This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY
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 09 06.2513 2461289.7513 11.10 05:01:33.32 +42:10:38.4
164.04245 0.10980 galactic Aur Second-epoch detections are separated by 0.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.3889+42.1774 | 05:01:33.35 +42:10:38.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.790+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:33.32 +42:10:38.4: 12.06 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:33.32 +42:10:38.4: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.3889+42.1774,2461289.7513,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.3889+42.1774 20260906.2513 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.87 04:53:06.39 +40:35:50.9
164.29050 -2.11395 galactic Aur Second-epoch detections are separated by 1.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.2765+40.5972 | 04:53:06.37 +40:35:50.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.790+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:06.39 +40:35:50.9: 12.72 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:06.39 +40:35:50.9: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.2765+40.5972,2461289.7513,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J073.2765+40.5972 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.80 04:56:20.68 +41:43:23.9
163.79857 -0.93195 galactic Aur Second-epoch detections are separated by 0.5" and 7.3 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 201871125135870464 | 04:56:17.45 +41:43:14.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.733+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:20.68 +41:43:23.9: 12.76 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:20.68 +41:43:23.9: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201871125135870464,2461289.7513,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201871125135870464 20260906.2513 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.86 05:00:58.13 +41:53:30.8
164.20081 -0.15147 galactic Aur Second-epoch detections are separated by 2.6" and 7.3 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 J075.2389+41.8929 | 05:00:58.13 +41:53:30.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.662+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:58.13 +41:53:30.8: 12.86 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:58.13 +41:53:30.8: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.2389+41.8929,2461289.7513,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.2389+41.8929 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.46 04:55:09.88 +40:33:03.2
164.57315 -1.83987 galactic Aur Second-epoch detections are separated by 2.7" and 7.0 pix
The object was found in VSX 2" NSVS J0455100+403305
Type: L:
# Max. Min./Amp. JD0 Period
10.866 R1 Y 0.543 R1 586.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:09.88 +40:33:03.2: 12.88 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:09.88 +40:33:03.2: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0455100+403305,2461289.7513,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0455100+403305 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.35 03:48:10.95 +41:57:18.6
154.66510 -9.77361 galactic Per Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:48:10.95 +41:57:18.6 (user input) | T | P | (position from user input) J-Ks=0.320+/-0.032 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:48:10.95 +41:57:18.6: 13.23 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:48:10.95 +41:57:18.6: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 48 10.95 +41 57 18.6 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.06 05:01:36.22 +42:07:32.6
164.08871 0.08521 galactic Aur Second-epoch detections are separated by 1.5" and 7.6 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 | target | 05:01:36.22 +42:07:32.6 (user input) | T | P | (position from user input) J-Ks=0.308+/-0.032 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:36.22 +42:07:32.6: 13.36 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:36.22 +42:07:32.6: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.58 03:51:04.96 +42:11:55.7
154.93112 -9.24433 galactic Per Second-epoch detections are separated by 2.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:04.96 +42:11:55.7 (user input) | T | P | (position from user input) J-Ks=0.696+/-0.033 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:04.96 +42:11:55.7: 13.85 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:04.96 +42:11:55.7: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 04.96 +42 11 55.7 12.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.68 03:53:49.46 +42:15:40.9
155.28543 -8.87142 galactic Per Second-epoch detections are separated by 0.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:53:49.46 +42:15:40.9 (user input) | T | P | (position from user input) J-Ks=1.285+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:53:49.46 +42:15:40.9: 13.77 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:53:49.46 +42:15:40.9: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 53 49.46 +42 15 40.9 12.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.52 03:49:35.78 +40:31:27.6
155.79381 -10.71395 galactic Per Second-epoch detections are separated by 3.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:49:35.78 +40:31:27.6 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.446+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:49:35.78 +40:31:27.6: 13.75 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:49:35.78 +40:31:27.6: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 49 35.78 +40 31 27.6 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.54 03:48:13.22 +40:09:25.5
155.82435 -11.16420 galactic Per Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:48:13.22 +40:09:25.5 (user input) | T | P | (position from user input) J-Ks=0.790+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:48:13.22 +40:09:25.5: 13.70 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:48:13.22 +40:09:25.5: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 48 13.22 +40 09 25.5 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.52 03:50:49.99 +41:45:03.2
155.18393 -9.61928 galactic Per Second-epoch detections are separated by 4.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 231042925263540352 | 03:50:52.61 +41:45:32.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:50:49.99 +41:45:03.2: 13.62 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:50:49.99 +41:45:03.2: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 50 49.99 +41 45 03.2 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 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 231042925263540352,2461289.7513,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 231042925263540352 20260906.2513 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.58 03:51:12.19 +42:07:35.2
154.99526 -9.28590 galactic Per Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J057.7887+42.1218 | 03:51:12.19 +42:07:35.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.738+/-0.032 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:12.19 +42:07:35.2: 13.64 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:12.19 +42:07:35.2: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 12.19 +42 07 35.2 12.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.7887+42.1218,2461289.7513,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J057.7887+42.1218 20260906.2513 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.47 03:47:57.54 +41:46:17.6
154.74955 -9.94249 galactic Per Second-epoch detections are separated by 2.1" and 6.6 pix
The object was found in VSX 3" Gaia DR3 231149229998410112
Type: ROT
# Max. Min./Amp. JD0 Period
15.330 G 15.360 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:57.54 +41:46:17.6: 13.61 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:57.54 +41:46:17.6: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 47 57.54 +41 46 17.6 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 231149229998410112,2461289.7513,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 231149229998410112 20260906.2513 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.24 04:58:17.08 +41:15:54.7
164.38331 -0.93339 galactic Aur Second-epoch detections are separated by 2.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5696+41.2573 | 04:58:17.08 +41:15:54.7 (user input) | CBH (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.003+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:17.08 +41:15:54.7: 13.57 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:17.08 +41:15:54.7: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.5696+41.2573,2461289.7513,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.5696+41.2573 20260906.2513 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.55 03:51:22.81 +41:49:40.8
155.21378 -9.49488 galactic Per Second-epoch detections are separated by 1.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:22.81 +41:49:40.8 (user input) | T | P | (position from user input) J-Ks=0.958+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:22.81 +41:49:40.8: 13.60 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:22.81 +41:49:40.8: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 22.81 +41 49 40.8 12.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.43 03:48:48.30 +42:19:43.5
154.51730 -9.41078 galactic Per Second-epoch detections are separated by 3.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:48:48.30 +42:19:43.5 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.479+/-0.033 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:48:48.30 +42:19:43.5: 13.54 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:48:48.30 +42:19:43.5: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 48 48.30 +42 19 43.5 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.39 03:51:34.91 +40:20:52.4
156.20440 -10.60878 galactic Per Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:34.91 +40:20:52.4 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.031 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:34.91 +40:20:52.4: 13.53 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:34.91 +40:20:52.4: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 34.91 +40 20 52.4 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.43 03:52:12.95 +41:28:22.4
155.56573 -9.66818 galactic Per Second-epoch detections are separated by 1.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:52:12.95 +41:28:22.4 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.032 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:12.95 +41:28:22.4: 13.51 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:12.95 +41:28:22.4: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 12.95 +41 28 22.4 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.41 03:51:22.42 +39:38:05.9
156.63859 -11.18154 galactic Per Second-epoch detections are separated by 1.7" and 7.0 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 | target | 03:51:22.42 +39:38:05.9 (user input) | T | P | (position from user input) J-Ks=0.529+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:22.42 +39:38:05.9: 13.50 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:22.42 +39:38:05.9: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 22.42 +39 38 05.9 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.50 03:45:53.65 +40:56:32.0
154.97144 -10.83147 galactic Per Second-epoch detections are separated by 3.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:45:53.65 +40:56:32.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.386+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:53.65 +40:56:32.0: 13.51 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:53.65 +40:56:32.0: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 45 53.65 +40 56 32.0 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.47 03:51:06.48 +42:26:37.5
154.77687 -9.05242 galactic Per Second-epoch detections are separated by 1.6" and 6.8 pix
The object was found in VSX18" Gaia DR3 231263549145600256
Type: S
# Max. Min./Amp. JD0 Period
16.280 G 17.580 G F
ATTENTION: measured mag 12.47 is 3.8 mag brighter than the VSX record maximum brightness 16.28 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:06.48 +42:26:37.5: 13.50 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:06.48 +42:26:37.5: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 06.48 +42 26 37.5 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 231263549145600256,2461289.7513,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 231263549145600256 20260906.2513 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.36 03:50:58.79 +41:54:33.5
155.10301 -9.47973 galactic Per Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:50:58.79 +41:54:33.5 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.336+/-0.031 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:50:58.79 +41:54:33.5: 13.48 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:50:58.79 +41:54:33.5: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 50 58.79 +41 54 33.5 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.46 03:48:43.39 +40:25:57.3
155.72237 -10.89020 galactic Per Second-epoch detections are separated by 0.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:48:43.39 +40:25:57.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.521+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:48:43.39 +40:25:57.3: 13.44 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:48:43.39 +40:25:57.3: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 48 43.39 +40 25 57.3 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.46CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.43 03:51:42.29 +39:24:03.1
156.84175 -11.32005 galactic Per Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:42.29 +39:24:03.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=1.117+/-0.030 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:42.29 +39:24:03.1: 13.45 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:42.29 +39:24:03.1: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 42.29 +39 24 03.1 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.43 03:54:01.48 +42:24:58.9
155.21314 -8.72897 galactic Per Second-epoch detections are separated by 1.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:54:01.48 +42:24:58.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:54:01.48 +42:24:58.9: 13.43 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:54:01.48 +42:24:58.9: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 54 01.48 +42 24 58.9 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.43 03:52:26.94 +40:24:09.8
156.29744 -10.46074 galactic Per Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 varaible 230064462992497792 | 03:52:26.94 +40:24:09.8 (user input) | AGN (Gaia DR3) | 2022yCat.1358....0G | (position from user input) Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: F0 (LAMOST DR5) J-Ks=0.465+/-0.037 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:26.94 +40:24:09.8: 13.44 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:26.94 +40:24:09.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 26.94 +40 24 09.8 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 varaible 230064462992497792,2461289.7513,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 varaible 230064462992497792 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.43 03:52:40.18 +40:13:30.4
156.44639 -10.56969 galactic Per Second-epoch detections are separated by 0.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:52:40.18 +40:13:30.4 (user input) | T | P | (position from user input) J-Ks=0.379+/-0.035 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:40.18 +40:13:30.4: 13.47 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:40.18 +40:13:30.4: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 40.18 +40 13 30.4 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.44 03:45:46.80 +39:11:32.7
156.07268 -12.20915 galactic Per Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:45:46.80 +39:11:32.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.648+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:45:46.80 +39:11:32.7: 13.44 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:45:46.80 +39:11:32.7: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 45 46.80 +39 11 32.7 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.41 03:56:39.13 +42:06:02.7
155.79468 -8.65479 galactic Per Second-epoch detections are separated by 2.1" and 7.1 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 | target | 03:56:39.13 +42:06:02.7 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.032 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:56:39.13 +42:06:02.7: 13.44 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:56:39.13 +42:06:02.7: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 56 39.13 +42 06 02.7 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.34 03:44:51.49 +39:44:55.4
155.57470 -11.88675 galactic Per Second-epoch detections are separated by 3.9" and 7.2 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 | ATO J056.2148+39.7500 | 03:44:51.49 +39:44:55.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.364+/-0.032 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:44:51.49 +39:44:55.4: 13.42 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:44:51.49 +39:44:55.4: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 44 51.49 +39 44 55.4 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J056.2148+39.7500,2461289.7513,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J056.2148+39.7500 20260906.2513 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.36 03:51:50.58 +42:07:48.8
155.08539 -9.20732 galactic Per Second-epoch detections are separated by 1.3" and 6.5 pix
The object was found in VSX24" Gaia DR3 231241455833917952
Type: ROT
# Max. Min./Amp. JD0 Period
15.180 G 15.210 G F
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:50.58 +42:07:48.8: 13.40 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:50.58 +42:07:48.8: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 50.58 +42 07 48.8 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 231241455833917952,2461289.7513,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 231241455833917952 20260906.2513 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.38 03:49:51.43 +42:06:23.2
154.81276 -9.45992 galactic Per Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J057.4623+42.1039 | 03:49:51.43 +42:06:23.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.762+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:49:51.43 +42:06:23.2: 13.41 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:49:51.43 +42:06:23.2: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 49 51.43 +42 06 23.2 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.4623+42.1039,2461289.7513,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J057.4623+42.1039 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.34 03:51:12.59 +40:50:11.7
155.83127 -10.27838 galactic Per Second-epoch detections are separated by 2.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:12.59 +40:50:11.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.893+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:12.59 +40:50:11.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:12.59 +40:50:11.7: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 12.59 +40 50 11.7 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.38 03:46:13.97 +41:22:08.9
154.75050 -10.45841 galactic Per Second-epoch detections are separated by 2.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:46:13.97 +41:22:08.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.823+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:13.97 +41:22:08.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:13.97 +41:22:08.9: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 46 13.97 +41 22 08.9 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.37 03:47:51.06 +42:20:17.3
154.37239 -9.51444 galactic Per Second-epoch detections are separated by 0.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J056.9724+42.3423 | 03:47:51.06 +42:20:17.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.658+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:51.06 +42:20:17.3: 13.36 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:51.06 +42:20:17.3: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 47 51.06 +42 20 17.3 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J056.9724+42.3423,2461289.7513,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J056.9724+42.3423 20260906.2513 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.38 03:50:22.85 +42:03:43.6
154.91742 -9.43257 galactic Per Second-epoch detections are separated by 1.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J057.5945+42.0654 | 03:50:22.85 +42:03:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.847+/-0.033 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:50:22.85 +42:03:43.6: 13.35 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:50:22.85 +42:03:43.6: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 50 22.85 +42 03 43.6 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.5945+42.0654,2461289.7513,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J057.5945+42.0654 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.04 04:57:28.14 +41:10:34.0
164.35767 -1.10891 galactic Aur Second-epoch detections are separated by 5.1" and 7.1 pix
The object was found in VSX 4" Gaia DR3 201623735017410048
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.300 G 13.330 G A
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:28.14 +41:10:34.0: 13.20 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:28.14 +41:10:34.0: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201623735017410048,2461289.7513,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201623735017410048 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.27 03:52:17.78 +42:29:02.4
154.92176 -8.88164 galactic Per Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:52:17.78 +42:29:02.4 (user input) | T | P | (position from user input) J-Ks=0.365+/-0.033 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:17.78 +42:29:02.4: 13.34 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:17.78 +42:29:02.4: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 17.78 +42 29 02.4 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.28 03:54:16.87 +41:53:57.0
155.58734 -9.09378 galactic Per Second-epoch detections are separated by 0.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J058.5704+41.8873 | 03:54:16.87 +41:53:57.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.315+/-0.034 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:54:16.87 +41:53:57.0: 13.36 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:54:16.87 +41:53:57.0: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 54 16.87 +41 53 57.0 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J058.5704+41.8873,2461289.7513,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J058.5704+41.8873 20260906.2513 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.36 03:47:57.35 +39:51:30.5
155.97688 -11.42756 galactic Per Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:47:57.35 +39:51:30.5 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.375+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:57.35 +39:51:30.5: 13.35 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:57.35 +39:51:30.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 47 57.35 +39 51 30.5 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.32 03:46:41.78 +41:58:24.7
154.43508 -9.93267 galactic Per Second-epoch detections are separated by 2.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:46:41.78 +41:58:24.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.366+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:41.78 +41:58:24.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:41.78 +41:58:24.7: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 46 41.78 +41 58 24.7 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.28 03:48:56.91 +39:55:42.5
156.08192 -11.25279 galactic Per Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:48:56.91 +39:55:42.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.919+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:48:56.91 +39:55:42.5: 13.34 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:48:56.91 +39:55:42.5: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 48 56.91 +39 55 42.5 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.36 03:47:53.99 +39:16:53.9
156.34096 -11.88111 galactic Per Second-epoch detections are separated by 1.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:47:53.99 +39:16:53.9 (user input) | T | P | (position from user input) J-Ks=0.543+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:53.99 +39:16:53.9: 13.33 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:53.99 +39:16:53.9: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 47 53.99 +39 16 53.9 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.28 03:51:37.56 +42:09:52.3
155.03184 -9.20659 galactic Per Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:37.56 +42:09:52.3 (user input) | T | P | (position from user input) J-Ks=0.901+/-0.030 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:37.56 +42:09:52.3: 13.33 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:37.56 +42:09:52.3: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 37.56 +42 09 52.3 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.36 03:50:38.36 +41:57:28.3
155.02216 -9.48256 galactic Per Second-epoch detections are separated by 2.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J057.6628+41.9595 | 03:50:38.36 +41:57:28.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.812+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:50:38.36 +41:57:28.3: 13.30 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:50:38.36 +41:57:28.3: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 50 38.36 +41 57 28.3 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.6628+41.9595,2461289.7513,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J057.6628+41.9595 20260906.2513 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.24 03:43:49.29 +40:49:44.0
154.73095 -11.16400 galactic Per Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:43:49.29 +40:49:44.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.850+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:43:49.29 +40:49:44.0: 13.30 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:43:49.29 +40:49:44.0: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 43 49.29 +40 49 44.0 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.36 03:44:50.45 +40:44:48.7
154.93698 -11.10843 galactic Per Second-epoch detections are separated by 2.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:44:50.45 +40:44:48.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.412+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:44:50.45 +40:44:48.7: 13.30 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:44:50.45 +40:44:48.7: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 44 50.45 +40 44 48.7 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.32 03:46:57.53 +39:45:21.5
155.89129 -11.62790 galactic Per Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:46:57.53 +39:45:21.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.449+/-0.026 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:57.53 +39:45:21.5: 13.30 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:57.53 +39:45:21.5: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 46 57.53 +39 45 21.5 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.30 03:47:50.31 +41:09:40.5
155.12204 -10.43093 galactic Per Second-epoch detections are separated by 2.7" and 7.0 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 231092811305323008 | 03:47:52.71 +41:10:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.251+/-0.030 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:50.31 +41:09:40.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:50.31 +41:09:40.5: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 47 50.31 +41 09 40.5 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 231092811305323008,2461289.7513,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 231092811305323008 20260906.2513 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.26 03:50:27.52 +40:43:19.5
155.79424 -10.45728 galactic Per Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 230837385309500928 | 03:50:27.46 +40:43:19.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.380+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:50:27.52 +40:43:19.5: 13.29 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:50:27.52 +40:43:19.5: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 50 27.52 +40 43 19.5 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 230837385309500928,2461289.7513,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 230837385309500928 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.23 03:52:07.88 +40:43:49.4
156.03655 -10.24829 galactic Per Second-epoch detections are separated by 0.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:52:07.88 +40:43:49.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.828+/-0.032 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:07.88 +40:43:49.4: 13.28 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:07.88 +40:43:49.4: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 07.88 +40 43 49.4 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.02 04:57:10.42 +41:22:55.7
164.16194 -1.02390 galactic Aur Second-epoch detections are separated by 2.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.2936+41.3824 | 04:57:10.42 +41:22:55.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.165+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:10.42 +41:22:55.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:10.42 +41:22:55.7: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.2936+41.3824,2461289.7513,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.2936+41.3824 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.27 03:48:01.97 +41:43:53.4
154.78601 -9.96496 galactic Per Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J057.0115+41.7298 | 03:48:01.97 +41:43:53.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.773+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:48:01.97 +41:43:53.4: 13.28 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:48:01.97 +41:43:53.4: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 48 01.97 +41 43 53.4 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.0115+41.7298,2461289.7513,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J057.0115+41.7298 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.18 04:39:17.27 +39:49:43.5
163.16458 -4.62123 galactic Per Second-epoch detections are separated by 2.1" and 7.0 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 | target | 04:39:17.27 +39:49:43.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.502+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:39:17.27 +39:49:43.5: 13.28 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:39:17.27 +39:49:43.5: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 39 17.27 +39 49 43.5 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.49 04:56:10.04 +33:01:16.7
170.59660 -6.38507 galactic Aur Second-epoch detections are separated by 2.4" and 7.3 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 | Large-amplitude variable Gaia DR2 160836737006772480 | 04:56:10.04 +33:01:16.7 (user input) | 2021A&A...648A..44M | | (position from user input) (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) J-Ks=1.207+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:10.04 +33:01:16.7: 13.25 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:10.04 +33:01:16.7: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 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 160836737006772480,2461289.7513,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 160836737006772480 20260906.2513 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.29 03:50:28.95 +40:07:07.8
156.18929 -10.91905 galactic Per Second-epoch detections are separated by 1.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:50:28.95 +40:07:07.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.526+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:50:28.95 +40:07:07.8: 13.25 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:50:28.95 +40:07:07.8: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 50 28.95 +40 07 07.8 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.19 03:52:35.26 +41:46:36.2
155.42240 -9.39040 galactic Per Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J058.1458+41.7788 | 03:52:35.26 +41:46:36.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.435+/-0.032 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:35.26 +41:46:36.2: 13.25 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:35.26 +41:46:36.2: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 35.26 +41 46 36.2 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J058.1458+41.7788,2461289.7513,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J058.1458+41.7788 20260906.2513 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.24 03:52:40.27 +41:04:35.5
155.89033 -9.91739 galactic Per Second-epoch detections are separated by 3.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:52:40.27 +41:04:35.5 (user input) | T | P | (position from user input) J-Ks=1.135+/-0.030 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:40.27 +41:04:35.5: 13.25 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:40.27 +41:04:35.5: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 40.27 +41 04 35.5 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.96 04:58:55.95 +42:08:02.7
163.77678 -0.29955 galactic Aur Second-epoch detections are separated by 3.6" and 7.8 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 | target | 04:58:55.95 +42:08:02.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.719+/-0.054 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:55.95 +42:08:02.7: 13.24 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:55.95 +42:08:02.7: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.30 03:44:54.77 +39:59:05.8
155.43243 -11.69566 galactic Per Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J056.2297+39.9876 | 03:44:54.77 +39:59:05.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.227+/-0.029 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:44:54.77 +39:59:05.8: 13.22 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:44:54.77 +39:59:05.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 44 54.77 +39 59 05.8 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J056.2297+39.9876,2461289.7513,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J056.2297+39.9876 20260906.2513 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.36 03:44:08.15 +40:15:34.0
155.13923 -11.57342 galactic Per Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:44:08.15 +40:15:34.0 (user input) | T | P | (position from user input) J-Ks=0.767+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:44:08.15 +40:15:34.0: 13.23 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:44:08.15 +40:15:34.0: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 44 08.15 +40 15 34.0 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.13 03:52:11.71 +40:33:50.8
156.15443 -10.36805 galactic Per Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:52:11.71 +40:33:50.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.476+/-0.034 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:11.71 +40:33:50.8: 13.22 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:11.71 +40:33:50.8: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 11.71 +40 33 50.8 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.15 04:40:22.43 +40:04:07.5
163.12236 -4.30635 galactic Per Second-epoch detections are separated by 3.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J070.0805+40.0624 | 04:40:22.36 +40:04:09.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.196+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:40:22.43 +40:04:07.5: 13.22 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:40:22.43 +40:04:07.5: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 40 22.43 +40 04 07.5 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J070.0805+40.0624,2461289.7513,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J070.0805+40.0624 20260906.2513 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.99 05:01:54.98 +41:54:01.4
164.30233 -0.00706 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 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 J075.4769+41.8978 | 05:01:54.98 +41:54:01.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.771+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:54.98 +41:54:01.4: 13.19 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:54.98 +41:54:01.4: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.4769+41.8978,2461289.7513,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.4769+41.8978 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.98 04:20:31.63 +33:37:33.2
165.17656 -11.59292 galactic Per Second-epoch detections are separated by 1.5" and 7.1 pix
The object was found in VSX 0" ASASSN-V J042031.64+333733.1
Type: SR
# Max. Min./Amp. JD0 Period
14.280 g Y 0.180 g 2458442.85400 528.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:20:31.63 +33:37:33.2: 13.19 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:20:31.63 +33:37:33.2: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 20 31.63 +33 37 33.2 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J042031.64+333733.1,2461289.7513,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J042031.64+333733.1 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.98 04:56:15.33 +41:07:15.6
164.25811 -1.32178 galactic Aur Second-epoch detections are separated by 2.0" and 7.4 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 | target | 04:56:15.33 +41:07:15.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.785+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:15.33 +41:07:15.6: 13.18 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:15.33 +41:07:15.6: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.16 03:51:00.85 +41:53:33.2
155.11882 -9.48857 galactic Per Second-epoch detections are separated by 2.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:00.85 +41:53:33.2 (user input) | T | P | (position from user input) J-Ks=0.752+/-0.031 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:00.85 +41:53:33.2: 13.18 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:00.85 +41:53:33.2: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 00.85 +41 53 33.2 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.17 03:52:50.85 +40:12:22.9
156.48510 -10.56217 galactic Per Second-epoch detections are separated by 3.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:52:50.85 +40:12:22.9 (user input) | T | P | (position from user input) J-Ks=0.876+/-0.030 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:50.85 +40:12:22.9: 13.17 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:50.85 +40:12:22.9: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 50.85 +40 12 22.9 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.23 03:50:35.94 +42:10:30.5
154.87632 -9.31958 galactic Per Second-epoch detections are separated by 1.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J057.6528+42.1775 | 03:50:35.94 +42:10:30.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.395+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:50:35.94 +42:10:30.5: 13.18 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:50:35.94 +42:10:30.5: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 50 35.94 +42 10 30.5 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.6528+42.1775,2461289.7513,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J057.6528+42.1775 20260906.2513 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.96 04:57:20.50 +41:14:23.1
164.29296 -1.08799 galactic Aur Second-epoch detections are separated by 1.0" and 7.3 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 | target | 04:57:20.50 +41:14:23.1 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.378+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:20.50 +41:14:23.1: 13.16 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:20.50 +41:14:23.1: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.03 04:56:46.73 +41:21:39.2
164.13231 -1.09504 galactic Aur Second-epoch detections are separated by 1.6" and 7.6 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 | target | 04:56:46.73 +41:21:39.2 (user input) | T | P | (position from user input) J-Ks=0.733+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:46.73 +41:21:39.2: 13.16 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:46.73 +41:21:39.2: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.12 04:37:13.14 +39:57:31.9
162.80216 -4.83085 galactic Per Second-epoch detections are separated by 2.1" and 7.3 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 | target | 04:37:13.14 +39:57:31.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.855+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:37:13.14 +39:57:31.9: 13.15 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:37:13.14 +39:57:31.9: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 37 13.14 +39 57 31.9 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.17 03:51:01.28 +40:06:04.2
156.28149 -10.86681 galactic Per Second-epoch detections are separated by 1.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:01.28 +40:06:04.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.923+/-0.032 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:01.28 +40:06:04.2: 13.15 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:01.28 +40:06:04.2: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 01.28 +40 06 04.2 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.22 03:42:06.96 +40:56:32.0
154.40110 -11.27388 galactic Per Second-epoch detections are separated by 2.7" and 7.0 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 | target | 03:42:06.96 +40:56:32.0 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.289+/-0.030 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:42:06.96 +40:56:32.0: 13.14 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:42:06.96 +40:56:32.0: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 42 06.96 +40 56 32.0 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.01 04:56:12.68 +40:32:52.5
164.70013 -1.68680 galactic Aur Second-epoch detections are separated by 1.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:12.68 +40:32:52.5 (user input) | T | P | (position from user input) J-Ks=1.089+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:12.68 +40:32:52.5: 13.14 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:12.68 +40:32:52.5: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.21 03:46:29.67 +40:03:09.3
155.63023 -11.45332 galactic Per Second-epoch detections are separated by 1.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:46:29.67 +40:03:09.3 (user input) | T | P | (position from user input) J-Ks=0.970+/-0.025 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:29.67 +40:03:09.3: 13.10 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:29.67 +40:03:09.3: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 46 29.67 +40 03 09.3 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.13 03:46:46.02 +41:33:42.1
154.70735 -10.24559 galactic Per Second-epoch detections are separated by 2.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 231163940264497408 | 03:46:44.29 +41:34:03.6 (Gaia DR3) | S (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.959+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:46:46.02 +41:33:42.1: 13.07 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:46:46.02 +41:33:42.1: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 46 46.02 +41 33 42.1 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 231163940264497408,2461289.7513,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 231163940264497408 20260906.2513 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.93 05:01:35.12 +41:56:43.7
164.22896 -0.02806 galactic Aur Second-epoch detections are separated by 0.6" and 7.4 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 | target | 05:01:35.12 +41:56:43.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.053+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:35.12 +41:56:43.7: 13.12 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:35.12 +41:56:43.7: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.89 04:57:32.33 +41:29:46.8
164.11527 -0.89922 galactic Aur Second-epoch detections are separated by 2.6" and 6.9 pix
The object was found in VSX 2" ASASSN-V J045732.47+412947.8
Type: SR
# Max. Min./Amp. JD0 Period
14.770 g Y 0.370 g 2459222.84200 698.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:32.33 +41:29:46.8: 13.12 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:32.33 +41:29:46.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045732.47+412947.8,2461289.7513,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045732.47+412947.8 20260906.2513 11.89CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.14 03:47:20.47 +41:39:38.4
154.72924 -10.10120 galactic Per Second-epoch detections are separated by 0.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 231123705009876992 | 03:47:22.87 +41:39:42.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.377+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:20.47 +41:39:38.4: 13.05 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:20.47 +41:39:38.4: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 47 20.47 +41 39 38.4 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 231123705009876992,2461289.7513,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 231123705009876992 20260906.2513 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.15 03:52:32.23 +40:59:48.4
155.92266 -9.99475 galactic Per Second-epoch detections are separated by 1.3" and 6.9 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 | target | 03:52:32.23 +40:59:48.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.001+/-0.033 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:32.23 +40:59:48.4: 13.11 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:32.23 +40:59:48.4: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 32.23 +40 59 48.4 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.05 04:58:08.84 +42:03:26.8
163.74650 -0.46133 galactic Aur Second-epoch detections are separated by 1.2" and 7.2 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 | ATO J074.5355+42.0548 | 04:58:08.84 +42:03:26.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.664+/-0.025 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:08.84 +42:03:26.8: 13.13 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:08.84 +42:03:26.8: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.5355+42.0548,2461289.7513,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.5355+42.0548 20260906.2513 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.94 04:55:29.69 +41:00:53.8
164.25095 -1.49997 galactic Aur Second-epoch detections are separated by 2.9" and 7.1 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 | target | 04:55:29.69 +41:00:53.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.410+/-0.026 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:29.69 +41:00:53.8: 13.09 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:29.69 +41:00:53.8: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.14 03:48:46.02 +38:45:24.8
156.81457 -12.17973 galactic Per Second-epoch detections are separated by 1.0" and 6.5 pix
The object was found in VSX 0" ZTF J034845.98+384524.6
Type: EB:
# Max. Min./Amp. JD0 Period
13.520 g Y 0.184 g 2458379.97290 1.348627100000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:48:46.02 +38:45:24.8: 13.08 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:48:46.02 +38:45:24.8: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 48 46.02 +38 45 24.8 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J034845.98+384524.6,2461289.7513,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J034845.98+384524.6 20260906.2513 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.01 04:56:53.62 +41:18:55.2
164.18137 -1.10665 galactic Aur Second-epoch detections are separated by 3.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:53.62 +41:18:55.2 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:53.62 +41:18:55.2: 13.07 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:53.62 +41:18:55.2: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.92 04:59:20.66 +41:30:27.2
164.31631 -0.62720 galactic Aur Second-epoch detections are separated by 2.0" and 7.0 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 201748499528532352 | 04:59:23.56 +41:30:51.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1958ApJS....4....1M LF 7 +41 130 J-Ks=0.328+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:20.66 +41:30:27.2: 13.06 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:20.66 +41:30:27.2: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201748499528532352,2461289.7513,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201748499528532352 20260906.2513 11.92CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.95 05:00:58.25 +41:39:16.5
164.38818 -0.29710 galactic Aur Second-epoch detections are separated by 1.1" and 7.6 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 | target | 05:00:58.25 +41:39:16.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.641+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:58.25 +41:39:16.5: 13.05 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:58.25 +41:39:16.5: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.97 04:59:28.78 +41:32:05.0
164.31063 -0.59049 galactic Aur Second-epoch detections are separated by 1.7" and 7.3 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 J074.8752+41.5286 | 04:59:28.78 +41:32:05.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.343+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:28.78 +41:32:05.0: 13.07 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:28.78 +41:32:05.0: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.8752+41.5286,2461289.7513,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.8752+41.5286 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.90 04:57:58.54 +41:14:17.0
164.36849 -0.99576 galactic Aur Second-epoch detections are separated by 1.1" and 7.0 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 | target | 04:57:58.54 +41:14:17.0 (user input) | T | P | (position from user input) J-Ks=0.997+/-0.030 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:58.54 +41:14:17.0: 13.04 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:58.54 +41:14:17.0: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.15 03:51:03.50 +41:57:59.7
155.07745 -9.42627 galactic Per Second-epoch detections are separated by 1.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:03.50 +41:57:59.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.441+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:03.50 +41:57:59.7: 13.04 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:03.50 +41:57:59.7: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 03.50 +41 57 59.7 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.04 04:53:31.48 +40:37:41.0
164.31698 -2.03312 galactic Aur Second-epoch detections are separated by 1.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:53:31.48 +40:37:41.0 (user input) | T | P | (position from user input) J-Ks=0.791+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:31.48 +40:37:41.0: 13.06 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:31.48 +40:37:41.0: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.92 04:59:07.41 +41:59:26.9
163.91122 -0.36047 galactic Aur Second-epoch detections are separated by 2.5" and 7.2 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 | ATO J074.7913+41.9897 | 04:59:07.41 +41:59:26.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K3 (LAMOST DR5)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:07.41 +41:59:26.9: 13.04 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:07.41 +41:59:26.9: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.7913+41.9897,2461289.7513,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.7913+41.9897 20260906.2513 11.92CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.99 04:08:25.99 +34:20:03.2
162.84681 -12.85901 galactic Per Second-epoch detections are separated by 1.5" and 6.9 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 | target | 04:08:25.99 +34:20:03.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.475+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:08:25.99 +34:20:03.2: 13.03 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:08:25.99 +34:20:03.2: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 08 25.99 +34 20 03.2 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.92 04:57:59.44 +42:02:10.4
163.74504 -0.49731 galactic Aur Second-epoch detections are separated by 1.5" and 7.4 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 J074.4983+42.0410 | 04:57:59.51 +42:02:11.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.177+/-0.023 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:59.44 +42:02:10.4: 13.03 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:59.44 +42:02:10.4: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.4983+42.0410,2461289.7513,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.4983+42.0410 20260906.2513 11.92CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.02 04:55:17.06 +40:24:11.3
164.70251 -1.91491 galactic Aur Second-epoch detections are separated by 5.4" and 6.5 pix
The object was found in VSX21" Gaia DR3 200095693031364992
Type: ROT
# Max. Min./Amp. JD0 Period
14.140 G 14.170 G 18.584000000000 F
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:17.06 +40:24:11.3: 13.04 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:17.06 +40:24:11.3: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 200095693031364992,2461289.7513,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 200095693031364992 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.96 03:50:09.86 +40:22:49.0
155.97194 -10.75636 galactic Per Second-epoch detections are separated by 1.8" and 6.3 pix
The object was found in VSX 2" ASASSN-V J035009.73+402248.7
Type: L
# Max. Min./Amp. JD0 Period
13.530 V 13.730 V
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:50:09.86 +40:22:49.0: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:50:09.86 +40:22:49.0: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 50 09.86 +40 22 49.0 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J035009.73+402248.7,2461289.7513,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J035009.73+402248.7 20260906.2513 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.93 04:57:23.85 +40:41:33.9
164.72750 -1.42055 galactic Aur Second-epoch detections are separated by 3.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.3615+40.7005 | 04:57:23.85 +40:41:33.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=11.629+/- (unrealisitic color!)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:23.85 +40:41:33.9: 13.00 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:23.85 +40:41:33.9: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.3615+40.7005,2461289.7513,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.3615+40.7005 20260906.2513 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.12 03:52:17.29 +40:29:03.9
156.22023 -10.41780 galactic Per Second-epoch detections are separated by 0.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:52:17.29 +40:29:03.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:52:17.29 +40:29:03.9: 13.04 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:52:17.29 +40:29:03.9: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 52 17.29 +40 29 03.9 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.94 05:01:11.57 +41:47:07.6
164.31041 -0.18399 galactic Aur Second-epoch detections are separated by 2.5" and 7.0 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 | target | 05:01:11.57 +41:47:07.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.375+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:11.57 +41:47:07.6: 13.02 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:11.57 +41:47:07.6: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.99 04:57:50.90 +41:07:05.1
164.44756 -1.08913 galactic Aur Second-epoch detections are separated by 3.3" and 7.9 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 | target | 04:57:50.90 +41:07:05.1 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=0.887+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:50.90 +41:07:05.1: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:50.90 +41:07:05.1: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 12.12 03:47:46.30 +39:56:18.4
155.89740 -11.38790 galactic Per Second-epoch detections are separated by 2.0" and 6.9 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 | target | 03:47:46.30 +39:56:18.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.802+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:47:46.30 +39:56:18.4: 12.99 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:47:46.30 +39:56:18.4: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 47 46.30 +39 56 18.4 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.93 05:01:58.51 +41:53:11.0
164.32010 -0.00698 galactic Aur Second-epoch detections are separated by 2.0" and 7.1 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 | target | 05:01:58.51 +41:53:11.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.605+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:58.51 +41:53:11.0: 13.00 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:58.51 +41:53:11.0: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.88 05:00:38.49 +42:11:35.2
163.92596 -0.01403 galactic Aur Second-epoch detections are separated by 3.0" and 7.3 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 J075.1739+42.1933 | 05:00:38.49 +42:11:35.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.359+/-0.032 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:38.49 +42:11:35.2: 12.98 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:38.49 +42:11:35.2: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.1739+42.1933,2461289.7513,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.1739+42.1933 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.96 04:58:32.79 +41:38:59.4
164.11217 -0.65617 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 pix
The object was found in VSX 8" Gaia DR3 201672014749553792
Type: ROT
# Max. Min./Amp. JD0 Period
14.860 G 14.900 G M
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:32.79 +41:38:59.4: 12.99 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:32.79 +41:38:59.4: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201672014749553792,2461289.7513,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201672014749553792 20260906.2513 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.99 04:17:22.94 +36:19:02.5
162.76238 -10.16514 galactic Per Second-epoch detections are separated by 0.3" and 7.0 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 177406647819564416 | 04:17:22.95 +36:19:02.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K4 (LAMOST DR5) J-Ks=1.036+/-0.023 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:17:22.94 +36:19:02.5: 12.97 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:17:22.94 +36:19:02.5: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 17 22.94 +36 19 02.5 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 177406647819564416,2461289.7513,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 177406647819564416 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.99 04:35:52.54 +38:38:30.5
163.61117 -5.90482 galactic Per Second-epoch detections are separated by 2.2" and 7.4 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 | ASASSN-V J043554.62+383901.7 | 04:35:54.62 +38:39:01.7 (Gaia DR3) | SR (local) | 62.510000000000 (local) | Gaia3var=NOT_AVAILABLE SpType: M1 1947AnDea...5....1L DO 10575
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:35:52.54 +38:38:30.5: 12.92 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:35:52.54 +38:38:30.5: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 35 52.54 +38 38 30.5 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J043554.62+383901.7,2461289.7513,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J043554.62+383901.7 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.91 04:54:57.28 +40:35:27.8
164.51682 -1.84567 galactic Aur Second-epoch detections are separated by 2.5" and 7.2 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 | target | 04:54:57.28 +40:35:27.8 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.033 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:57.28 +40:35:27.8: 12.94 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:57.28 +40:35:27.8: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.80 04:59:32.68 +41:42:08.7
164.18633 -0.47727 galactic Aur Second-epoch detections are separated by 1.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.8744+41.7099 | 04:59:32.67 +41:42:07.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.121+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:32.68 +41:42:08.7: 12.92 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:32.68 +41:42:08.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.8744+41.7099,2461289.7513,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.8744+41.7099 20260906.2513 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.89 04:56:36.30 +40:50:53.7
164.51229 -1.44081 galactic Aur Second-epoch detections are separated by 0.8" and 7.3 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 J074.1510+40.8482 | 04:56:36.30 +40:50:53.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.357+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:36.30 +40:50:53.7: 12.92 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:36.30 +40:50:53.7: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.1510+40.8482,2461289.7513,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.1510+40.8482 20260906.2513 11.89CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.82 04:57:05.16 +40:26:37.1
164.88550 -1.62206 galactic Aur Second-epoch detections are separated by 1.7" and 7.3 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 200053391894799488 | 04:57:05.18 +40:26:37.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.953+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:05.16 +40:26:37.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:05.16 +40:26:37.1: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 200053391894799488,2461289.7513,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 200053391894799488 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.86 05:00:43.34 +41:54:22.8
164.16120 -0.17874 galactic Aur Second-epoch detections are separated by 1.1" and 7.2 pix
The object was found in VSX25" ZTF J050042.65+415359.1
Type: BY
# Max. Min./Amp. JD0 Period
16.836 r Y 0.082 r 2458428.87440 2.969700800000
ATTENTION: measured mag 11.86 is 4.9 mag brighter than the VSX record maximum brightness 16.75 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:43.34 +41:54:22.8: 12.91 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:43.34 +41:54:22.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J050042.65+415359.1,2461289.7513,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J050042.65+415359.1 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.94 05:01:27.07 +42:04:34.8
164.11034 0.03257 galactic Aur Second-epoch detections are separated by 2.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:01:27.07 +42:04:34.8 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.183+/-0.033 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:27.07 +42:04:34.8: 12.91 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:27.07 +42:04:34.8: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.80 04:53:59.81 +40:26:54.0
164.51313 -2.07695 galactic Aur Second-epoch detections are separated by 2.1" and 7.0 pix
The object was found in VSX21" Gaia DR3 200088404471583232
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.880 G 13.910 G F
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:59.81 +40:26:54.0: 12.89 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:59.81 +40:26:54.0: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 200088404471583232,2461289.7513,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 200088404471583232 20260906.2513 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.94 04:08:51.36 +34:22:14.8
162.88548 -12.77223 galactic Per Second-epoch detections are separated by 2.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J062.2133+34.3711 | 04:08:51.36 +34:22:14.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.341+/-0.031 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:08:51.36 +34:22:14.8: 12.92 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:08:51.36 +34:22:14.8: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 08 51.36 +34 22 14.8 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J062.2133+34.3711,2461289.7513,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J062.2133+34.3711 20260906.2513 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.92 04:57:17.41 +41:14:55.8
164.27982 -1.08990 galactic Aur Second-epoch detections are separated by 3.7" and 7.2 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 | target | 04:57:17.41 +41:14:55.8 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:17.41 +41:14:55.8: 12.87 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:17.41 +41:14:55.8: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.92CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.86 04:05:22.71 +33:16:17.2
163.12731 -14.06638 galactic Per Second-epoch detections are separated by 0.7" and 7.1 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 | target | 04:05:22.71 +33:16:17.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.472+/-0.036 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:05:22.71 +33:16:17.2: 12.90 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:05:22.71 +33:16:17.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 05 22.71 +33 16 17.2 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.97 03:51:54.75 +41:20:59.5
155.60132 -9.79910 galactic Per Second-epoch detections are separated by 2.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J057.9717+41.3581 | 03:51:54.76 +41:21:00.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.868+/-0.032 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 03:51:54.75 +41:20:59.5: 12.88 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 03:51:54.75 +41:20:59.5: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 03 51 54.75 +41 20 59.5 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J057.9717+41.3581,2461289.7513,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J057.9717+41.3581 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.86 05:01:32.97 +42:00:47.2
164.17146 0.00818 galactic Aur Second-epoch detections are separated by 0.8" and 7.3 pix
The object was found in VSX 2" Gaia DR3 201785981706456576
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.670 G 12.700 G A
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:32.97 +42:00:47.2: 12.87 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:32.97 +42:00:47.2: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201785981706456576,2461289.7513,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201785981706456576 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.85 04:08:46.93 +34:32:47.8
162.74945 -12.65586 galactic Per Second-epoch detections are separated by 0.8" and 7.1 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 170819920332859776 | 04:08:46.82 +34:32:47.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.765+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:08:46.93 +34:32:47.8: 12.87 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:08:46.93 +34:32:47.8: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 08 46.93 +34 32 47.8 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 170819920332859776,2461289.7513,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 170819920332859776 20260906.2513 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.94 04:52:23.66 +39:58:22.9
164.68812 -2.61449 galactic Aur Second-epoch detections are separated by 1.7" and 7.5 pix
The object was found in VSX 2" Gaia DR3 199981103303294464
Type: ROT
# Max. Min./Amp. JD0 Period
12.510 G 12.540 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:52:23.66 +39:58:22.9: 12.88 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:52:23.66 +39:58:22.9: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 199981103303294464,2461289.7513,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 199981103303294464 20260906.2513 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.82 04:54:20.61 +40:25:29.2
164.57303 -2.04058 galactic Aur Second-epoch detections are separated by 4.2" and 7.1 pix
The object was found in VSX19" Gaia DR3 200087859011059072
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.010 G 14.030 G F
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:20.61 +40:25:29.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:20.61 +40:25:29.2: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 200087859011059072,2461289.7513,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 200087859011059072 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.94 05:00:33.80 +42:05:03.7
164.00273 -0.09242 galactic Aur Second-epoch detections are separated by 2.5" and 7.3 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 | target | 05:00:33.80 +42:05:03.7 (user input) | T | P | (position from user input) J-Ks=0.136+/-0.033 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:33.80 +42:05:03.7: 12.85 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:33.80 +42:05:03.7: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.71 04:58:38.55 +41:47:29.8
164.01208 -0.55417 galactic Aur Second-epoch detections are separated by 3.0" and 7.6 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 201769832626885376 | 04:58:38.43 +41:47:31.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.753+/-0.031 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:38.55 +41:47:29.8: 12.86 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:38.55 +41:47:29.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201769832626885376,2461289.7513,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201769832626885376 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.85 05:00:27.75 +41:46:29.5
164.23499 -0.29783 galactic Aur Second-epoch detections are separated by 2.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 201758566932639104 | 05:00:27.75 +41:46:29.5 (user input) | 2021A&A...648A..44M | | (position from user input) (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) J-Ks=0.780+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:27.75 +41:46:29.5: 12.87 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:27.75 +41:46:29.5: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 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 201758566932639104,2461289.7513,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 201758566932639104 20260906.2513 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.77 04:57:15.99 +41:20:49.5
164.20021 -1.03214 galactic Aur Second-epoch detections are separated by 1.3" and 7.1 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 | target | 04:57:15.99 +41:20:49.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.421+/-0.026 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:15.99 +41:20:49.5: 12.85 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:15.99 +41:20:49.5: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.88 04:54:35.57 +40:27:52.2
164.57202 -1.97871 galactic Aur Second-epoch detections are separated by 2.4" and 7.7 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 200111219337858688 | 04:54:35.47 +40:27:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.729+/-0.032 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:35.57 +40:27:52.2: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:35.57 +40:27:52.2: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 200111219337858688,2461289.7513,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 200111219337858688 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.80 04:21:51.52 +33:53:49.8
165.17340 -11.20541 galactic Per Second-epoch detections are separated by 1.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J065.4646+33.8974 | 04:21:51.51 +33:53:50.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M4 (LAMOST DR5) J-Ks=1.268+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:21:51.52 +33:53:49.8: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:21:51.52 +33:53:49.8: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 21 51.52 +33 53 49.8 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J065.4646+33.8974,2461289.7513,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J065.4646+33.8974 20260906.2513 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.80 04:55:10.24 +41:08:38.4
164.11210 -1.46652 galactic Aur Second-epoch detections are separated by 2.0" and 7.2 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 201819104491307392 | 04:55:10.22 +41:08:38.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.832+/-0.025 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:10.24 +41:08:38.4: 12.85 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:10.24 +41:08:38.4: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201819104491307392,2461289.7513,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201819104491307392 20260906.2513 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.80 05:00:57.87 +41:38:25.1
164.39871 -0.30681 galactic Aur Second-epoch detections are separated by 0.6" and 7.5 pix
The object was found in VSX20" Gaia DR3 201709844825131392
Type: S
# Max. Min./Amp. JD0 Period
17.200 G 17.560 G A
ATTENTION: measured mag 11.80 is 5.4 mag brighter than the VSX record maximum brightness 17.20 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:57.87 +41:38:25.1: 12.79 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:57.87 +41:38:25.1: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201709844825131392,2461289.7513,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201709844825131392 20260906.2513 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.71 04:58:01.47 +40:43:28.5
164.77652 -1.30772 galactic Aur Second-epoch detections are separated by 3.2" and 7.3 pix
The object was found in VSX16" Gaia DR3 201563815930153216
Type: E
# Max. Min./Amp. JD0 Period
19.060 G 19.550 G 7.116700000000
ATTENTION: measured mag 11.71 is 7.3 mag brighter than the VSX record maximum brightness 19.06 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:01.47 +40:43:28.5: 12.82 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:01.47 +40:43:28.5: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201563815930153216,2461289.7513,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201563815930153216 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.78 04:57:36.87 +42:23:16.7
163.42633 -0.33296 galactic Aur Second-epoch detections are separated by 0.8" and 7.3 pix
The object was found in VSX 1" V0864 Aur
Type: EA
# Max. Min./Amp. JD0 Period
13.630 g 14.240 g 2458465.90000 185.190000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:36.87 +42:23:16.7: 12.78 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:36.87 +42:23:16.7: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0864 Aur,2461289.7513,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0864 Aur 20260906.2513 11.78CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.86 04:57:04.27 +41:58:49.5
163.68231 -0.66570 galactic Aur Second-epoch detections are separated by 3.0" and 7.9 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 201881226900556288 | 04:57:08.14 +41:58:48.6 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B8 1958ApJS....4....1M LF 7 +41 85 J-Ks=0.662+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:04.27 +41:58:49.5: 12.77 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:04.27 +41:58:49.5: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201881226900556288,2461289.7513,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201881226900556288 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.85 04:12:30.16 +34:12:09.6
163.55917 -12.36816 galactic Per Second-epoch detections are separated by 1.8" and 7.3 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 170760447926895232 | 04:12:30.13 +34:12:10.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.764+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:12:30.16 +34:12:09.6: 12.78 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:12:30.16 +34:12:09.6: 12.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 12 30.16 +34 12 09.6 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 170760447926895232,2461289.7513,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 170760447926895232 20260906.2513 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.74 04:57:24.43 +41:18:28.6
164.24728 -1.03588 galactic Aur Second-epoch detections are separated by 0.3" and 7.4 pix
The object was found in VSX 1" Gaia DR3 201659748322238208
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.510 G 12.540 G F
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:24.43 +41:18:28.6: 12.75 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:24.43 +41:18:28.6: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201659748322238208,2461289.7513,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201659748322238208 20260906.2513 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.71 05:01:21.71 +41:26:28.6
164.60142 -0.37045 galactic Aur Second-epoch detections are separated by 2.6" and 7.6 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 | target | 05:01:21.71 +41:26:28.6 (user input) | T | P | (position from user input) SpType: A2IV (LAMOST DR5) J-Ks=0.261+/-0.027 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:21.71 +41:26:28.6: 12.77 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:21.71 +41:26:28.6: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.82 04:23:10.25 +34:32:53.9
164.88617 -10.55889 galactic Per Second-epoch detections are separated by 4.1" and 7.1 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 176225673548111744 | 04:23:10.18 +34:32:54.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.769+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:23:10.25 +34:32:53.9: 12.77 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:23:10.25 +34:32:53.9: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 23 10.25 +34 32 53.9 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 176225673548111744,2461289.7513,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 176225673548111744 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.88 04:57:54.10 +41:07:37.0
164.44686 -1.07575 galactic Aur Second-epoch detections are separated by 1.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:54.10 +41:07:37.0 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.239+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:54.10 +41:07:37.0: 12.74 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:54.10 +41:07:37.0: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.74 05:01:46.93 +41:38:09.5
164.49593 -0.18889 galactic Aur Second-epoch detections are separated by 0.9" and 7.4 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 201718018151229056 | 05:01:49.74 +41:38:36.0 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE SpType: A0 1958ApJS....4....1M LF 7 +41 190 J-Ks=0.116+/-0.030 (A)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:46.93 +41:38:09.5: 12.75 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:46.93 +41:38:09.5: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201718018151229056,2461289.7513,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201718018151229056 20260906.2513 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.73 04:06:28.59 +33:03:39.8
163.44843 -14.06078 galactic Per Second-epoch detections are separated by 3.1" and 7.4 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 | target | 04:06:28.59 +33:03:39.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.454+/-0.029 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:06:28.59 +33:03:39.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:06:28.59 +33:03:39.8: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 06 28.59 +33 03 39.8 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.77 04:58:32.67 +41:20:39.4
164.35159 -0.84605 galactic Aur Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.6402+41.3455 | 04:58:32.67 +41:20:39.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.306+/-0.029 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:32.67 +41:20:39.4: 12.74 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:32.67 +41:20:39.4: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.6402+41.3455,2461289.7513,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.6402+41.3455 20260906.2513 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.77 04:59:20.73 +42:14:03.0
163.74555 -0.17751 galactic Aur Second-epoch detections are separated by 0.4" and 7.4 pix
The object was found in VSX12" Gaia DR3 201973036120140800
Type: RS
# Max. Min./Amp. JD0 Period
17.310 G 17.650 G F
ATTENTION: measured mag 11.77 is 5.5 mag brighter than the VSX record maximum brightness 17.31 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:20.73 +42:14:03.0: 12.73 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:20.73 +42:14:03.0: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201973036120140800,2461289.7513,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201973036120140800 20260906.2513 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.71 05:01:18.58 +41:11:29.6
164.79251 -0.53152 galactic Aur Second-epoch detections are separated by 1.1" and 7.3 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 J075.3274+41.1801 | 05:01:18.71 +41:11:30.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.034+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:18.58 +41:11:29.6: 12.73 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:18.58 +41:11:29.6: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.3274+41.1801,2461289.7513,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.3274+41.1801 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.74 05:01:30.42 +41:43:11.5
164.39816 -0.17801 galactic Aur Second-epoch detections are separated by 1.1" and 7.6 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 | target | 05:01:30.42 +41:43:11.5 (user input) | T | P | (position from user input) J-Ks=0.271+/-0.037 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:30.42 +41:43:11.5: 12.72 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:30.42 +41:43:11.5: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.84 04:54:31.05 +40:48:57.5
164.28973 -1.76863 galactic Aur Second-epoch detections are separated by 5.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.6248+40.8098 | 04:54:29.96 +40:48:35.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.247+/-0.033 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:31.05 +40:48:57.5: 12.72 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:31.05 +40:48:57.5: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.6248+40.8098,2461289.7513,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J073.6248+40.8098 20260906.2513 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.62 04:44:37.96 +36:19:20.5
166.51640 -6.12612 galactic Per Second-epoch detections are separated by 0.6" and 7.2 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 | ATO J071.1581+36.3223 | 04:44:37.99 +36:19:20.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.459+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:44:37.96 +36:19:20.5: 12.72 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:44:37.96 +36:19:20.5: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 44 37.96 +36 19 20.5 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J071.1581+36.3223,2461289.7513,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J071.1581+36.3223 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.82 04:55:14.50 +40:22:32.9
164.71870 -1.93839 galactic Aur Second-epoch detections are separated by 1.4" and 7.4 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 J073.7965+40.3784 | 04:55:14.50 +40:22:32.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.506+/-0.032 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:14.50 +40:22:32.9: 12.71 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:14.50 +40:22:32.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.7965+40.3784,2461289.7513,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J073.7965+40.3784 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.65 04:58:12.89 +41:11:28.1
164.43321 -0.98968 galactic Aur Second-epoch detections are separated by 1.0" and 7.2 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 201645209853888768 | 04:58:12.85 +41:11:27.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.220+/-0.036 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:12.89 +41:11:28.1: 12.72 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:12.89 +41:11:28.1: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201645209853888768,2461289.7513,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201645209853888768 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.78 05:01:00.05 +41:08:16.0
164.79922 -0.61042 galactic Aur Second-epoch detections are separated by 3.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.2584+41.1358 | 05:01:00.07 +41:08:15.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.520+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:00.05 +41:08:16.0: 12.71 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:00.05 +41:08:16.0: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.2584+41.1358,2461289.7513,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.2584+41.1358 20260906.2513 11.78CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.75 04:56:10.90 +40:09:16.2
165.00370 -1.93730 galactic Aur Second-epoch detections are separated by 0.5" and 7.4 pix
The object was found in VSX17" Gaia DR3 200041743947701888
Type: S
# Max. Min./Amp. JD0 Period
17.870 G 18.430 G
ATTENTION: measured mag 11.75 is 6.1 mag brighter than the VSX record maximum brightness 17.87 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:10.90 +40:09:16.2: 12.71 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:10.90 +40:09:16.2: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 200041743947701888,2461289.7513,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 200041743947701888 20260906.2513 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.76 04:56:35.01 +41:29:30.3
164.00723 -1.04189 galactic Aur Second-epoch detections are separated by 1.2" and 7.2 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 | ATO J074.1417+41.4825 | 04:56:35.06 +41:29:31.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.236+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:35.01 +41:29:30.3: 12.70 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:35.01 +41:29:30.3: 12.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.1417+41.4825,2461289.7513,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.1417+41.4825 20260906.2513 11.76CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.81 04:58:16.58 +41:09:54.5
164.46077 -0.99676 galactic Aur Second-epoch detections are separated by 3.3" and 7.0 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 | target | 04:58:16.58 +41:09:54.5 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.129+/-0.035 (A)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:16.58 +41:09:54.5: 12.71 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:16.58 +41:09:54.5: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7513,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2513 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.62 04:56:55.24 +41:16:29.2
164.21622 -1.12800 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 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 201639991472715264 | 04:56:55.24 +41:16:29.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.291+/-0.026 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:55.24 +41:16:29.2: 12.69 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:55.24 +41:16:29.2: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201639991472715264,2461289.7513,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201639991472715264 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.66 04:52:35.42 +40:09:50.6
164.56399 -2.46443 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 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 199987558636258688 | 04:52:35.35 +40:09:51.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.763+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:52:35.42 +40:09:50.6: 12.68 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:52:35.42 +40:09:50.6: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 199987558636258688,2461289.7513,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 199987558636258688 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.67 05:00:26.58 +41:55:28.2
164.11489 -0.20850 galactic Aur Second-epoch detections are separated by 1.3" and 7.5 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 201763927050787584 | 05:00:26.68 +41:55:28.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.650+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:26.58 +41:55:28.2: 12.65 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:26.58 +41:55:28.2: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201763927050787584,2461289.7513,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201763927050787584 20260906.2513 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.62 05:00:24.45 +42:03:37.6
164.00375 -0.12993 galactic Aur Second-epoch detections are separated by 1.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.1155+42.0560 | 05:00:24.55 +42:03:37.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.850+/-0.032 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:24.45 +42:03:37.6: 12.66 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:24.45 +42:03:37.6: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.1155+42.0560,2461289.7513,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.1155+42.0560 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.52 04:18:31.62 +32:56:11.9
165.38406 -12.37305 galactic Per Second-epoch detections are separated by 1.9" and 7.0 pix
The object was found in VSX 2" ASASSN-V J041831.57+325610.2
Type: SR
# Max. Min./Amp. JD0 Period
13.860 g Y 0.350 g 2458691.11700 49.140000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:18:31.62 +32:56:11.9: 12.66 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:18:31.62 +32:56:11.9: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 18 31.62 +32 56 11.9 11.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J041831.57+325610.2,2461289.7513,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J041831.57+325610.2 20260906.2513 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.75 04:04:59.54 +33:28:20.4
162.92476 -13.97562 galactic Per Second-epoch detections are separated by 0.5" and 7.2 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 | ATO J061.2453+33.4737 | 04:04:59.54 +33:28:20.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.431+/-0.033 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:04:59.54 +33:28:20.4: 12.68 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:04:59.54 +33:28:20.4: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 04 59.54 +33 28 20.4 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J061.2453+33.4737,2461289.7513,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J061.2453+33.4737 20260906.2513 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.65 05:00:44.55 +41:18:33.5
164.63409 -0.54321 galactic Aur Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 201684830934080512 | 05:00:44.75 +41:18:33.7 (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) J-Ks=1.260+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:44.55 +41:18:33.5: 12.66 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:44.55 +41:18:33.5: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 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 201684830934080512,2461289.7513,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 201684830934080512 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.69 04:20:16.08 +33:34:29.0
165.17576 -11.66728 galactic Per Second-epoch detections are separated by 2.0" and 6.9 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 175702576594383104 | 04:20:17.55 +33:35:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.064+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:20:16.08 +33:34:29.0: 12.66 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:20:16.08 +33:34:29.0: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 20 16.08 +33 34 29.0 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 175702576594383104,2461289.7513,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 175702576594383104 20260906.2513 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.62 05:00:04.13 +40:55:58.1
164.85248 -0.87512 galactic Aur Second-epoch detections are separated by 1.4" and 7.4 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 201581579917805184 | 05:00:04.03 +40:55:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.732+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:04.13 +40:55:58.1: 12.65 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:04.13 +40:55:58.1: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201581579917805184,2461289.7513,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201581579917805184 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.58 04:57:29.45 +41:08:59.7
164.38073 -1.12201 galactic Aur Second-epoch detections are separated by 2.7" and 7.5 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 201623631938195840 | 04:57:29.41 +41:09:00.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.842+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:29.45 +41:08:59.7: 12.67 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:29.45 +41:08:59.7: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201623631938195840,2461289.7513,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201623631938195840 20260906.2513 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.71 04:59:21.33 +41:25:17.6
164.38518 -0.67876 galactic Aur Second-epoch detections are separated by 1.6" and 7.4 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 J074.8479+41.4258 | 04:59:21.34 +41:25:17.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.380+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:21.33 +41:25:17.6: 12.63 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:21.33 +41:25:17.6: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.8479+41.4258,2461289.7513,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.8479+41.4258 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.64 04:58:07.50 +41:17:15.6
164.34706 -0.94294 galactic Aur Second-epoch detections are separated by 1.6" and 7.2 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 | ATO J074.5268+41.2860 | 04:58:07.50 +41:17:15.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.233+/-0.030 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:07.50 +41:17:15.6: 12.64 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:07.50 +41:17:15.6: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.5268+41.2860,2461289.7513,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.5268+41.2860 20260906.2513 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.64 05:01:30.01 +41:39:29.2
164.44613 -0.21691 galactic Aur Second-epoch detections are separated by 1.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.3751+41.6582 | 05:01:30.04 +41:39:29.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.382+/-0.026 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:30.01 +41:39:29.2: 12.63 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:30.01 +41:39:29.2: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.3751+41.6582,2461289.7513,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.3751+41.6582 20260906.2513 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.51 04:56:15.73 +40:27:41.1
164.77370 -1.73337 galactic Aur Second-epoch detections are separated by 1.1" and 7.1 pix
The object was found in VSX 0" ASASSN-V J045615.72+402741.1
Type: SR
# Max. Min./Amp. JD0 Period
14.060 g Y 0.200 g 2458333.96600 229.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:15.73 +40:27:41.1: 12.64 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:15.73 +40:27:41.1: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045615.72+402741.1,2461289.7513,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045615.72+402741.1 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.61 04:18:23.09 +33:07:48.1
165.22114 -12.25925 galactic Per Second-epoch detections are separated by 3.1" and 6.9 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 175660657713618304 | 04:18:23.09 +33:07:47.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.961+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:18:23.09 +33:07:48.1: 12.62 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:18:23.09 +33:07:48.1: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 18 23.09 +33 07 48.1 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 175660657713618304,2461289.7513,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 175660657713618304 20260906.2513 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.69 04:56:43.63 +41:20:50.2
164.13689 -1.11112 galactic Aur Second-epoch detections are separated by 1.4" and 7.2 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 201641189767470080 | 04:56:43.69 +41:20:49.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.265+/-0.030 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:43.63 +41:20:50.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:43.63 +41:20:50.2: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201641189767470080,2461289.7513,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201641189767470080 20260906.2513 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.68 04:54:51.37 +40:41:54.7
164.42143 -1.79265 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 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 | Large-amplitude variable Gaia DR2 200118404818349184 | 04:54:51.43 +40:41:54.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.328+/-0.033 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:51.37 +40:41:54.7: 12.61 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:51.37 +40:41:54.7: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 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 200118404818349184,2461289.7513,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 200118404818349184 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.69 04:59:55.93 +41:06:08.7
164.70309 -0.79075 galactic Aur Second-epoch detections are separated by 1.9" and 7.3 pix
The object was found in VSX 2" ASASSN-V J045955.96+410609.3
Type: ROT
# Max. Min./Amp. JD0 Period
13.410 g Y 0.170 g 2459444.07000 6.245200000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:55.93 +41:06:08.7: 12.60 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:55.93 +41:06:08.7: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045955.96+410609.3,2461289.7513,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045955.96+410609.3 20260906.2513 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.66 04:59:27.41 +42:00:20.7
163.93781 -0.30257 galactic Aur Second-epoch detections are separated by 2.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 201779182774049664 | 04:59:27.42 +42:00:22.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G3 (LAMOST DR5) J-Ks=0.401+/-0.031 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:27.41 +42:00:20.7: 12.60 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:27.41 +42:00:20.7: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 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 201779182774049664,2461289.7513,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 201779182774049664 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.60 05:01:52.17 +42:12:30.6
164.05352 0.17488 galactic Aur Second-epoch detections are separated by 1.6" and 7.5 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 201802852333528064 | 05:01:48.17 +42:12:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1958ApJS....4....1M LF 7 +42 151
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:52.17 +42:12:30.6: 12.60 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:52.17 +42:12:30.6: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201802852333528064,2461289.7513,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201802852333528064 20260906.2513 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.63 04:17:37.89 +33:42:21.2
164.68814 -11.96814 galactic Per Second-epoch detections are separated by 0.7" and 7.2 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 175741063797822848 | 04:17:37.91 +33:42:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.017+/-0.030 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:17:37.89 +33:42:21.2: 12.58 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:17:37.89 +33:42:21.2: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 17 37.89 +33 42 21.2 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 175741063797822848,2461289.7513,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 175741063797822848 20260906.2513 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.66 04:58:55.90 +42:01:51.1
163.85770 -0.36363 galactic Aur Second-epoch detections are separated by 0.8" and 7.2 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 | ATO J074.7282+42.0238 | 04:58:55.88 +42:01:51.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G9 (LAMOST DR5) J-Ks=0.681+/-0.031 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:55.90 +42:01:51.1: 12.60 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:55.90 +42:01:51.1: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.7282+42.0238,2461289.7513,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.7282+42.0238 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.58 04:58:14.04 +41:20:56.9
164.31160 -0.88872 galactic Aur Second-epoch detections are separated by 0.9" and 7.3 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 201650020220230144 | 04:58:14.09 +41:20:56.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.380+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:14.04 +41:20:56.9: 12.58 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:14.04 +41:20:56.9: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201650020220230144,2461289.7513,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201650020220230144 20260906.2513 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.57 04:57:02.40 +41:06:06.8
164.36537 -1.21833 galactic Aur Second-epoch detections are separated by 0.4" and 7.4 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 201621810872066048 | 04:57:02.42 +41:06:07.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.766+/-0.036 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:02.40 +41:06:06.8: 12.56 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:02.40 +41:06:06.8: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201621810872066048,2461289.7513,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201621810872066048 20260906.2513 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.66 04:57:02.56 +40:36:38.0
164.74983 -1.52441 galactic Aur Second-epoch detections are separated by 1.3" and 7.3 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 201558588953500672 | 04:57:02.50 +40:36:37.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.724+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:02.56 +40:36:38.0: 12.57 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:02.56 +40:36:38.0: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201558588953500672,2461289.7513,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201558588953500672 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.57 04:56:06.03 +40:41:36.7
164.57333 -1.61210 galactic Aur Second-epoch detections are separated by 0.8" and 7.4 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 200109363908584576 | 04:56:05.98 +40:41:35.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.676+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:06.03 +40:41:36.7: 12.56 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:06.03 +40:41:36.7: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 200109363908584576,2461289.7513,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 200109363908584576 20260906.2513 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.59 04:55:03.05 +40:40:19.5
164.46522 -1.78057 galactic Aur Second-epoch detections are separated by 2.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.7669+40.6789 | 04:55:03.05 +40:40:20.0 (Gaia DR3) | CBF (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.284+/-0.033 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:03.05 +40:40:19.5: 12.54 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:03.05 +40:40:19.5: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.7669+40.6789,2461289.7513,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J073.7669+40.6789 20260906.2513 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.52 04:58:06.04 +41:18:52.3
164.32317 -0.92983 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 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 201649504824156160 | 04:58:06.21 +41:18:53.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.216+/-0.038 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:06.04 +41:18:52.3: 12.53 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:06.04 +41:18:52.3: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201649504824156160,2461289.7513,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201649504824156160 20260906.2513 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.54 04:58:58.26 +41:32:00.9
164.25260 -0.66597 galactic Aur Second-epoch detections are separated by 0.1" and 7.3 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 J074.7351+41.5322 | 04:58:58.35 +41:32:00.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.358+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:58.26 +41:32:00.9: 12.52 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:58.26 +41:32:00.9: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.7351+41.5322,2461289.7513,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.7351+41.5322 20260906.2513 11.54CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.56 04:56:46.56 +41:00:13.4
164.41102 -1.31849 galactic Aur Second-epoch detections are separated by 3.0" and 7.2 pix
The object was found in VSX18" Gaia DR3 201615149381977472
Type: ROT
# Max. Min./Amp. JD0 Period
15.730 G 15.790 G G
ATTENTION: measured mag 11.56 is 4.2 mag brighter than the VSX record maximum brightness 15.73 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:46.56 +41:00:13.4: 12.50 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:46.56 +41:00:13.4: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201615149381977472,2461289.7513,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201615149381977472 20260906.2513 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.44 04:56:50.77 +40:43:40.9
164.63474 -1.48023 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 pix
The object was found in VSX 1" ASASSN-V J045650.83+404342.1
Type: SR
# Max. Min./Amp. JD0 Period
13.920 g Y 0.200 g 2459084.04600 39.680000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:50.77 +40:43:40.9: 12.48 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:50.77 +40:43:40.9: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045650.83+404342.1,2461289.7513,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045650.83+404342.1 20260906.2513 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.49 04:58:47.68 +41:24:10.8
164.33463 -0.77281 galactic Aur Second-epoch detections are separated by 2.0" and 7.2 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 201655552138105472 | 04:58:47.95 +41:24:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:47.68 +41:24:10.8: 12.51 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:47.68 +41:24:10.8: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201655552138105472,2461289.7513,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201655552138105472 20260906.2513 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.52 04:39:27.68 +40:01:25.1
163.04034 -4.46712 galactic Per Second-epoch detections are separated by 1.7" and 7.3 pix
The object was found in VSX 2" ASASSN-V J043927.84+400124.9
Type: SRS
# Max. Min./Amp. JD0 Period
12.760 V 12.860 V 2457228.11700 27.043000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:39:27.68 +40:01:25.1: 12.49 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:39:27.68 +40:01:25.1: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 39 27.68 +40 01 25.1 11.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J043927.84+400124.9,2461289.7513,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J043927.84+400124.9 20260906.2513 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.62 05:00:34.76 +40:59:23.3
164.86699 -0.76409 galactic Aur Second-epoch detections are separated by 1.0" and 7.3 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 J075.1448+40.9898 | 05:00:34.76 +40:59:23.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.026 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:34.76 +40:59:23.3: 12.49 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:34.76 +40:59:23.3: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.1448+40.9898,2461289.7513,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.1448+40.9898 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.40 05:01:49.62 +41:41:01.7
164.46327 -0.15295 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 pix
The object was found in VSX 1" ASASSN-V J050149.69+414101.4
Type: SR
# Max. Min./Amp. JD0 Period
12.850 V 13.050 V 2457319.92400 41.260000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:49.62 +41:41:01.7: 12.52 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:49.62 +41:41:01.7: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050149.69+414101.4,2461289.7513,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050149.69+414101.4 20260906.2513 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.62 04:09:54.24 +34:17:01.2
163.10720 -12.68489 galactic Per Second-epoch detections are separated by 1.3" and 7.3 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 J062.4760+34.2836 | 04:09:54.24 +34:17:01.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.221+/-0.044 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:09:54.24 +34:17:01.2: 12.46 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:09:54.24 +34:17:01.2: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 09 54.24 +34 17 01.2 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J062.4760+34.2836,2461289.7513,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J062.4760+34.2836 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.53 04:54:40.40 +40:30:57.8
164.54155 -1.93438 galactic Aur Second-epoch detections are separated by 2.6" and 6.9 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 200112009611839616 | 04:54:40.40 +40:30:57.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.672+/-0.033 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:40.40 +40:30:57.8: 12.45 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:40.40 +40:30:57.8: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 200112009611839616,2461289.7513,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 200112009611839616 20260906.2513 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.43 04:56:43.57 +41:04:49.3
164.34527 -1.27797 galactic Aur Second-epoch detections are separated by 1.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1849+41.0702 | 04:56:43.62 +41:04:48.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.718+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:43.57 +41:04:49.3: 12.43 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:43.57 +41:04:49.3: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.1849+41.0702,2461289.7513,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.1849+41.0702 20260906.2513 11.43CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.43 05:01:28.85 +41:51:01.1
164.29217 -0.10181 galactic Aur Second-epoch detections are separated by 1.5" and 7.2 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 201735782126177408 | 05:01:28.81 +41:51:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.900+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:28.85 +41:51:01.1: 12.41 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:28.85 +41:51:01.1: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201735782126177408,2461289.7513,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201735782126177408 20260906.2513 11.43CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.47 04:58:30.12 +41:31:49.7
164.20062 -0.73676 galactic Aur Second-epoch detections are separated by 1.6" and 7.6 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 201670258106123264 | 04:58:30.18 +41:31:50.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.167+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:30.12 +41:31:49.7: 12.41 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:30.12 +41:31:49.7: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201670258106123264,2461289.7513,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201670258106123264 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.38 04:56:23.92 +41:08:21.6
164.26066 -1.28928 galactic Aur Second-epoch detections are separated by 1.2" and 7.4 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 201637272754328448 | 04:56:23.84 +41:08:22.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.412+/-0.033 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:23.92 +41:08:21.6: 12.37 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:23.92 +41:08:21.6: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201637272754328448,2461289.7513,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201637272754328448 20260906.2513 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.37 04:55:17.17 +40:33:49.6
164.57760 -1.81382 galactic Aur Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.8208+40.5634 | 04:55:17.01 +40:33:48.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.980+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:17.17 +40:33:49.6: 12.34 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:17.17 +40:33:49.6: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.8208+40.5634,2461289.7513,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J073.8208+40.5634 20260906.2513 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.35 04:54:52.37 +40:30:58.9
164.56517 -1.90471 galactic Aur Second-epoch detections are separated by 3.0" and 7.2 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 200111803450019712 | 04:54:52.33 +40:30:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.779+/-0.032 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:52.37 +40:30:58.9: 12.33 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:52.37 +40:30:58.9: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 200111803450019712,2461289.7513,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 200111803450019712 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.33 05:01:37.66 +42:05:05.4
164.12373 0.06364 galactic Aur Second-epoch detections are separated by 1.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.4073+42.0845 | 05:01:37.76 +42:05:04.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.212+/-0.040 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:37.66 +42:05:05.4: 12.34 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:37.66 +42:05:05.4: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.4073+42.0845,2461289.7513,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.4073+42.0845 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.26 05:01:47.51 +41:46:31.9
164.38678 -0.10191 galactic Aur Second-epoch detections are separated by 0.2" and 7.4 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 J075.4479+41.7752 | 05:01:47.26 +41:46:56.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.655+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:47.51 +41:46:31.9: 12.22 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:47.51 +41:46:31.9: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.4479+41.7752,2461289.7513,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J075.4479+41.7752 20260906.2513 11.26CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.21 04:18:24.02 +33:22:35.1
165.04327 -12.08465 galactic Per Second-epoch detections are separated by 0.8" and 7.2 pix
The object was found in VSX 1" ASASSN-V J041824.00+332234.5
Type: SR
# Max. Min./Amp. JD0 Period
13.370 g Y 0.200 g 2459268.75500 36.560000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:18:24.02 +33:22:35.1: 12.23 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:18:24.02 +33:22:35.1: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 18 24.02 +33 22 35.1 11.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J041824.00+332234.5,2461289.7513,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J041824.00+332234.5 20260906.2513 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.35 04:52:37.96 +40:11:17.8
164.55036 -2.44282 galactic Aur Second-epoch detections are separated by 0.9" and 7.1 pix
The object was found in VSX 1" ASASSN-V J045237.98+401118.6
Type: SR
# Max. Min./Amp. JD0 Period
13.490 g Y 0.120 g 2459172.81600 44.330000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:52:37.96 +40:11:17.8: 12.22 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:52:37.96 +40:11:17.8: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045237.98+401118.6,2461289.7513,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045237.98+401118.6 20260906.2513 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.27 04:56:06.36 +41:17:31.2
164.10709 -1.23670 galactic Aur Second-epoch detections are separated by 0.7" and 7.4 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 201827183327859840 | 04:56:06.44 +41:17:30.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.096+/-0.035 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:06.36 +41:17:31.2: 12.22 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:06.36 +41:17:31.2: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201827183327859840,2461289.7513,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201827183327859840 20260906.2513 11.27CV 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
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.11 04:57:00.10 +41:12:54.8
164.27227 -1.15327 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 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 J074.2368+41.2094 | 04:56:59.93 +41:12:56.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:00.10 +41:12:54.8: 12.07 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:00.10 +41:12:54.8: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.2368+41.2094,2461289.7513,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J074.2368+41.2094 20260906.2513 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.17 04:15:22.69 +32:59:33.5
164.86831 -12.80432 galactic Per Second-epoch detections are separated by 0.8" and 7.3 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 169700209477997056 | 04:15:22.63 +32:59:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.187+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:15:22.69 +32:59:33.5: 12.07 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:15:22.69 +32:59:33.5: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 06.2513* 04 15 22.69 +32 59 33.5 11.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 169700209477997056,2461289.7513,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 169700209477997056 20260906.2513 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2513 2461289.7513 11.04 05:01:52.16 +41:48:37.7
164.36802 -0.06908 galactic Aur Second-epoch detections are separated by 0.5" and 7.5 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 201733102064655104 | 05:01:52.16 +41:48:37.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.055+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:01:52.16 +41:48:37.7: 12.02 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:01:52.16 +41:48:37.7: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 201733102064655104,2461289.7513,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 201733102064655104 20260906.2513 11.04CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
First image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Last image: 2461289.75158118 06.09.2026 06:02:06.614 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 18
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 16213
Objects passed selection criteria: 16113
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 10208
Average stars matched: 9589 (93.9361 %)
Memory usage VmPeak: 242664 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 6 01:04:19 CDT 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: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
First image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Last image: 2461289.75158118 06.09.2026 06:02:06.614 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 484
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 19 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 119573
Objects passed selection criteria: 119225
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 77739
Average stars matched: 72201.5 (92.8768 %)
Memory usage VmPeak: 586040 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 6 01:05:15 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> '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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
SExtractor catalog cache: saved Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.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/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.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: 2461289.75101734
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits exists and is non-empty
wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits exists and is non-empty
wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits exists and is non-empty
wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (1st reference image)
verification OK: wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:49.059 +37:59:50.85 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits (1st new image)
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
Image size: 943.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:56.087 +38:00:44.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:21:49.059 +37:59:50.85
Second-epoch image center 04:21:56.087 +38:00:44.26
Angular distance between the image centers 0.0274 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits (2nd new image)
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
Image size: 943.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:53.933 +38:00:10.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:21:49.059 +37:59:50.85
Second-epoch image center 04:21:53.933 +38:00:10.95
Angular distance between the image centers 0.0169 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:21:56.087 +38:00:44.26
Second-epoch second image center 04:21:53.933 +38:00:10.95
Angular distance between the image centers 0.01165 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits &> /tmp/tmp.bUSBFCYOdZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits &> /tmp/tmp.2DNoRsUvHt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits &> /tmp/tmp.6OhPgrhNAu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits &> /tmp/tmp.cCRtGbi4f9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
Found non-empty wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
The reference image (wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits) and catalog (wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat) found
'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat' -> 'wcsmag.cat'
Read 18677 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9661 to 76.3326 deg, Dec +32.1948 to +43.3141 deg
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
Tycho-2 catalog search boundaries: RA 54.9661 to 76.3326 deg, Dec 32.1948 to 43.3141 deg
Loaded 9192 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6385 out of 7127 total matches.
Matched with Tycho-2 7127 out of 18677 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.973500
a=0.000000 b=1.000000 c=22.973500
From vast_summary.log: estimated ref. image limiting mag.: -7.58
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
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 18677 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9661 to 76.3326 deg, Dec +32.1948 to +43.3141 deg
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
Tycho-2 catalog search boundaries: RA 54.9661 to 76.3326 deg, Dec 32.1948 to 43.3141 deg
Loaded 9192 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6385 out of 7127 total matches.
Matched with Tycho-2 7127 out of 18677 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Forced-photometry filter: calibrated wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -> calib.txt_param_ref_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (aperture=6.0)
Read 18569 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.4956 to 75.7898 deg, Dec +32.0248 to +43.3806 deg
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
Tycho-2 catalog search boundaries: RA 54.4956 to 75.7898 deg, Dec 32.0248 to 43.3806 deg
Loaded 9219 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6462 out of 7192 total matches.
Matched with Tycho-2 7192 out of 18569 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Forced-photometry filter: calibrated wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits -> calib.txt_param_ref_wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
2.1 pix Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
2.5 pix fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
2.5 pix fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
Limiting magnitude estimates:
15.4 mag. Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
15.4 mag. Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
12.4 mag. fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
12.6 mag. fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 10.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.bUSBFCYOdZ (6) ############
Parsing command line arguments...
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_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1808, bad_region=0, passed=18677
Got 18677 stars (including 16842 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
util/solve_plate_with_UCAC5 got 18677 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 4856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 18677 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 18677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 18677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4856 stars left (next iteration limit 5341)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits N_match=4856 sigma_overall_arcsec=0.308 sigma_q1_arcsec=0.418 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.271 sigma_q4_arcsec=0.245 n_q1=1609 n_q2=1204 n_q3=763 n_q4=1280 worst_quadrant_to_overall_ratio=1.356
The image catalog is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -region wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.2DNoRsUvHt (6) ############
Parsing command line arguments...
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_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits' -> 'wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat corresponding to the image wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat corresponding to the image wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1757, bad_region=0, passed=18569
Got 18569 stars (including 16779 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat
util/solve_plate_with_UCAC5 got 18569 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 4857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 18569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 18569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 18569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4857 stars left (next iteration limit 5342)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits N_match=4857 sigma_overall_arcsec=0.390 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.394 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.351 n_q1=1197 n_q2=768 n_q3=1133 n_q4=1759 worst_quadrant_to_overall_ratio=1.371
The image catalog is written to wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits -region wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.6OhPgrhNAu (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_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.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_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits.wcscat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits.wcscat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=94, bad_region=1, passed=1835
Got 1835 stars (including 1734 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits.wcscat
util/solve_plate_with_UCAC5 got 1835 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.3'
Seting catalog search parameters based on the expected field of view 943.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013101 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010481 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 1685 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1670 matched stars entering correct_measured_positions(), 1654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1670 matched stars entering correct_measured_positions(), 1815 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 1685 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1670 matched stars entering correct_measured_positions(), 1815 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 1670 matched stars entering correct_measured_positions(), 1815 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 1670 stars left (next iteration limit 1837)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1670 robust_rms=12.030 arcsec worst_quadrant_rms=15.097 arcsec
SIP_REFIT: SIP order 3 trial: matched=1670 robust_rms=0.592 arcsec worst_quadrant_rms=0.704 arcsec
SIP_REFIT: SIP order 5 trial: matched=1670 robust_rms=0.426 arcsec worst_quadrant_rms=0.509 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1670 robust_rms_before=1.181 arcsec robust_rms_before_corrected=0.451 arcsec robust_rms_after=0.426 arcsec worst_quadrant_rms_before=0.567 worst_quadrant_rms_after=0.509
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
Image size: 943.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:56.167 +38:00:43.06 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1835 stars ###
'wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/correct_sextractor_wcs_catalog_usingxy2sky1173015.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.181 -> 0.426 arcsec)
WCS_QUALITY_DIAG: file=fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits N_match=1670 sigma_overall_arcsec=0.413 sigma_q1_arcsec=0.373 sigma_q2_arcsec=0.524 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.485 n_q1=345 n_q2=162 n_q3=673 n_q4=490 worst_quadrant_to_overall_ratio=1.271
The image catalog is written to wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits -region wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.cCRtGbi4f9 (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_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.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_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits.wcscat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits.wcscat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=95, bad_region=0, passed=2088
Got 2088 stars (including 1983 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits.wcscat
util/solve_plate_with_UCAC5 got 2088 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.2'
Seting catalog search parameters based on the expected field of view 943.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013100 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010480 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 1929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1915 matched stars entering correct_measured_positions(), 1899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1915 matched stars entering correct_measured_positions(), 2067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 1929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1914 matched stars entering correct_measured_positions(), 2066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 1914 matched stars entering correct_measured_positions(), 2066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 1914 stars left (next iteration limit 2106)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1914 robust_rms=12.263 arcsec worst_quadrant_rms=14.325 arcsec
SIP_REFIT: SIP order 3 trial: matched=1914 robust_rms=0.523 arcsec worst_quadrant_rms=0.636 arcsec
SIP_REFIT: SIP order 5 trial: matched=1914 robust_rms=0.409 arcsec worst_quadrant_rms=0.474 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1914 robust_rms_before=1.097 arcsec robust_rms_before_corrected=0.445 arcsec robust_rms_after=0.409 arcsec worst_quadrant_rms_before=0.568 worst_quadrant_rms_after=0.474
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
Image size: 943.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:54.008 +38:00:09.84 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 2088 stars ###
'wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/correct_sextractor_wcs_catalog_usingxy2sky1173101.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.097 -> 0.409 arcsec)
WCS_QUALITY_DIAG: file=fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits N_match=1914 sigma_overall_arcsec=0.432 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.504 sigma_q3_arcsec=0.373 sigma_q4_arcsec=0.506 n_q1=387 n_q2=179 n_q3=745 n_q4=603 worst_quadrant_to_overall_ratio=1.172
The image catalog is written to wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits -region wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits to local_wcs_cache/
'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'local_wcs_cache/wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
Saving the final (post-refit) wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits to local_wcs_cache/
'wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits' -> 'local_wcs_cache/wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits'
Saving the final (post-refit) wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits to local_wcs_cache/
'wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits'
Saving the final (post-refit) wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits to local_wcs_cache/
'wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits sigma_overall=0.308 worst_q_ratio=1.356
ref2=Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits sigma_overall=0.390 worst_q_ratio=1.371
new1=fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits sigma_overall=0.413 worst_q_ratio=1.271
new2=fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits sigma_overall=0.432 worst_q_ratio=1.172
reference average sigma_overall=0.349 worst_q_ratio=1.3635
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342_astrometric_residuals.png (4856 matched stars from wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025_astrometric_residuals.png (4857 matched stars from wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151_astrometric_residuals.png (1670 matched stars from wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152_astrometric_residuals.png (1914 matched stars from wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/wcs_fd_Per-05-Q1b1x1_2026-09-06_01-01-17_20.00sec_-0.00C_LIGHTs_0151.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Per-05-Q1b1x1_010245_TTUQ1b1x1_1144910_sBU3BmsY/wcs_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152.fits'
Preparing the HTML report for the field Per-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 0s
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Considering the candidate 18410_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 18410_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:55:30.35 +32:47:02.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 17551_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 17551_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:55.38 +33:00:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16254_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 16254_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:58:05.53 +33:44:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16443_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 16443_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:43.02 +33:39:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18487_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 18487_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:54:23.56 +32:48:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18062_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 18062_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:49.52 +33:23:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18660_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 18660_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
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Considering the candidate 168950_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 168950_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 03:53:53.31 +36:58:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168952_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 168952_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:04:12.16 +43:02:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169051_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 169051_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
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Considering the candidate 169128_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 169128_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:08:05.74 +43:11:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169181_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 169181_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 03:48:34.71 +40:56:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169193_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 169193_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
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Considering the candidate 169295_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 169295_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 03:43:40.42 +42:35:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96764_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 96764_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:54:23.58 +32:48:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92603_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 92603_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
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Considering the candidate 94406_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94406_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
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Considering the candidate 14974_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 14974_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
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Considering the candidate 15702_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 15702_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
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Considering the candidate 95708_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 95708_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
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Considering the candidate 17582_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 17582_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
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Considering the candidate 08311_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 08311_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 19495_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 19495_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 05:01:09.79 +41:35:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96955_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 96955_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:54:28.76 +32:49:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97531_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 97531_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:05.46 +32:50:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13494_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 13494_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16639_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 16639_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07867_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 07867_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08932_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 08932_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40618_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 40618_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19213_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 19213_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10562_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 10562_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95863_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 95863_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:55:35.19 +32:41:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13760_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 13760_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 40438_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 40438_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 95427_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 95427_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93291_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 93291_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08043_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 08043_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
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Considering the candidate 22671_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 22671_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 09194_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 09194_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06493_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 06493_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08878_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 08878_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 06239_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 06239_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52541_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 52541_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:50:00.83 +39:55:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18912_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 18912_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 18179_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 18179_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 48175_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 48175_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53575_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 53575_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09779_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 09779_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27115_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 27115_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 20214_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 20214_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 26079_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 26079_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 26704_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 26704_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25854_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 25854_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15867_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 15867_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51269_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 51269_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04248_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 04248_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32304_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 32304_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61537_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 61537_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 40384_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 40384_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14255_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 14255_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24326_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 24326_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 49445_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 49445_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64710_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 64710_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15450_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 15450_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06491_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 06491_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50539_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 50539_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53306_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 53306_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66422_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 66422_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 21639_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 21639_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07642_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 07642_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58754_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 58754_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20338_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 20338_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20316_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 20316_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43217_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 43217_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32901_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 32901_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15457_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 15457_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21240_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 21240_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28525_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 28525_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13715_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 13715_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24920_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 24920_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57861_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 57861_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21993_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 21993_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57075_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 57075_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65662_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 65662_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19572_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 19572_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23284_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 23284_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41777_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 41777_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43433_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 43433_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59054_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 59054_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36843_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 36843_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44985_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 44985_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45161_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 45161_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24988_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 24988_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26787_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 26787_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56995_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 56995_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99610_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 99610_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54508_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 54508_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26894_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 26894_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17341_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 17341_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39397_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 39397_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 10172_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 10172_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55444_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 55444_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51191_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 51191_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 47850_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 47850_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115764_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 115764_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:09:54.88 +35:34:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53165_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 53165_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 13079_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 13079_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 95782_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 95782_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135303_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 135303_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94286_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94286_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30092_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 30092_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 24658_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 24658_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23838_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 23838_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 03:56:15.76 +41:59:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53525_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 53525_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19141_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 19141_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27585_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 27585_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25702_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 25702_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136051_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 136051_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:55:42.96 +33:09:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55546_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 55546_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54760_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 54760_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39433_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 39433_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40249_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 40249_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54686_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 54686_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29596_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 29596_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95901_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 95901_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12413_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 12413_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73635_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 73635_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:23:36.60 +38:38:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22974_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 22974_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27894_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 27894_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40728_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 40728_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11992_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 11992_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32240_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 32240_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11745_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 11745_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72045_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 72045_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26404_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 26404_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21801_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 21801_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18229_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 18229_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19438_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 19438_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21197_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 21197_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27167_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 27167_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23203_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 23203_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40022_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 40022_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12866_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 12866_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96258_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 96258_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:54:41.64 +32:45:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129828_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 129828_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110714_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 110714_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:48.08 +33:16:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09676_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 09676_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07666_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 07666_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12648_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 12648_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43075_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 43075_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50384_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 50384_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37001_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 37001_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49178_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 49178_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15604_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 15604_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29426_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 29426_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97002_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 97002_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:10.57 +32:45:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136924_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 136924_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:05.68 +33:13:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56620_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 56620_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13340_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 13340_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08197_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 08197_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19530_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 19530_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125277_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 125277_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96524_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 96524_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:54:57.11 +32:46:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06650_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 06650_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72716_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 72716_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08774_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 08774_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40054_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 40054_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54966_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 54966_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:37:54.06 +39:56:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18203_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 18203_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07391_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 07391_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12645_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 12645_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34741_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 34741_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41589_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 41589_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13620_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 13620_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23549_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 23549_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:00:21.05 +42:02:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10021_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 10021_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42838_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 42838_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95781_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 95781_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103893_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 103893_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92813_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 92813_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27387_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 27387_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96147_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 96147_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34429_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 34429_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11218_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 11218_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131087_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 131087_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51097_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 51097_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42890_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 42890_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10283_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 10283_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17883_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 17883_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16969_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 16969_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16281_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 16281_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108791_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 108791_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:33.54 +33:19:56.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25633_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 25633_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42328_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 42328_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108062_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 108062_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30058_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 30058_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18519_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 18519_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36282_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 36282_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13367_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 13367_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19416_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 19416_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93427_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 93427_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06377_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 06377_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14045_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 14045_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136723_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 136723_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26179_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 26179_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21909_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 21909_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129495_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 129495_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29240_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 29240_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115519_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 115519_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:15:40.64 +35:31:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18272_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 18272_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93959_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 93959_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96981_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 96981_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:36.46 +32:46:02.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25031_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 25031_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08166_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 08166_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26477_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 26477_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100529_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 100529_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:53.56 +33:33:45.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16765_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 16765_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36313_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 36313_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45835_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 45835_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129636_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 129636_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97185_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 97185_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:54:18.88 +32:50:29.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37951_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 37951_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43555_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 43555_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27874_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 27874_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27408_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 27408_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10020_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 10020_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13132_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 13132_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46792_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 46792_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23718_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 23718_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28323_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 28323_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06923_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 06923_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27021_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 27021_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47808_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 47808_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96657_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 96657_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:43.51 +32:44:23.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13441_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 13441_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102798_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 102798_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:30.20 +33:28:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10922_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 10922_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93012_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 93012_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98366_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 98366_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119826_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 119826_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:15:16.94 +35:54:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24687_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 24687_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99814_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 99814_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31600_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 31600_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28954_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 28954_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23390_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 23390_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26269_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 26269_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
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Considering the candidate 17944_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 17944_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07865_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 07865_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41560_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 41560_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94923_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 94923_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25764_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 25764_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104316_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 104316_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:25:25.59 +34:44:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38157_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 38157_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09796_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 09796_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28719_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 28719_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12445_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 12445_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94559_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94559_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07362_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 07362_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136050_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 136050_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12239_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 12239_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40705_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 40705_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:47.06 +40:30:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25099_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 25099_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93112_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 93112_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30030_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 30030_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15766_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 15766_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97023_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 97023_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:43.33 +32:46:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38728_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 38728_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37760_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 37760_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38100_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 38100_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92862_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 92862_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94950_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94950_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25768_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 25768_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47653_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 47653_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:15.98 +40:04:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21604_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 21604_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31818_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 31818_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36723_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 36723_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24148_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 24148_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17226_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 17226_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 05:01:20.62 +41:41:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93840_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 93840_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53949_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 53949_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18581_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 18581_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30222_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 30222_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94911_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94911_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136024_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 136024_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:57.00 +33:06:50.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 17377_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 17377_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07463_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 07463_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 05:01:48.01 +42:12:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107514_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 107514_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09765_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 09765_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16380_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 16380_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41342_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 41342_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30547_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 30547_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135420_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 135420_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:27:22.79 +33:35:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136170_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 136170_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:38.02 +33:07:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14492_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 14492_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21937_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 21937_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06555_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 06555_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29652_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 29652_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96686_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 96686_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:20:11.40 +33:17:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08530_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 08530_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16309_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 16309_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94525_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94525_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40246_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 40246_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18971_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 18971_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13754_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 13754_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41202_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 41202_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13550_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 13550_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09929_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 09929_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105502_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 105502_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:34.72 +33:26:31.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21523_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 21523_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06956_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 06956_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94573_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94573_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94541_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94541_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15641_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 15641_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97539_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 97539_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47370_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 47370_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107388_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 107388_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:25.89 +33:22:43.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26550_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 26550_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94339_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94339_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12504_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 12504_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:58.46 +42:03:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100293_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 100293_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:55:42.29 +33:12:45.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109445_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 109445_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:03.73 +33:17:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27937_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 27937_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93412_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 93412_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92980_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 92980_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92722_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 92722_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09734_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 09734_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 05:03:18.50 +42:03:04.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14944_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
Preparing report for the candidate 14944_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97627_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 97627_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:46.92 +32:49:36.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94071_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94071_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100385_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 100385_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:04.53 +33:29:13.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100281_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 100281_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:57.90 +33:05:59.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92879_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 92879_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100354_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 100354_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:01.30 +33:24:10.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129173_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 129173_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:52.07 +33:33:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94847_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 94847_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97118_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 97118_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:24.41 +32:45:56.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97309_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 97309_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:02.19 +32:47:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135713_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 135713_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:55:50.31 +33:08:15.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100072_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 100072_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:27.05 +33:03:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104458_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 104458_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:49.04 +33:26:59.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97164_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 97164_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:55:19.30 +32:49:12.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99576_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 99576_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:55.36 +33:00:15.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100809_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 100809_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:58:05.48 +33:44:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136549_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 136549_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:57:43.03 +33:39:59.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02995_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 02995_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 03:51:50.88 +43:02:47.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106739_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 106739_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:49.56 +33:23:12.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96696_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 96696_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:55:30.40 +32:47:01.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101165_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 101165_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:20:24.58 +34:34:02.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24193_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 24193_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 05:02:28.30 +41:04:30.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135996_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152
The candidate 135996_fd_Per-05-Q1b1x1_2026-09-06_01-02-06_20.00sec_-0.00C_LIGHTs_0152 did not pass the final checks
**** FOUND 04:56:59.44 +33:09:57.1 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 14s
make_report_in_HTML.sh TOTAL: 304s
Prepared the HTML report for the field Per-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:57:36.87 +42:23:16.7
05:01:52.17 +42:12:30.6
04:59:20.73 +42:14:03.0
05:00:38.49 +42:11:35.2
05:01:33.32 +42:10:38.4
05:01:36.22 +42:07:32.6
05:01:37.66 +42:05:05.4
05:01:27.07 +42:04:34.8
04:58:55.95 +42:08:02.7
05:00:33.80 +42:05:03.7
04:08:51.36 +34:22:14.8
04:09:54.24 +34:17:01.2
04:21:51.52 +33:53:49.8
05:00:24.45 +42:03:37.6
05:01:32.97 +42:00:47.2
04:58:08.84 +42:03:26.8
04:58:55.90 +42:01:51.1
05:01:35.12 +41:56:43.7
04:59:27.41 +42:00:20.7
04:17:22.94 +36:19:02.5
04:57:59.44 +42:02:10.4
04:59:07.41 +41:59:26.9
04:23:10.25 +34:32:53.9
04:44:37.96 +36:19:20.5
04:08:25.99 +34:20:03.2
05:01:54.98 +41:54:01.4
04:08:46.93 +34:32:47.8
05:01:58.51 +41:53:11.0
05:00:26.58 +41:55:28.2
04:20:31.63 +33:37:33.2
04:17:37.89 +33:42:21.2
05:00:43.34 +41:54:22.8
04:12:30.16 +34:12:09.6
03:52:17.78 +42:29:02.4
05:00:58.13 +41:53:30.8
04:57:04.27 +41:58:49.5
03:51:06.48 +42:26:37.5
05:01:28.85 +41:51:01.1
05:01:52.16 +41:48:37.7
03:54:01.48 +42:24:58.9
03:47:51.06 +42:20:17.3
05:01:11.57 +41:47:07.6
05:01:47.51 +41:46:31.9
03:48:48.30 +42:19:43.5
05:00:27.75 +41:46:29.5
05:01:30.42 +41:43:11.5
04:58:38.55 +41:47:29.8
05:01:49.62 +41:41:01.7
05:01:30.01 +41:39:29.2
03:53:49.46 +42:15:40.9
04:59:32.68 +41:42:08.7
05:00:58.25 +41:39:16.5
05:01:46.93 +41:38:09.5
05:00:57.87 +41:38:25.1
03:51:04.96 +42:11:55.7
03:50:35.94 +42:10:30.5
04:56:20.68 +41:43:23.9
04:58:32.79 +41:38:59.4
03:51:37.56 +42:09:52.3
03:51:12.19 +42:07:35.2
03:49:51.43 +42:06:23.2
03:51:50.58 +42:07:48.8
04:59:28.78 +41:32:05.0
03:50:22.85 +42:03:43.6
04:58:58.26 +41:32:00.9
03:56:39.13 +42:06:02.7
04:59:20.66 +41:30:27.2
05:01:21.71 +41:26:28.6
04:58:30.12 +41:31:49.7
03:46:41.78 +41:58:24.7
03:48:10.95 +41:57:18.6
04:57:32.33 +41:29:46.8
03:51:03.50 +41:57:59.7
03:50:38.36 +41:57:28.3
04:59:21.33 +41:25:17.6
04:56:35.01 +41:29:30.3
04:58:47.68 +41:24:10.8
03:50:58.79 +41:54:33.5
03:51:00.85 +41:53:33.2
05:00:44.55 +41:18:33.5
03:54:16.87 +41:53:57.0
04:57:10.42 +41:22:55.7
04:58:32.67 +41:20:39.4
04:58:14.04 +41:20:56.9
04:57:15.99 +41:20:49.5
04:56:46.73 +41:21:39.2
04:56:43.63 +41:20:50.2
04:58:06.04 +41:18:52.3
03:51:22.81 +41:49:40.8
03:47:57.54 +41:46:17.6
04:57:24.43 +41:18:28.6
04:58:07.50 +41:17:15.6
04:56:53.62 +41:18:55.2
05:01:18.58 +41:11:29.6
04:56:06.36 +41:17:31.2
04:58:17.08 +41:15:54.7
03:48:01.97 +41:43:53.4
03:52:35.26 +41:46:36.2
04:56:55.24 +41:16:29.2
03:50:49.99 +41:45:03.2
04:57:58.54 +41:14:17.0
04:57:17.41 +41:14:55.8
05:01:00.05 +41:08:16.0
04:57:20.50 +41:14:23.1
04:58:12.89 +41:11:28.1
03:47:20.47 +41:39:38.4
04:57:00.10 +41:12:54.8
04:58:16.58 +41:09:54.5
04:57:28.14 +41:10:34.0
04:59:55.93 +41:06:08.7
04:57:29.45 +41:08:59.7
04:57:54.10 +41:07:37.0
04:57:50.90 +41:07:05.1
03:46:46.02 +41:33:42.1
04:56:23.92 +41:08:21.6
04:57:02.40 +41:06:06.8
04:55:10.24 +41:08:38.4
04:56:15.33 +41:07:15.6
05:00:34.76 +40:59:23.3
04:56:43.57 +41:04:49.3
05:00:04.13 +40:55:58.1
04:56:46.56 +41:00:13.4
04:55:29.69 +41:00:53.8
03:52:12.95 +41:28:22.4
03:46:13.97 +41:22:08.9
03:51:54.75 +41:20:59.5
04:56:36.30 +40:50:53.7
04:58:01.47 +40:43:28.5
04:54:31.05 +40:48:57.5
04:56:50.77 +40:43:40.9
03:47:50.31 +41:09:40.5
04:57:23.85 +40:41:33.9
04:56:06.03 +40:41:36.7
04:55:03.05 +40:40:19.5
04:54:51.37 +40:41:54.7
04:57:02.56 +40:36:38.0
03:52:40.27 +41:04:35.5
03:42:06.96 +40:56:32.0
04:53:31.48 +40:37:41.0
04:54:57.28 +40:35:27.8
04:55:17.17 +40:33:49.6
04:56:12.68 +40:32:52.5
03:45:53.65 +40:56:32.0
04:55:09.88 +40:33:03.2
04:53:06.39 +40:35:50.9
03:52:32.23 +40:59:48.4
04:54:52.37 +40:30:58.9
04:54:40.40 +40:30:57.8
04:56:15.73 +40:27:41.1
04:57:05.16 +40:26:37.1
03:43:49.29 +40:49:44.0
04:54:35.57 +40:27:52.2
04:53:59.81 +40:26:54.0
04:54:20.61 +40:25:29.2
04:55:17.06 +40:24:11.3
03:51:12.59 +40:50:11.7
03:44:50.45 +40:44:48.7
04:55:14.50 +40:22:32.9
03:50:27.52 +40:43:19.5
03:52:07.88 +40:43:49.4
04:56:10.90 +40:09:16.2
04:52:37.96 +40:11:17.8
04:52:35.42 +40:09:50.6
03:52:11.71 +40:33:50.8
03:49:35.78 +40:31:27.6
03:52:17.29 +40:29:03.9
03:48:43.39 +40:25:57.3
03:50:09.86 +40:22:49.0
03:52:26.94 +40:24:09.8
04:52:23.66 +39:58:22.9
03:44:08.15 +40:15:34.0
03:51:34.91 +40:20:52.4
04:40:22.43 +40:04:07.5
03:52:40.18 +40:13:30.4
03:52:50.85 +40:12:22.9
03:48:13.22 +40:09:25.5
04:39:27.68 +40:01:25.1
03:50:28.95 +40:07:07.8
03:46:29.67 +40:03:09.3
03:51:01.28 +40:06:04.2
03:44:54.77 +39:59:05.8
04:37:13.14 +39:57:31.9
03:47:46.30 +39:56:18.4
04:39:17.27 +39:49:43.5
03:48:56.91 +39:55:42.5
03:47:57.35 +39:51:30.5
03:44:51.49 +39:44:55.4
03:46:57.53 +39:45:21.5
03:51:22.42 +39:38:05.9
03:51:42.29 +39:24:03.1
03:47:53.99 +39:16:53.9
03:45:46.80 +39:11:32.7
03:48:46.02 +38:45:24.8
04:35:52.54 +38:38:30.5
04:18:31.62 +32:56:11.9
04:15:22.69 +32:59:33.5
04:06:28.59 +33:03:39.8
04:18:23.09 +33:07:48.1
04:05:22.71 +33:16:17.2
04:18:24.02 +33:22:35.1
04:04:59.54 +33:28:20.4
04:56:10.04 +33:01:16.7
04:20:16.08 +33:34:29.0
########### Completed Per-05-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:01:33.32 +42:10:38.4
04:53:06.39 +40:35:50.9
04:56:20.68 +41:43:23.9
05:00:58.13 +41:53:30.8
04:55:09.88 +40:33:03.2
03:48:10.95 +41:57:18.6
05:01:36.22 +42:07:32.6
03:51:04.96 +42:11:55.7
03:53:49.46 +42:15:40.9
03:49:35.78 +40:31:27.6
03:48:13.22 +40:09:25.5
03:50:49.99 +41:45:03.2
03:51:12.19 +42:07:35.2
03:47:57.54 +41:46:17.6
04:58:17.08 +41:15:54.7
03:51:22.81 +41:49:40.8
03:48:48.30 +42:19:43.5
03:51:34.91 +40:20:52.4
03:52:12.95 +41:28:22.4
03:51:22.42 +39:38:05.9
03:45:53.65 +40:56:32.0
03:51:06.48 +42:26:37.5
03:50:58.79 +41:54:33.5
03:48:43.39 +40:25:57.3
03:51:42.29 +39:24:03.1
03:54:01.48 +42:24:58.9
03:52:26.94 +40:24:09.8
03:52:40.18 +40:13:30.4
03:45:46.80 +39:11:32.7
03:56:39.13 +42:06:02.7
03:44:51.49 +39:44:55.4
03:51:50.58 +42:07:48.8
03:49:51.43 +42:06:23.2
03:51:12.59 +40:50:11.7
03:46:13.97 +41:22:08.9
03:47:51.06 +42:20:17.3
03:50:22.85 +42:03:43.6
04:57:28.14 +41:10:34.0
03:52:17.78 +42:29:02.4
03:54:16.87 +41:53:57.0
03:47:57.35 +39:51:30.5
03:46:41.78 +41:58:24.7
03:48:56.91 +39:55:42.5
03:47:53.99 +39:16:53.9
03:51:37.56 +42:09:52.3
03:50:38.36 +41:57:28.3
03:43:49.29 +40:49:44.0
03:44:50.45 +40:44:48.7
03:46:57.53 +39:45:21.5
03:47:50.31 +41:09:40.5
03:50:27.52 +40:43:19.5
03:52:07.88 +40:43:49.4
04:57:10.42 +41:22:55.7
03:48:01.97 +41:43:53.4
04:39:17.27 +39:49:43.5
04:56:10.04 +33:01:16.7
03:50:28.95 +40:07:07.8
03:52:35.26 +41:46:36.2
03:52:40.27 +41:04:35.5
04:58:55.95 +42:08:02.7
03:44:54.77 +39:59:05.8
03:44:08.15 +40:15:34.0
03:52:11.71 +40:33:50.8
04:40:22.43 +40:04:07.5
05:01:54.98 +41:54:01.4
04:20:31.63 +33:37:33.2
04:56:15.33 +41:07:15.6
03:51:00.85 +41:53:33.2
03:52:50.85 +40:12:22.9
03:50:35.94 +42:10:30.5
04:57:20.50 +41:14:23.1
04:56:46.73 +41:21:39.2
04:37:13.14 +39:57:31.9
03:51:01.28 +40:06:04.2
03:42:06.96 +40:56:32.0
04:56:12.68 +40:32:52.5
03:46:29.67 +40:03:09.3
03:46:46.02 +41:33:42.1
05:01:35.12 +41:56:43.7
04:57:32.33 +41:29:46.8
03:47:20.47 +41:39:38.4
03:52:32.23 +40:59:48.4
04:58:08.84 +42:03:26.8
04:55:29.69 +41:00:53.8
03:48:46.02 +38:45:24.8
04:56:53.62 +41:18:55.2
04:59:20.66 +41:30:27.2
05:00:58.25 +41:39:16.5
04:59:28.78 +41:32:05.0
04:57:58.54 +41:14:17.0
03:51:03.50 +41:57:59.7
04:53:31.48 +40:37:41.0
04:59:07.41 +41:59:26.9
04:08:25.99 +34:20:03.2
04:57:59.44 +42:02:10.4
04:55:17.06 +40:24:11.3
03:50:09.86 +40:22:49.0
04:57:23.85 +40:41:33.9
03:52:17.29 +40:29:03.9
05:01:11.57 +41:47:07.6
04:57:50.90 +41:07:05.1
03:47:46.30 +39:56:18.4
05:01:58.51 +41:53:11.0
05:00:38.49 +42:11:35.2
04:58:32.79 +41:38:59.4
04:17:22.94 +36:19:02.5
04:35:52.54 +38:38:30.5
04:54:57.28 +40:35:27.8
04:59:32.68 +41:42:08.7
04:56:36.30 +40:50:53.7
04:57:05.16 +40:26:37.1
05:00:43.34 +41:54:22.8
05:01:27.07 +42:04:34.8
04:53:59.81 +40:26:54.0
04:08:51.36 +34:22:14.8
04:57:17.41 +41:14:55.8
04:05:22.71 +33:16:17.2
03:51:54.75 +41:20:59.5
05:01:32.97 +42:00:47.2
04:08:46.93 +34:32:47.8
04:52:23.66 +39:58:22.9
04:54:20.61 +40:25:29.2
05:00:33.80 +42:05:03.7
04:58:38.55 +41:47:29.8
05:00:27.75 +41:46:29.5
04:57:15.99 +41:20:49.5
04:54:35.57 +40:27:52.2
04:21:51.52 +33:53:49.8
04:55:10.24 +41:08:38.4
05:00:57.87 +41:38:25.1
04:58:01.47 +40:43:28.5
04:57:36.87 +42:23:16.7
04:57:04.27 +41:58:49.5
04:12:30.16 +34:12:09.6
04:57:24.43 +41:18:28.6
05:01:21.71 +41:26:28.6
04:23:10.25 +34:32:53.9
04:57:54.10 +41:07:37.0
05:01:46.93 +41:38:09.5
04:06:28.59 +33:03:39.8
04:58:32.67 +41:20:39.4
04:59:20.73 +42:14:03.0
05:01:18.58 +41:11:29.6
05:01:30.42 +41:43:11.5
04:54:31.05 +40:48:57.5
04:44:37.96 +36:19:20.5
04:55:14.50 +40:22:32.9
04:58:12.89 +41:11:28.1
05:01:00.05 +41:08:16.0
04:56:10.90 +40:09:16.2
04:56:35.01 +41:29:30.3
04:58:16.58 +41:09:54.5
04:56:55.24 +41:16:29.2
04:52:35.42 +40:09:50.6
05:00:26.58 +41:55:28.2
05:00:24.45 +42:03:37.6
04:18:31.62 +32:56:11.9
04:04:59.54 +33:28:20.4
05:00:44.55 +41:18:33.5
04:20:16.08 +33:34:29.0
05:00:04.13 +40:55:58.1
04:57:29.45 +41:08:59.7
04:59:21.33 +41:25:17.6
04:58:07.50 +41:17:15.6
05:01:30.01 +41:39:29.2
04:56:15.73 +40:27:41.1
04:18:23.09 +33:07:48.1
04:56:43.63 +41:20:50.2
04:54:51.37 +40:41:54.7
04:59:55.93 +41:06:08.7
04:59:27.41 +42:00:20.7
05:01:52.17 +42:12:30.6
04:17:37.89 +33:42:21.2
04:58:55.90 +42:01:51.1
04:58:14.04 +41:20:56.9
04:57:02.40 +41:06:06.8
04:57:02.56 +40:36:38.0
04:56:06.03 +40:41:36.7
04:55:03.05 +40:40:19.5
04:58:06.04 +41:18:52.3
04:58:58.26 +41:32:00.9
04:56:46.56 +41:00:13.4
04:56:50.77 +40:43:40.9
04:58:47.68 +41:24:10.8
04:39:27.68 +40:01:25.1
05:00:34.76 +40:59:23.3
05:01:49.62 +41:41:01.7
04:09:54.24 +34:17:01.2
04:54:40.40 +40:30:57.8
04:56:43.57 +41:04:49.3
05:01:28.85 +41:51:01.1
04:58:30.12 +41:31:49.7
04:56:23.92 +41:08:21.6
04:55:17.17 +40:33:49.6
04:54:52.37 +40:30:58.9
05:01:37.66 +42:05:05.4
05:01:47.51 +41:46:31.9
04:18:24.02 +33:22:35.1
04:52:37.96 +40:11:17.8
04:56:06.36 +41:17:31.2
04:57:00.10 +41:12:54.8
04:15:22.69 +32:59:33.5
05:01:52.16 +41:48:37.7
###################################################################################
05:01:33.32 +42:10:38.4 -- not an asteroid (will add it to exclusion list)
04:53:06.39 +40:35:50.9 -- not an asteroid (will add it to exclusion list)
04:56:20.68 +41:43:23.9 -- not an asteroid (will add it to exclusion list)
05:00:58.13 +41:53:30.8 -- not an asteroid (will add it to exclusion list)
04:55:09.88 +40:33:03.2 -- not an asteroid (will add it to exclusion list)
03:48:10.95 +41:57:18.6 -- not an asteroid (will add it to exclusion list)
05:01:36.22 +42:07:32.6 -- not an asteroid (will add it to exclusion list)
03:51:04.96 +42:11:55.7 -- not an asteroid (will add it to exclusion list)
03:53:49.46 +42:15:40.9 -- not an asteroid (will add it to exclusion list)
03:49:35.78 +40:31:27.6 -- not an asteroid (will add it to exclusion list)
03:48:13.22 +40:09:25.5 -- not an asteroid (will add it to exclusion list)
03:50:49.99 +41:45:03.2 -- not an asteroid (will add it to exclusion list)
03:51:12.19 +42:07:35.2 -- not an asteroid (will add it to exclusion list)
03:47:57.54 +41:46:17.6 -- not an asteroid (will add it to exclusion list)
04:58:17.08 +41:15:54.7 -- not an asteroid (will add it to exclusion list)
03:51:22.81 +41:49:40.8 -- not an asteroid (will add it to exclusion list)
03:48:48.30 +42:19:43.5 -- not an asteroid (will add it to exclusion list)
03:51:34.91 +40:20:52.4 -- not an asteroid (will add it to exclusion list)
03:52:12.95 +41:28:22.4 -- not an asteroid (will add it to exclusion list)
03:51:22.42 +39:38:05.9 -- not an asteroid (will add it to exclusion list)
03:45:53.65 +40:56:32.0 -- not an asteroid (will add it to exclusion list)
03:51:06.48 +42:26:37.5 -- not an asteroid (will add it to exclusion list)
03:50:58.79 +41:54:33.5 -- not an asteroid (will add it to exclusion list)
03:48:43.39 +40:25:57.3 -- not an asteroid (will add it to exclusion list)
03:51:42.29 +39:24:03.1 -- not an asteroid (will add it to exclusion list)
03:54:01.48 +42:24:58.9 -- not an asteroid (will add it to exclusion list)
03:52:26.94 +40:24:09.8 -- not an asteroid (will add it to exclusion list)
03:52:40.18 +40:13:30.4 -- not an asteroid (will add it to exclusion list)
03:45:46.80 +39:11:32.7 -- not an asteroid (will add it to exclusion list)
03:56:39.13 +42:06:02.7 -- not an asteroid (will add it to exclusion list)
03:44:51.49 +39:44:55.4 -- not an asteroid (will add it to exclusion list)
03:51:50.58 +42:07:48.8 -- not an asteroid (will add it to exclusion list)
03:49:51.43 +42:06:23.2 -- not an asteroid (will add it to exclusion list)
03:51:12.59 +40:50:11.7 -- not an asteroid (will add it to exclusion list)
03:46:13.97 +41:22:08.9 -- not an asteroid (will add it to exclusion list)
03:47:51.06 +42:20:17.3 -- not an asteroid (will add it to exclusion list)
03:50:22.85 +42:03:43.6 -- not an asteroid (will add it to exclusion list)
04:57:28.14 +41:10:34.0 -- not an asteroid (will add it to exclusion list)
03:52:17.78 +42:29:02.4 -- not an asteroid (will add it to exclusion list)
03:54:16.87 +41:53:57.0 -- not an asteroid (will add it to exclusion list)
03:47:57.35 +39:51:30.5 -- not an asteroid (will add it to exclusion list)
03:46:41.78 +41:58:24.7 -- not an asteroid (will add it to exclusion list)
03:48:56.91 +39:55:42.5 -- not an asteroid (will add it to exclusion list)
03:47:53.99 +39:16:53.9 -- not an asteroid (will add it to exclusion list)
03:51:37.56 +42:09:52.3 -- not an asteroid (will add it to exclusion list)
03:50:38.36 +41:57:28.3 -- not an asteroid (will add it to exclusion list)
03:43:49.29 +40:49:44.0 -- not an asteroid (will add it to exclusion list)
03:44:50.45 +40:44:48.7 -- not an asteroid (will add it to exclusion list)
03:46:57.53 +39:45:21.5 -- not an asteroid (will add it to exclusion list)
03:47:50.31 +41:09:40.5 -- not an asteroid (will add it to exclusion list)
03:50:27.52 +40:43:19.5 -- not an asteroid (will add it to exclusion list)
03:52:07.88 +40:43:49.4 -- not an asteroid (will add it to exclusion list)
04:57:10.42 +41:22:55.7 -- not an asteroid (will add it to exclusion list)
03:48:01.97 +41:43:53.4 -- not an asteroid (will add it to exclusion list)
04:39:17.27 +39:49:43.5 -- not an asteroid (will add it to exclusion list)
04:56:10.04 +33:01:16.7 -- not an asteroid (will add it to exclusion list)
03:50:28.95 +40:07:07.8 -- not an asteroid (will add it to exclusion list)
03:52:35.26 +41:46:36.2 -- not an asteroid (will add it to exclusion list)
03:52:40.27 +41:04:35.5 -- not an asteroid (will add it to exclusion list)
04:58:55.95 +42:08:02.7 -- not an asteroid (will add it to exclusion list)
03:44:54.77 +39:59:05.8 -- not an asteroid (will add it to exclusion list)
03:44:08.15 +40:15:34.0 -- not an asteroid (will add it to exclusion list)
03:52:11.71 +40:33:50.8 -- not an asteroid (will add it to exclusion list)
04:40:22.43 +40:04:07.5 -- not an asteroid (will add it to exclusion list)
05:01:54.98 +41:54:01.4 -- not an asteroid (will add it to exclusion list)
04:20:31.63 +33:37:33.2 -- not an asteroid (will add it to exclusion list)
04:56:15.33 +41:07:15.6 -- not an asteroid (will add it to exclusion list)
03:51:00.85 +41:53:33.2 -- not an asteroid (will add it to exclusion list)
03:52:50.85 +40:12:22.9 -- not an asteroid (will add it to exclusion list)
03:50:35.94 +42:10:30.5 -- not an asteroid (will add it to exclusion list)
04:57:20.50 +41:14:23.1 -- not an asteroid (will add it to exclusion list)
04:56:46.73 +41:21:39.2 -- not an asteroid (will add it to exclusion list)
04:37:13.14 +39:57:31.9 -- not an asteroid (will add it to exclusion list)
03:51:01.28 +40:06:04.2 -- not an asteroid (will add it to exclusion list)
03:42:06.96 +40:56:32.0 -- not an asteroid (will add it to exclusion list)
04:56:12.68 +40:32:52.5 -- not an asteroid (will add it to exclusion list)
03:46:29.67 +40:03:09.3 -- not an asteroid (will add it to exclusion list)
03:46:46.02 +41:33:42.1 -- not an asteroid (will add it to exclusion list)
05:01:35.12 +41:56:43.7 -- not an asteroid (will add it to exclusion list)
04:57:32.33 +41:29:46.8 -- not an asteroid (will add it to exclusion list)
03:47:20.47 +41:39:38.4 -- not an asteroid (will add it to exclusion list)
03:52:32.23 +40:59:48.4 -- not an asteroid (will add it to exclusion list)
04:58:08.84 +42:03:26.8 -- not an asteroid (will add it to exclusion list)
04:55:29.69 +41:00:53.8 -- not an asteroid (will add it to exclusion list)
03:48:46.02 +38:45:24.8 -- not an asteroid (will add it to exclusion list)
04:56:53.62 +41:18:55.2 -- not an asteroid (will add it to exclusion list)
04:59:20.66 +41:30:27.2 -- not an asteroid (will add it to exclusion list)
05:00:58.25 +41:39:16.5 -- not an asteroid (will add it to exclusion list)
04:59:28.78 +41:32:05.0 -- not an asteroid (will add it to exclusion list)
04:57:58.54 +41:14:17.0 -- not an asteroid (will add it to exclusion list)
03:51:03.50 +41:57:59.7 -- not an asteroid (will add it to exclusion list)
04:53:31.48 +40:37:41.0 -- not an asteroid (will add it to exclusion list)
04:59:07.41 +41:59:26.9 -- not an asteroid (will add it to exclusion list)
04:08:25.99 +34:20:03.2 -- not an asteroid (will add it to exclusion list)
04:57:59.44 +42:02:10.4 -- not an asteroid (will add it to exclusion list)
04:55:17.06 +40:24:11.3 -- not an asteroid (will add it to exclusion list)
03:50:09.86 +40:22:49.0 -- not an asteroid (will add it to exclusion list)
04:57:23.85 +40:41:33.9 -- not an asteroid (will add it to exclusion list)
03:52:17.29 +40:29:03.9 -- not an asteroid (will add it to exclusion list)
05:01:11.57 +41:47:07.6 -- not an asteroid (will add it to exclusion list)
04:57:50.90 +41:07:05.1 -- not an asteroid (will add it to exclusion list)
03:47:46.30 +39:56:18.4 -- not an asteroid (will add it to exclusion list)
05:01:58.51 +41:53:11.0 -- not an asteroid (will add it to exclusion list)
05:00:38.49 +42:11:35.2 -- not an asteroid (will add it to exclusion list)
04:58:32.79 +41:38:59.4 -- not an asteroid (will add it to exclusion list)
04:17:22.94 +36:19:02.5 -- not an asteroid (will add it to exclusion list)
04:35:52.54 +38:38:30.5 -- not an asteroid (will add it to exclusion list)
04:54:57.28 +40:35:27.8 -- not an asteroid (will add it to exclusion list)
04:59:32.68 +41:42:08.7 -- not an asteroid (will add it to exclusion list)
04:56:36.30 +40:50:53.7 -- not an asteroid (will add it to exclusion list)
04:57:05.16 +40:26:37.1 -- not an asteroid (will add it to exclusion list)
05:00:43.34 +41:54:22.8 -- not an asteroid (will add it to exclusion list)
05:01:27.07 +42:04:34.8 -- not an asteroid (will add it to exclusion list)
04:53:59.81 +40:26:54.0 -- not an asteroid (will add it to exclusion list)
04:08:51.36 +34:22:14.8 -- not an asteroid (will add it to exclusion list)
04:57:17.41 +41:14:55.8 -- not an asteroid (will add it to exclusion list)
04:05:22.71 +33:16:17.2 -- not an asteroid (will add it to exclusion list)
03:51:54.75 +41:20:59.5 -- not an asteroid (will add it to exclusion list)
05:01:32.97 +42:00:47.2 -- not an asteroid (will add it to exclusion list)
04:08:46.93 +34:32:47.8 -- not an asteroid (will add it to exclusion list)
04:52:23.66 +39:58:22.9 -- not an asteroid (will add it to exclusion list)
04:54:20.61 +40:25:29.2 -- not an asteroid (will add it to exclusion list)
05:00:33.80 +42:05:03.7 -- not an asteroid (will add it to exclusion list)
04:58:38.55 +41:47:29.8 -- not an asteroid (will add it to exclusion list)
05:00:27.75 +41:46:29.5 -- not an asteroid (will add it to exclusion list)
04:57:15.99 +41:20:49.5 -- not an asteroid (will add it to exclusion list)
04:54:35.57 +40:27:52.2 -- not an asteroid (will add it to exclusion list)
04:21:51.52 +33:53:49.8 -- not an asteroid (will add it to exclusion list)
04:55:10.24 +41:08:38.4 -- not an asteroid (will add it to exclusion list)
05:00:57.87 +41:38:25.1 -- not an asteroid (will add it to exclusion list)
04:58:01.47 +40:43:28.5 -- not an asteroid (will add it to exclusion list)
04:57:36.87 +42:23:16.7 -- not an asteroid (will add it to exclusion list)
04:57:04.27 +41:58:49.5 -- not an asteroid (will add it to exclusion list)
04:12:30.16 +34:12:09.6 -- not an asteroid (will add it to exclusion list)
04:57:24.43 +41:18:28.6 -- not an asteroid (will add it to exclusion list)
05:01:21.71 +41:26:28.6 -- not an asteroid (will add it to exclusion list)
04:23:10.25 +34:32:53.9 -- not an asteroid (will add it to exclusion list)
04:57:54.10 +41:07:37.0 -- not an asteroid (will add it to exclusion list)
05:01:46.93 +41:38:09.5 -- not an asteroid (will add it to exclusion list)
04:06:28.59 +33:03:39.8 -- not an asteroid (will add it to exclusion list)
04:58:32.67 +41:20:39.4 -- not an asteroid (will add it to exclusion list)
04:59:20.73 +42:14:03.0 -- not an asteroid (will add it to exclusion list)
05:01:18.58 +41:11:29.6 -- not an asteroid (will add it to exclusion list)
05:01:30.42 +41:43:11.5 -- not an asteroid (will add it to exclusion list)
04:54:31.05 +40:48:57.5 -- not an asteroid (will add it to exclusion list)
04:44:37.96 +36:19:20.5 -- not an asteroid (will add it to exclusion list)
04:55:14.50 +40:22:32.9 -- not an asteroid (will add it to exclusion list)
04:58:12.89 +41:11:28.1 -- not an asteroid (will add it to exclusion list)
05:01:00.05 +41:08:16.0 -- not an asteroid (will add it to exclusion list)
04:56:10.90 +40:09:16.2 -- not an asteroid (will add it to exclusion list)
04:56:35.01 +41:29:30.3 -- not an asteroid (will add it to exclusion list)
04:58:16.58 +41:09:54.5 -- not an asteroid (will add it to exclusion list)
04:56:55.24 +41:16:29.2 -- not an asteroid (will add it to exclusion list)
04:52:35.42 +40:09:50.6 -- not an asteroid (will add it to exclusion list)
05:00:26.58 +41:55:28.2 -- not an asteroid (will add it to exclusion list)
05:00:24.45 +42:03:37.6 -- not an asteroid (will add it to exclusion list)
04:18:31.62 +32:56:11.9 -- not an asteroid (will add it to exclusion list)
04:04:59.54 +33:28:20.4 -- not an asteroid (will add it to exclusion list)
05:00:44.55 +41:18:33.5 -- not an asteroid (will add it to exclusion list)
04:20:16.08 +33:34:29.0 -- not an asteroid (will add it to exclusion list)
05:00:04.13 +40:55:58.1 -- not an asteroid (will add it to exclusion list)
04:57:29.45 +41:08:59.7 -- not an asteroid (will add it to exclusion list)
04:59:21.33 +41:25:17.6 -- not an asteroid (will add it to exclusion list)
04:58:07.50 +41:17:15.6 -- not an asteroid (will add it to exclusion list)
05:01:30.01 +41:39:29.2 -- not an asteroid (will add it to exclusion list)
04:56:15.73 +40:27:41.1 -- not an asteroid (will add it to exclusion list)
04:18:23.09 +33:07:48.1 -- not an asteroid (will add it to exclusion list)
04:56:43.63 +41:20:50.2 -- not an asteroid (will add it to exclusion list)
04:54:51.37 +40:41:54.7 -- not an asteroid (will add it to exclusion list)
04:59:55.93 +41:06:08.7 -- not an asteroid (will add it to exclusion list)
04:59:27.41 +42:00:20.7 -- not an asteroid (will add it to exclusion list)
05:01:52.17 +42:12:30.6 -- not an asteroid (will add it to exclusion list)
04:17:37.89 +33:42:21.2 -- not an asteroid (will add it to exclusion list)
04:58:55.90 +42:01:51.1 -- not an asteroid (will add it to exclusion list)
04:58:14.04 +41:20:56.9 -- not an asteroid (will add it to exclusion list)
04:57:02.40 +41:06:06.8 -- not an asteroid (will add it to exclusion list)
04:57:02.56 +40:36:38.0 -- not an asteroid (will add it to exclusion list)
04:56:06.03 +40:41:36.7 -- not an asteroid (will add it to exclusion list)
04:55:03.05 +40:40:19.5 -- not an asteroid (will add it to exclusion list)
04:58:06.04 +41:18:52.3 -- not an asteroid (will add it to exclusion list)
04:58:58.26 +41:32:00.9 -- not an asteroid (will add it to exclusion list)
04:56:46.56 +41:00:13.4 -- not an asteroid (will add it to exclusion list)
04:56:50.77 +40:43:40.9 -- not an asteroid (will add it to exclusion list)
04:58:47.68 +41:24:10.8 -- not an asteroid (will add it to exclusion list)
04:39:27.68 +40:01:25.1 -- not an asteroid (will add it to exclusion list)
05:00:34.76 +40:59:23.3 -- not an asteroid (will add it to exclusion list)
05:01:49.62 +41:41:01.7 -- not an asteroid (will add it to exclusion list)
04:09:54.24 +34:17:01.2 -- not an asteroid (will add it to exclusion list)
04:54:40.40 +40:30:57.8 -- not an asteroid (will add it to exclusion list)
04:56:43.57 +41:04:49.3 -- not an asteroid (will add it to exclusion list)
05:01:28.85 +41:51:01.1 -- not an asteroid (will add it to exclusion list)
04:58:30.12 +41:31:49.7 -- not an asteroid (will add it to exclusion list)
04:56:23.92 +41:08:21.6 -- not an asteroid (will add it to exclusion list)
04:55:17.17 +40:33:49.6 -- not an asteroid (will add it to exclusion list)
04:54:52.37 +40:30:58.9 -- not an asteroid (will add it to exclusion list)
05:01:37.66 +42:05:05.4 -- not an asteroid (will add it to exclusion list)
05:01:47.51 +41:46:31.9 -- not an asteroid (will add it to exclusion list)
04:18:24.02 +33:22:35.1 -- not an asteroid (will add it to exclusion list)
04:52:37.96 +40:11:17.8 -- not an asteroid (will add it to exclusion list)
04:56:06.36 +41:17:31.2 -- not an asteroid (will add it to exclusion list)
04:57:00.10 +41:12:54.8 -- not an asteroid (will add it to exclusion list)
04:15:22.69 +32:59:33.5 -- not an asteroid (will add it to exclusion list)
05:01:52.16 +41:48:37.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:42:06.96 +40:56:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:49.29 +40:49:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:08.15 +40:15:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:50.45 +40:44:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:51.49 +39:44:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:54.77 +39:59:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:46.80 +39:11:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:53.65 +40:56:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:13.97 +41:22:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:29.67 +40:03:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:41.78 +41:58:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:46.02 +41:33:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:57.53 +39:45:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:20.47 +41:39:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:46.30 +39:56:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:50.31 +41:09:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:51.06 +42:20:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:53.99 +39:16:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:57.35 +39:51:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:57.54 +41:46:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:01.97 +41:43:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:10.95 +41:57:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:13.22 +40:09:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:43.39 +40:25:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:46.02 +38:45:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:48.30 +42:19:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:56.91 +39:55:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:35.78 +40:31:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:51.43 +42:06:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:09.86 +40:22:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:22.85 +42:03:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:27.52 +40:43:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:28.95 +40:07:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:35.94 +42:10:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:38.36 +41:57:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:49.99 +41:45:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:58.79 +41:54:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:00.85 +41:53:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:01.28 +40:06:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:03.50 +41:57:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:04.96 +42:11:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:06.48 +42:26:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:12.19 +42:07:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:12.59 +40:50:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:22.42 +39:38:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:22.81 +41:49:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:34.91 +40:20:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:37.56 +42:09:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:42.29 +39:24:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:50.58 +42:07:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:54.75 +41:20:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:07.88 +40:43:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:11.71 +40:33:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:12.95 +41:28:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:17.29 +40:29:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:17.78 +42:29:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:26.94 +40:24:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:32.23 +40:59:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:35.26 +41:46:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:40.18 +40:13:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:40.27 +41:04:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:50.85 +40:12:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:49.46 +42:15:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:01.48 +42:24:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:16.87 +41:53:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:39.13 +42:06:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:04:59.54 +33:28:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:22.71 +33:16:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:28.59 +33:03:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:08:25.99 +34:20:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:08:46.93 +34:32:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:08:51.36 +34:22:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:09:54.24 +34:17:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:30.16 +34:12:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:22.69 +32:59:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:17:22.94 +36:19:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:17:37.89 +33:42:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:23.09 +33:07:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:24.02 +33:22:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:31.62 +32:56:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:16.08 +33:34:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:31.63 +33:37:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:21:51.52 +33:53:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:10.25 +34:32:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:52.54 +38:38:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:13.14 +39:57:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:17.27 +39:49:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:27.68 +40:01:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:22.43 +40:04:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:44:37.96 +36:19:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:23.66 +39:58:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:35.42 +40:09:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:37.96 +40:11:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:06.39 +40:35:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:31.48 +40:37:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:59.81 +40:26:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:20.61 +40:25:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:31.05 +40:48:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:35.57 +40:27:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:40.40 +40:30:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:51.37 +40:41:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:52.37 +40:30:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:57.28 +40:35:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:03.05 +40:40:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:09.88 +40:33:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:10.24 +41:08:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:14.50 +40:22:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:17.06 +40:24:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:17.17 +40:33:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:29.69 +41:00:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:06.03 +40:41:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:06.36 +41:17:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:10.04 +33:01:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:10.90 +40:09:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:12.68 +40:32:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:15.33 +41:07:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:15.73 +40:27:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:20.68 +41:43:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:23.92 +41:08:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:35.01 +41:29:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:36.30 +40:50:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:43.57 +41:04:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:43.63 +41:20:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:46.56 +41:00:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:46.73 +41:21:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:50.77 +40:43:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:53.62 +41:18:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:55.24 +41:16:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:00.10 +41:12:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:02.40 +41:06:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:02.56 +40:36:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:04.27 +41:58:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:05.16 +40:26:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:10.42 +41:22:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:15.99 +41:20:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:17.41 +41:14:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:20.50 +41:14:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:23.85 +40:41:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:24.43 +41:18:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:28.14 +41:10:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:29.45 +41:08:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:32.33 +41:29:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:36.87 +42:23:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:50.90 +41:07:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:54.10 +41:07:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:58.54 +41:14:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:59.44 +42:02:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:01.47 +40:43:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:06.04 +41:18:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:07.50 +41:17:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:08.84 +42:03:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:12.89 +41:11:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:14.04 +41:20:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:16.58 +41:09:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:17.08 +41:15:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:30.12 +41:31:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:32.67 +41:20:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:32.79 +41:38:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:38.55 +41:47:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:47.68 +41:24:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:55.90 +42:01:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:55.95 +42:08:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:58.26 +41:32:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:07.41 +41:59:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:20.66 +41:30:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:20.73 +42:14:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:21.33 +41:25:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:27.41 +42:00:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:28.78 +41:32:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:32.68 +41:42:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:55.93 +41:06:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:04.13 +40:55:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:24.45 +42:03:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:26.58 +41:55:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:27.75 +41:46:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:33.80 +42:05:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:34.76 +40:59:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:38.49 +42:11:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:43.34 +41:54:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:44.55 +41:18:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:57.87 +41:38:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:58.13 +41:53:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:58.25 +41:39:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:00.05 +41:08:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:11.57 +41:47:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:18.58 +41:11:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:21.71 +41:26:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:27.07 +42:04:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:28.85 +41:51:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:30.01 +41:39:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:30.42 +41:43:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:32.97 +42:00:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:33.32 +42:10:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:35.12 +41:56:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:36.22 +42:07:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:37.66 +42:05:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:46.93 +41:38:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:47.51 +41:46:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:49.62 +41:41:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:52.16 +41:48:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:52.17 +42:12:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:54.98 +41:54:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:58.51 +41:53:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
03:42:06.96 +40:56:32.0 -- not a known variable star
03:43:49.29 +40:49:44.0 -- not a known variable star
03:44:08.15 +40:15:34.0 -- not a known variable star
03:44:50.45 +40:44:48.7 -- not a known variable star
03:44:51.49 +39:44:55.4 -- not a known variable star
03:44:54.77 +39:59:05.8 -- not a known variable star
03:45:46.80 +39:11:32.7 -- not a known variable star
03:45:53.65 +40:56:32.0 -- not a known variable star
03:46:13.97 +41:22:08.9 -- not a known variable star
03:46:29.67 +40:03:09.3 -- not a known variable star
03:46:41.78 +41:58:24.7 -- not a known variable star
03:46:46.02 +41:33:42.1 -- not a known variable star
03:46:57.53 +39:45:21.5 -- not a known variable star
03:47:20.47 +41:39:38.4 -- not a known variable star
03:47:46.30 +39:56:18.4 -- not a known variable star
03:47:50.31 +41:09:40.5 -- not a known variable star
03:47:51.06 +42:20:17.3 -- not a known variable star
03:47:53.99 +39:16:53.9 -- not a known variable star
03:47:57.35 +39:51:30.5 -- not a known variable star
03:47:57.54 +41:46:17.6 -- a known variable star
03:48:01.97 +41:43:53.4 -- not a known variable star
03:48:10.95 +41:57:18.6 -- not a known variable star
03:48:13.22 +40:09:25.5 -- not a known variable star
03:48:43.39 +40:25:57.3 -- not a known variable star
03:48:46.02 +38:45:24.8 -- a known variable star
03:48:48.30 +42:19:43.5 -- not a known variable star
03:48:56.91 +39:55:42.5 -- not a known variable star
03:49:35.78 +40:31:27.6 -- not a known variable star
03:49:51.43 +42:06:23.2 -- not a known variable star
03:50:09.86 +40:22:49.0 -- a known variable star
03:50:22.85 +42:03:43.6 -- not a known variable star
03:50:27.52 +40:43:19.5 -- not a known variable star
03:50:28.95 +40:07:07.8 -- not a known variable star
03:50:35.94 +42:10:30.5 -- not a known variable star
03:50:38.36 +41:57:28.3 -- not a known variable star
03:50:49.99 +41:45:03.2 -- not a known variable star
03:50:58.79 +41:54:33.5 -- not a known variable star
03:51:00.85 +41:53:33.2 -- not a known variable star
03:51:01.28 +40:06:04.2 -- not a known variable star
03:51:03.50 +41:57:59.7 -- not a known variable star
03:51:04.96 +42:11:55.7 -- not a known variable star
03:51:06.48 +42:26:37.5 -- a known variable star
03:51:12.19 +42:07:35.2 -- not a known variable star
03:51:12.59 +40:50:11.7 -- not a known variable star
03:51:22.42 +39:38:05.9 -- not a known variable star
03:51:22.81 +41:49:40.8 -- not a known variable star
03:51:34.91 +40:20:52.4 -- not a known variable star
03:51:37.56 +42:09:52.3 -- not a known variable star
03:51:42.29 +39:24:03.1 -- not a known variable star
03:51:50.58 +42:07:48.8 -- a known variable star
03:51:54.75 +41:20:59.5 -- not a known variable star
03:52:07.88 +40:43:49.4 -- not a known variable star
03:52:11.71 +40:33:50.8 -- not a known variable star
03:52:12.95 +41:28:22.4 -- not a known variable star
03:52:17.29 +40:29:03.9 -- not a known variable star
03:52:17.78 +42:29:02.4 -- not a known variable star
03:52:26.94 +40:24:09.8 -- not a known variable star
03:52:32.23 +40:59:48.4 -- not a known variable star
03:52:35.26 +41:46:36.2 -- not a known variable star
03:52:40.18 +40:13:30.4 -- not a known variable star
03:52:40.27 +41:04:35.5 -- not a known variable star
03:52:50.85 +40:12:22.9 -- not a known variable star
03:53:49.46 +42:15:40.9 -- not a known variable star
03:54:01.48 +42:24:58.9 -- not a known variable star
03:54:16.87 +41:53:57.0 -- not a known variable star
03:56:39.13 +42:06:02.7 -- not a known variable star
04:04:59.54 +33:28:20.4 -- not a known variable star
04:05:22.71 +33:16:17.2 -- not a known variable star
04:06:28.59 +33:03:39.8 -- not a known variable star
04:08:25.99 +34:20:03.2 -- not a known variable star
04:08:46.93 +34:32:47.8 -- not a known variable star
04:08:51.36 +34:22:14.8 -- not a known variable star
04:09:54.24 +34:17:01.2 -- not a known variable star
04:12:30.16 +34:12:09.6 -- not a known variable star
04:15:22.69 +32:59:33.5 -- not a known variable star
04:17:22.94 +36:19:02.5 -- not a known variable star
04:17:37.89 +33:42:21.2 -- not a known variable star
04:18:23.09 +33:07:48.1 -- not a known variable star
04:18:24.02 +33:22:35.1 -- a known variable star
04:18:31.62 +32:56:11.9 -- a known variable star
04:20:16.08 +33:34:29.0 -- not a known variable star
04:20:31.63 +33:37:33.2 -- a known variable star
04:21:51.52 +33:53:49.8 -- not a known variable star
04:23:10.25 +34:32:53.9 -- not a known variable star
04:35:52.54 +38:38:30.5 -- not a known variable star
04:37:13.14 +39:57:31.9 -- not a known variable star
04:39:17.27 +39:49:43.5 -- not a known variable star
04:39:27.68 +40:01:25.1 -- a known variable star
04:40:22.43 +40:04:07.5 -- not a known variable star
04:44:37.96 +36:19:20.5 -- not a known variable star
04:52:23.66 +39:58:22.9 -- a known variable star
04:52:35.42 +40:09:50.6 -- not a known variable star
04:52:37.96 +40:11:17.8 -- a known variable star
04:53:06.39 +40:35:50.9 -- not a known variable star
04:53:31.48 +40:37:41.0 -- not a known variable star
04:53:59.81 +40:26:54.0 -- a known variable star
04:54:20.61 +40:25:29.2 -- a known variable star
04:54:31.05 +40:48:57.5 -- not a known variable star
04:54:35.57 +40:27:52.2 -- not a known variable star
04:54:40.40 +40:30:57.8 -- not a known variable star
04:54:51.37 +40:41:54.7 -- not a known variable star
04:54:52.37 +40:30:58.9 -- not a known variable star
04:54:57.28 +40:35:27.8 -- not a known variable star
04:55:03.05 +40:40:19.5 -- not a known variable star
04:55:09.88 +40:33:03.2 -- a known variable star
04:55:10.24 +41:08:38.4 -- not a known variable star
04:55:14.50 +40:22:32.9 -- not a known variable star
04:55:17.06 +40:24:11.3 -- a known variable star
04:55:17.17 +40:33:49.6 -- not a known variable star
04:55:29.69 +41:00:53.8 -- not a known variable star
04:56:06.03 +40:41:36.7 -- not a known variable star
04:56:06.36 +41:17:31.2 -- not a known variable star
04:56:10.04 +33:01:16.7 -- not a known variable star
04:56:10.90 +40:09:16.2 -- a known variable star
04:56:12.68 +40:32:52.5 -- not a known variable star
04:56:15.33 +41:07:15.6 -- not a known variable star
04:56:15.73 +40:27:41.1 -- a known variable star
04:56:20.68 +41:43:23.9 -- not a known variable star
04:56:23.92 +41:08:21.6 -- not a known variable star
04:56:35.01 +41:29:30.3 -- not a known variable star
04:56:36.30 +40:50:53.7 -- not a known variable star
04:56:43.57 +41:04:49.3 -- not a known variable star
04:56:43.63 +41:20:50.2 -- not a known variable star
04:56:46.56 +41:00:13.4 -- a known variable star
04:56:46.73 +41:21:39.2 -- not a known variable star
04:56:50.77 +40:43:40.9 -- a known variable star
04:56:53.62 +41:18:55.2 -- not a known variable star
04:56:55.24 +41:16:29.2 -- not a known variable star
04:57:00.10 +41:12:54.8 -- not a known variable star
04:57:02.40 +41:06:06.8 -- not a known variable star
04:57:02.56 +40:36:38.0 -- not a known variable star
04:57:04.27 +41:58:49.5 -- not a known variable star
04:57:05.16 +40:26:37.1 -- not a known variable star
04:57:10.42 +41:22:55.7 -- not a known variable star
04:57:15.99 +41:20:49.5 -- not a known variable star
04:57:17.41 +41:14:55.8 -- not a known variable star
04:57:20.50 +41:14:23.1 -- not a known variable star
04:57:23.85 +40:41:33.9 -- not a known variable star
04:57:24.43 +41:18:28.6 -- a known variable star
04:57:28.14 +41:10:34.0 -- a known variable star
04:57:29.45 +41:08:59.7 -- not a known variable star
04:57:32.33 +41:29:46.8 -- a known variable star
04:57:36.87 +42:23:16.7 -- a known variable star
04:57:50.90 +41:07:05.1 -- not a known variable star
04:57:54.10 +41:07:37.0 -- not a known variable star
04:57:58.54 +41:14:17.0 -- not a known variable star
04:57:59.44 +42:02:10.4 -- not a known variable star
04:58:01.47 +40:43:28.5 -- a known variable star
04:58:06.04 +41:18:52.3 -- not a known variable star
04:58:07.50 +41:17:15.6 -- not a known variable star
04:58:08.84 +42:03:26.8 -- not a known variable star
04:58:12.89 +41:11:28.1 -- not a known variable star
04:58:14.04 +41:20:56.9 -- not a known variable star
04:58:16.58 +41:09:54.5 -- not a known variable star
04:58:17.08 +41:15:54.7 -- not a known variable star
04:58:30.12 +41:31:49.7 -- not a known variable star
04:58:32.67 +41:20:39.4 -- not a known variable star
04:58:32.79 +41:38:59.4 -- a known variable star
04:58:38.55 +41:47:29.8 -- not a known variable star
04:58:47.68 +41:24:10.8 -- not a known variable star
04:58:55.90 +42:01:51.1 -- not a known variable star
04:58:55.95 +42:08:02.7 -- not a known variable star
04:58:58.26 +41:32:00.9 -- not a known variable star
04:59:07.41 +41:59:26.9 -- not a known variable star
04:59:20.66 +41:30:27.2 -- not a known variable star
04:59:20.73 +42:14:03.0 -- a known variable star
04:59:21.33 +41:25:17.6 -- not a known variable star
04:59:27.41 +42:00:20.7 -- not a known variable star
04:59:28.78 +41:32:05.0 -- not a known variable star
04:59:32.68 +41:42:08.7 -- not a known variable star
04:59:55.93 +41:06:08.7 -- a known variable star
05:00:04.13 +40:55:58.1 -- not a known variable star
05:00:24.45 +42:03:37.6 -- not a known variable star
05:00:26.58 +41:55:28.2 -- not a known variable star
05:00:27.75 +41:46:29.5 -- not a known variable star
05:00:33.80 +42:05:03.7 -- not a known variable star
05:00:34.76 +40:59:23.3 -- not a known variable star
05:00:38.49 +42:11:35.2 -- not a known variable star
05:00:43.34 +41:54:22.8 -- a known variable star
05:00:44.55 +41:18:33.5 -- not a known variable star
05:00:57.87 +41:38:25.1 -- a known variable star
05:00:58.13 +41:53:30.8 -- not a known variable star
05:00:58.25 +41:39:16.5 -- not a known variable star
05:01:00.05 +41:08:16.0 -- not a known variable star
05:01:11.57 +41:47:07.6 -- not a known variable star
05:01:18.58 +41:11:29.6 -- not a known variable star
05:01:21.71 +41:26:28.6 -- not a known variable star
05:01:27.07 +42:04:34.8 -- not a known variable star
05:01:28.85 +41:51:01.1 -- not a known variable star
05:01:30.01 +41:39:29.2 -- not a known variable star
05:01:30.42 +41:43:11.5 -- not a known variable star
05:01:32.97 +42:00:47.2 -- a known variable star
05:01:33.32 +42:10:38.4 -- not a known variable star
05:01:35.12 +41:56:43.7 -- not a known variable star
05:01:36.22 +42:07:32.6 -- not a known variable star
05:01:37.66 +42:05:05.4 -- not a known variable star
05:01:46.93 +41:38:09.5 -- not a known variable star
05:01:47.51 +41:46:31.9 -- not a known variable star
05:01:49.62 +41:41:01.7 -- a known variable star
05:01:52.16 +41:48:37.7 -- not a known variable star
05:01:52.17 +42:12:30.6 -- not a known variable star
05:01:54.98 +41:54:01.4 -- not a known variable star
05:01:58.51 +41:53:11.0 -- not a known variable star
Found 172 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
203 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 203 (excluding asteroids and hot pixels, 172 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461289.75101734 -observatory V36
11:32:15.29 +04:16:45.3 Mercury (-1.0mag)
13:33:24.26 -14:07:10.2 Venus (-4.7mag)
07:11:09.68 +23:02:47.2 Mars (1.2mag)
09:08:11.22 +17:01:11.2 Jupiter (-1.8mag)
00:51:58.30 +02:40:19.6 Saturn (0.5mag)
04:13:40.40 +21:01:57.1 Uranus (5.7mag)
00:13:50.71 -00:02:33.7 Neptune (7.7mag)
20:25:39.97 -23:39:22.5 Pluto (14.5mag)
06:42:44.26 +26:29:29.0 Moon (-9.7mag)
-rw-r--r-- 1 apache apache 362 Sep 6 01:04 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461289.75101734:
09:08:07.43 +17:01:31.2 Io (6.2mag)
09:08:21.84 +17:00:19.8 Europa (6.3mag)
09:08:28.14 +16:59:48.0 Ganymede (5.7mag)
09:07:44.76 +17:03:20.6 Callisto (6.9mag)
09:05:55.45 +17:17:14.9 Himalia (15.7mag)
09:08:09.27 +17:01:21.0 Thebe (16.6mag)
09:05:33.28 +17:11:17.1 Elara (17.7mag)
09:12:06.29 +16:29:04.8 Pasiphae (17.9mag)
09:09:20.82 +17:18:40.7 Carme (19.0mag)
00:51:59.54 +02:40:40.1 Titan (8.3mag)
00:51:54.78 +02:40:25.4 Rhea (9.6mag)
00:52:16.21 +02:42:55.0 Iapetus (11.0mag)
00:52:09.91 +02:39:40.3 Hyperion (14.3mag)
00:50:46.17 +02:30:09.7 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 6 01:04 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461289.75101734:
21:56:21.97 -00:04:29.1 JWST
14:50:35.23 +53:24:56.7 Chandra
05:12:32.92 +44:35:46.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 6 01:04 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461289.75101734 -observatory V36
03:39:47.33 +19:17:27.7 17.4mag P/1996 R2 (Lagerkvist)
18:02:33.31 -34:13:50.0 14.3mag P/2010 H2 (Vales)
07:18:40.52 -70:14:38.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:34.17 +33:40:23.8 17.7mag C/2017 K2 (PANSTARRS)
04:49:52.75 +45:19:13.5 15.7mag P/2021 N1 (ZTF)
04:49:52.75 +45:19:13.5 15.7mag P/2021 N1 (ZTF)
04:49:52.75 +45:19:13.5 15.7mag P/2021 N1 (ZTF)
04:49:52.75 +45:19:13.5 15.7mag P/2021 N1 (ZTF)
22:14:19.39 +28:47:47.8 17.4mag C/2022 E2 (ATLAS)
07:09:23.37 +25:59:54.6 16.9mag C/2022 N2 (PANSTARRS)
10:48:31.96 +27:15:50.4 17.1mag C/2022 QE78 (ATLAS)
09:48:00.23 +05:14:19.1 18.0mag C/2022 R6 (PANSTARRS)
15:29:49.82 -15:33:26.6 14.8mag C/2023 R1 (PANSTARRS)
08:37:28.17 +32:49:42.6 15.8mag C/2024 E1 (Wierzchos)
15:06:28.08 +15:20:06.7 17.9mag C/2024 G6 (ATLAS)
18:34:17.09 +43:12:48.1 13.7mag C/2024 J3 (ATLAS)
20:27:36.65 +49:21:18.0 17.4mag C/2024 R4 (PANSTARRS)
05:35:02.59 -13:00:46.2 15.1mag C/2024 T5 (ATLAS)
07:11:15.69 +18:45:06.6 17.8mag C/2025 J1 (Borisov)
11:16:18.15 +18:51:01.4 16.8mag C/2025 V2 (Rankin)
13:18:46.12 +00:12:01.4 16.8mag C/2025 Y1 (ATLAS)
16:38:42.42 +74:12:14.5 16.1mag C/2026 A2 (Bok)
03:06:17.40 +46:09:57.6 17.4mag C/2026 B2 (Sun-Gao)
12:12:18.28 +11:11:49.9 17.5mag A/2026 E1
22:25:08.42 -34:57:43.6 13.4mag 10P/Tempel
01:17:51.17 +36:48:46.0 18.0mag 11P/Tempel-Swift-LINEAR
11:47:28.32 -05:23:23.8 16.3mag 29P/Schwassmann-Wachmann
12:06:27.78 -04:45:48.0 17.6mag 63P/Wild
00:45:14.23 -07:00:09.6 15.4mag 65P/Gunn
06:37:17.88 +19:19:50.0 17.1mag 78P/Gehrels
03:17:11.84 +14:59:01.8 16.7mag 88P/Howell
05:34:45.65 +28:13:48.7 17.5mag 112P/Urata-Niijima
07:28:41.13 +25:04:50.2 17.9mag 114P/Wiseman-Skiff
10:25:33.24 +21:05:19.0 14.8mag 123P/West-Hartley
12:44:18.17 -20:58:23.0 17.4mag 124P/Mrkos
06:16:08.53 +20:40:15.3 15.9mag 128P/Shoemaker-Holt
02:36:04.77 -17:43:36.6 15.3mag 161P/Hartley-IRAS
09:39:39.82 +14:25:48.8 12.0mag 169P/NEAT
03:23:32.12 +08:33:31.7 14.5mag 220P/McNaught
04:45:14.28 +35:59:24.6 15.2mag 260P/McNaught
08:29:03.59 +35:48:37.2 17.3mag 295P/LINEAR
15:24:33.79 -00:07:53.2 17.9mag 391P/Kowalski
09:26:52.81 +16:54:14.0 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.1K Sep 6 01:04 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
-rw-r--r-- 1 apache apache 5.7K Sep 6 01:04 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
-rw-r--r-- 1 apache apache 190K Sep 6 01:04 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
22:48:01.050 +02:29:57.95 AT 2026ymz 2026-08-05.73 21.98
22:56:40.110 +02:46:51.37 AT 2026ymy 2026-08-04.80 21.96
01:44:34.660 +05:27:13.55 AT 2026ymx 2026-08-01.88 21.27
01:29:50.630 +00:07:42.35 AT 2026ymw 2026-07-21.86 22.34
01:20:55.160 +01:31:29.58 AT 2026ymv 2026-07-20.88 22.17
23:25:01.600 +02:19:39.37 AT 2026ymu 2026-07-20.78 22.49
22:52:58.240 +03:42:25.38 AT 2026ymt 2026-08-05.73 21.81
23:42:43.162 +19:31:30.19 AT 2026yms 2026-08-09.94 19.57
21:20:13.290 -37:42:51.98 AT 2026ymr 2026-08-09.45 19.171
17:37:51.010 -21:58:53.20 AT 2026ymq 2026-08-09.59 14.86
22:57:17.960 +47:07:41.80 AT 2026ymp 2026-08-09.33 14.3
21:11:14.725 +16:08:57.69 AT 2026ymo 2026-08-04.97 19.97
00:45:33.395 +25:23:53.86 AT 2026ymn 2026-08-10.09 19.737
16:42:12.700 +21:20:23.08 AT 2026ymm 2026-08-09.32 19.568
00:16:26.794 -31:27:04.55 AT 2026yml 2026-08-09.54 18.69
20:46:11.408 +21:33:49.40 SN 2026ymk 2026-08-10.01 19.906
16:27:21.310 +63:36:15.74 AT 2026ymj 2026-08-08.31 19.192
00:43:25.659 +22:56:56.07 SN 2026ymi 2026-08-10.10 19.196
00:25:21.922 +28:26:14.78 AT 2026ymh 2026-08-09.50 19.349
00:12:57.521 -28:42:47.48 AT 2026ymg 2026-08-09.53 18.729
-rw-r--r-- 1 apache apache 88K Sep 6 01:04 tns_transients_list.txt
