)
02:07:42.77 +00:38:29.0 -- not an asteroid (will add it to exclusion list)
02:06:58.61 +01:57:34.2 -- not an asteroid (will add it to exclusion list)
02:06:07.32 +01:24:51.5 -- not an asteroid (will add it to exclusion list)
02:05:50.68 +02:48:36.1 -- not an asteroid (will add it to exclusion list)
02:03:02.08 -02:59:47.2 -- not an asteroid (will add it to exclusion list)
02:15:26.65 +02:36:11.7 -- not an asteroid (will add it to exclusion list)
02:10:02.88 +02:56:35.3 -- not an asteroid (will add it to exclusion list)
02:06:03.94 +02:51:18.5 -- not an asteroid (will add it to exclusion list)
02:06:03.76 +02:51:15.6 -- not an asteroid (will add it to exclusion list)
02:06:06.20 +02:29:01.2 -- not an asteroid (will add it to exclusion list)
02:08:34.80 +01:08:56.4 -- not an asteroid (will add it to exclusion list)
02:05:36.73 +01:10:22.4 -- not an asteroid (will add it to exclusion list)
02:07:20.07 +03:08:17.6 -- not an asteroid (will add it to exclusion list)
02:12:29.28 +00:48:34.9 -- not an asteroid (will add it to exclusion list)
02:06:22.17 +02:54:48.0 -- not an asteroid (will add it to exclusion list)
02:13:06.70 +01:58:24.2 -- not an asteroid (will add it to exclusion list)
02:12:56.14 +01:58:01.7 -- not an asteroid (will add it to exclusion list)
02:07:31.96 +03:03:50.3 -- not an asteroid (will add it to exclusion list)
02:05:06.46 +02:03:54.6 -- not an asteroid (will add it to exclusion list)
02:12:19.82 +00:21:09.1 -- not an asteroid (will add it to exclusion list)
02:42:35.88 -03:04:22.9 -- not an asteroid (will add it to exclusion list)
02:26:02.51 -00:10:43.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
02:02:51.98 -04:20:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:54.01 -04:34:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:02.08 -02:59:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:15.23 -06:08:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:18.43 -02:52:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:34.39 -02:32:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:36.50 -01:03:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:41.23 -02:12:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:48.78 -02:03:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:49.71 -03:58:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:50.18 -00:32:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:51.42 -04:53:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:57.98 -03:39:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:01.36 -05:50:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:09.82 -01:41:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:35.13 +00:50:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:37.54 +00:05:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:40.32 +01:07:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:57.05 -05:23:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:58.17 -03:28:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:04.89 -00:54:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:06.46 +02:03:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:07.73 -03:19:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:17.62 +02:57:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:33.28 -05:40:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:34.62 -05:59:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:36.73 +01:10:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:38.22 +00:31:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:38.22 -00:56:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:42.86 +01:53:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:43.55 -04:20:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:50.68 +02:48:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:03.76 +02:51:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:03.94 +02:51:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:03.96 +02:18:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:06.20 +02:29:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:07.32 +01:24:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:18.17 -01:42:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:22.17 +02:54:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:23.81 -05:41:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:31.73 +02:57:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:37.73 +02:56:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:38.21 -05:35:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:39.03 +03:06:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:46.63 +01:08:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:48.57 +02:51:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:50.99 -03:24:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:06:58.61 +01:57:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:03.66 -01:33:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:05.27 +00:21:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:05.30 -01:17:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:20.07 +03:08:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:31.96 +03:03:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:37.04 -02:04:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:42.77 +00:38:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:43.23 +00:38:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:59.19 -02:17:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:07.10 -04:50:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:17.92 -01:43:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:20.95 +03:03:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:31.20 -00:12:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:34.80 +01:08:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:35.45 -06:11:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:36.83 -05:08:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:44.02 +01:58:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:53.52 -05:46:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:01.05 +02:47:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:05.56 +03:05:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:15.25 +00:53:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:34.78 -05:13:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:42.80 +03:04:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:49.97 +01:26:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:52.95 -04:14:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:02.88 +02:56:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:06.73 +02:12:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:11.82 +01:25:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:14.98 +02:23:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:27.38 -00:39:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:29.04 +02:38:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:15.84 +02:37:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:17.23 +01:39:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:32.52 +01:47:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:49.95 +01:43:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:19.82 +00:21:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:20.10 +00:32:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:29.28 +00:48:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:44.89 +02:07:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:53.27 +00:05:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:56.14 +01:58:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:06.70 +01:58:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:13.49 +01:07:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:13.77 +02:28:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:19.41 +03:03:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:23.91 +02:07:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:12.01 +02:43:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:34.82 +02:04:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:46.59 +02:13:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:51.16 +02:31:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:16.47 +02:22:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:26.65 +02:36:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:36.88 +02:28:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:21.28 -06:27:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:51.12 +02:22:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:46.79 +02:41:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:48.46 +02:51:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:37.10 +02:50:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:02.51 -00:10:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:42:35.88 -03:04:22.9 -- 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)
02:02:51.98 -04:20:39.0 -- not a known variable star
02:02:54.01 -04:34:01.4 -- not a known variable star
02:03:02.08 -02:59:47.2 -- not a known variable star
02:03:15.23 -06:08:28.4 -- not a known variable star
02:03:18.43 -02:52:48.5 -- not a known variable star
02:03:34.39 -02:32:25.0 -- not a known variable star
02:03:36.50 -01:03:38.3 -- not a known variable star
02:03:41.23 -02:12:51.2 -- not a known variable star
02:03:48.78 -02:03:44.5 -- not a known variable star
02:03:49.71 -03:58:42.0 -- not a known variable star
02:03:50.18 -00:32:25.5 -- not a known variable star
02:03:51.42 -04:53:20.5 -- not a known variable star
02:03:57.98 -03:39:57.3 -- not a known variable star
02:04:01.36 -05:50:56.0 -- not a known variable star
02:04:09.82 -01:41:01.3 -- not a known variable star
02:04:35.13 +00:50:27.5 -- not a known variable star
02:04:37.54 +00:05:58.9 -- not a known variable star
02:04:40.32 +01:07:20.2 -- not a known variable star
02:04:57.05 -05:23:32.7 -- not a known variable star
02:04:58.17 -03:28:45.4 -- not a known variable star
02:05:04.89 -00:54:51.7 -- not a known variable star
02:05:06.46 +02:03:54.6 -- not a known variable star
02:05:07.73 -03:19:24.8 -- not a known variable star
02:05:17.62 +02:57:27.3 -- a known variable star
02:05:33.28 -05:40:38.6 -- not a known variable star
02:05:34.62 -05:59:47.7 -- not a known variable star
02:05:36.73 +01:10:22.4 -- not a known variable star
02:05:38.22 +00:31:20.2 -- not a known variable star
02:05:38.22 -00:56:42.3 -- not a known variable star
02:05:42.86 +01:53:20.2 -- not a known variable star
02:05:43.55 -04:20:49.3 -- not a known variable star
02:05:50.68 +02:48:36.1 -- not a known variable star
02:06:03.76 +02:51:15.6 -- not a known variable star
02:06:03.94 +02:51:18.5 -- not a known variable star
02:06:03.96 +02:18:57.9 -- not a known variable star
02:06:06.20 +02:29:01.2 -- not a known variable star
02:06:07.32 +01:24:51.5 -- not a known variable star
02:06:18.17 -01:42:37.2 -- not a known variable star
02:06:22.17 +02:54:48.0 -- not a known variable star
02:06:23.81 -05:41:01.4 -- not a known variable star
02:06:31.73 +02:57:38.4 -- not a known variable star
02:06:37.73 +02:56:03.0 -- not a known variable star
02:06:38.21 -05:35:47.1 -- not a known variable star
02:06:39.03 +03:06:12.1 -- not a known variable star
02:06:46.63 +01:08:57.6 -- not a known variable star
02:06:48.57 +02:51:54.0 -- not a known variable star
02:06:50.99 -03:24:13.3 -- not a known variable star
02:06:58.61 +01:57:34.2 -- not a known variable star
02:07:03.66 -01:33:37.0 -- not a known variable star
02:07:05.27 +00:21:09.3 -- not a known variable star
02:07:05.30 -01:17:37.8 -- not a known variable star
02:07:20.07 +03:08:17.6 -- not a known variable star
02:07:31.96 +03:03:50.3 -- not a known variable star
02:07:37.04 -02:04:47.5 -- not a known variable star
02:07:42.77 +00:38:29.0 -- not a known variable star
02:07:43.23 +00:38:52.4 -- not a known variable star
02:07:59.19 -02:17:33.2 -- not a known variable star
02:08:07.10 -04:50:40.1 -- not a known variable star
02:08:17.92 -01:43:10.5 -- not a known variable star
02:08:20.95 +03:03:22.5 -- not a known variable star
02:08:31.20 -00:12:45.2 -- not a known variable star
02:08:34.80 +01:08:56.4 -- not a known variable star
02:08:35.45 -06:11:42.5 -- not a known variable star
02:08:36.83 -05:08:56.7 -- not a known variable star
02:08:44.02 +01:58:36.3 -- not a known variable star
02:08:53.52 -05:46:32.5 -- not a known variable star
02:09:01.05 +02:47:46.4 -- not a known variable star
02:09:05.56 +03:05:11.2 -- not a known variable star
02:09:15.25 +00:53:28.3 -- not a known variable star
02:09:34.78 -05:13:27.2 -- not a known variable star
02:09:42.80 +03:04:57.3 -- not a known variable star
02:09:49.97 +01:26:58.4 -- not a known variable star
02:09:52.95 -04:14:07.4 -- not a known variable star
02:10:02.88 +02:56:35.3 -- not a known variable star
02:10:06.73 +02:12:27.4 -- not a known variable star
02:10:11.82 +01:25:32.7 -- not a known variable star
02:10:14.98 +02:23:35.9 -- not a known variable star
02:10:27.38 -00:39:00.6 -- not a known variable star
02:10:29.04 +02:38:39.4 -- not a known variable star
02:11:15.84 +02:37:21.0 -- not a known variable star
02:11:17.23 +01:39:01.3 -- not a known variable star
02:11:32.52 +01:47:52.9 -- not a known variable star
02:11:49.95 +01:43:49.0 -- not a known variable star
02:12:19.82 +00:21:09.1 -- not a known variable star
02:12:20.10 +00:32:21.8 -- not a known variable star
02:12:29.28 +00:48:34.9 -- not a known variable star
02:12:44.89 +02:07:41.5 -- not a known variable star
02:12:53.27 +00:05:38.8 -- not a known variable star
02:12:56.14 +01:58:01.7 -- not a known variable star
02:13:06.70 +01:58:24.2 -- not a known variable star
02:13:13.49 +01:07:24.9 -- a known variable star
02:13:13.77 +02:28:31.8 -- not a known variable star
02:13:19.41 +03:03:40.5 -- not a known variable star
02:13:23.91 +02:07:14.7 -- not a known variable star
02:14:12.01 +02:43:00.8 -- not a known variable star
02:14:34.82 +02:04:49.4 -- not a known variable star
02:14:46.59 +02:13:55.3 -- not a known variable star
02:14:51.16 +02:31:17.6 -- not a known variable star
02:15:16.47 +02:22:34.2 -- not a known variable star
02:15:26.65 +02:36:11.7 -- not a known variable star
02:15:36.88 +02:28:03.1 -- not a known variable star
02:16:21.28 -06:27:26.4 -- not a known variable star
02:17:51.12 +02:22:28.9 -- a known variable star
02:18:46.79 +02:41:22.7 -- not a known variable star
02:19:48.46 +02:51:38.4 -- a known variable star
02:20:37.10 +02:50:46.8 -- not a known variable star
02:26:02.51 -00:10:43.0 -- a known variable star
02:42:35.88 -03:04:22.9 -- a known variable star
Found 102 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
108 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)2461093.64077693 -observatory 500
23:23:22.77 -01:59:40.0 Mercury (-0.1mag)
23:04:20.34 -07:30:37.3 Venus (-3.9mag)
21:42:43.72 -14:53:15.6 Mars (1.1mag)
07:06:06.40 +22:54:19.3 Jupiter (-2.5mag)
00:05:25.49 -01:44:32.6 Saturn (1.0mag)
03:39:59.39 +19:21:43.3 Uranus (5.7mag)
00:03:40.69 -01:01:38.7 Neptune (7.8mag)
20:29:06.85 -22:59:34.6 Pluto (14.5mag)
01:52:48.44 +16:06:09.4 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 22 04:03 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461093.64077693:
07:06:10.08 +22:54:14.7 Io (5.4mag)
07:06:17.72 +22:53:58.6 Europa (5.5mag)
07:05:56.86 +22:54:45.4 Ganymede (4.9mag)
07:06:25.22 +22:53:54.3 Callisto (6.2mag)
07:09:15.27 +23:10:42.8 Himalia (15.0mag)
07:06:07.19 +22:54:20.2 Thebe (15.9mag)
07:08:40.37 +23:19:10.7 Elara (17.0mag)
07:01:39.89 +24:02:18.2 Pasiphae (17.0mag)
07:15:07.30 +22:42:18.9 Carme (18.1mag)
00:05:37.17 -01:44:37.3 Titan (8.8mag)
00:05:30.93 -01:44:31.3 Rhea (10.1mag)
00:05:20.84 -01:45:53.7 Iapetus (11.5mag)
00:05:26.26 -01:44:35.6 Hyperion (14.8mag)
00:07:29.77 -01:31:32.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 22 04:03 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.64077693:
08:45:40.56 +24:30:42.1 JWST
11:18:21.02 +46:52:16.1 Chandra
15:14:02.23 -60:28:59.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 22 04:03 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)2461093.64077693 at 500
16:59:40.03 -11:03:48.6 17.5mag 10P/Tempel 2
03:37:17.95 +28:57:46.5 18.0mag 123P/West-Hartley
08:23:40.05 +60:43:09.1 18.4mag 124P/Mrkos
21:19:31.88 -07:39:00.8 22.1mag 141P/Machholz
01:21:07.12 +11:54:37.0 17.6mag 145P/Shoemaker-Levy 5
11:02:59.81 +30:34:26.7 17.9mag 164P/Christensen
09:33:08.42 -33:51:50.2 18.0mag 195P/Hill
15:52:03.32 -06:35:57.8 19.2mag 210P/Christensen
18:16:47.62 -21:28:33.6 17.3mag 218P/LINEAR
16:21:32.75 -18:10:57.5 15.2mag 235P/LINEAR
03:56:22.18 +27:44:21.7 17.8mag 240P/NEAT
15:17:36.83 +06:38:28.7 14.8mag 24P/Schaumasse
11:23:31.41 -03:23:10.9 17.4mag 29P/Schwassmann-Wachmann 1
07:03:47.96 +27:24:49.7 19.6mag 407P/PanSTARRS-Fuls
17:07:07.40 -11:19:14.6 17.6mag 40P/Vaisala 1
11:02:13.39 -08:51:55.7 16.6mag 43P/Wolf-Harrington
13:25:29.69 -05:49:36.6 20.0mag 489P/Denning
04:34:21.50 +48:34:37.9 17.8mag 493P/2024 Q2 (LONEOS)
06:04:22.86 +47:31:36.6 17.7mag 63P/Wild 1
23:14:34.92 -02:07:39.7 16.2mag 78P/Gehrels 2
20:01:27.29 -22:18:25.0 15.0mag 88P/Howell
15:27:54.27 -29:00:37.1 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.04 -72:35:57.0 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:50.10 +31:12:54.0 18.2mag C/2017 K2 (PanSTARRS)
20:06:37.82 -65:11:36.7 18.1mag C/2020 V2 (ZTF)
17:21:40.09 +04:21:18.2 16.3mag C/2021 G2 (ATLAS)
03:35:40.39 +24:36:41.3 15.8mag C/2022 N2 (PanSTARRS)
09:08:13.51 +29:49:30.8 15.3mag C/2022 QE78 (ATLAS)
08:35:40.79 -06:33:52.5 16.7mag C/2022 R6 (PanSTARRS)
23:53:01.22 +48:26:43.7 18.0mag C/2023 C2 (ATLAS)
09:51:08.65 -20:46:05.7 17.5mag C/2023 F3 (ATLAS)
20:34:43.81 +61:14:30.9 17.3mag C/2023 H5 (Lemmon)
19:34:30.04 -03:24:15.5 16.1mag C/2023 R1 (PANSTARRS)
02:48:55.03 +35:40:34.6 18.5mag C/2023 RS61 (PanSTARRS)
21:01:25.84 +81:19:55.6 18.0mag C/2023 X2 (Lemmon)
06:39:10.81 +63:49:12.4 17.3mag C/2024 A1 (ATLAS)
01:56:39.99 -24:38:48.8 11.2mag C/2024 E1 (Wierzchos)
11:44:59.26 -02:34:59.1 18.1mag C/2024 G2 (ATLAS)
19:28:18.31 +00:39:11.1 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.75 -01:42:58.4 17.7mag C/2024 G6 (ATLAS)
19:53:27.10 +03:14:59.1 15.6mag C/2024 J3 (ATLAS)
02:47:14.23 -31:34:36.8 15.4mag C/2024 T5 (ATLAS)
16:25:07.96 -58:13:32.5 15.6mag C/2025 A6 (Lemmon)
04:50:29.63 +62:14:47.3 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)
15:56:43.92 -13:01:51.0 14.8mag C/2025 L1 (ATLAS)
02:20:13.49 -19:05:52.3 16.7mag C/2025 Q3 (ATLAS)
02:09:33.63 +17:16:40.1 21.2mag C/2025 R2 (SWAN)
22:20:45.61 +17:39:13.7 16.4mag C/2025 R3 (PANSTARRS)
21:46:00.52 -16:50:16.4 21.5mag C/2025 T1 (ATLAS)
03:06:16.00 -20:34:21.7 18.3mag C/2026 A1 (MAPS)
21:02:59.40 +20:55:19.3 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 22 04:04 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 04:03 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
-rw-r--r-- 1 apache apache 187K Feb 22 04:03 tocp_transients_list.txt