This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Lyn-06-Q1b1x1_233240_TTUQ1b1x1_826851_r1aPi9WG
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 06 08.1494 2461199.6494 12.51 08:16:27.40 +34:05:41.0
187.80286 31.51919 galactic Lyn Second-epoch detections are separated by 0.9" 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 | 08:16:27.40 +34:05:41.0 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.574+/-0.029 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:27.40 +34:05:41.0: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:27.40 +34:05:41.0: 13.40 +/- 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!
Don'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,2461199.6494,12.51,0.05,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
target 20260608.1494 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.36 08:17:27.79 +34:37:59.7
187.24199 31.84377 galactic Lyn 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 | 08:17:27.79 +34:37:59.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.470+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:27.79 +34:37:59.7: 13.46 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:27.79 +34:37:59.7: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 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,2461199.6494,12.36,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.36 08:18:33.85 +33:44:02.0
188.33401 31.86140 galactic Lyn 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 | target | 08:18:33.85 +33:44:02.0 (user input) | T | P | (position from user input) J-Ks=0.589+/-0.024 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:33.85 +33:44:02.0: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:33.85 +33:44:02.0: 13.42 +/- 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!
Don'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,2461199.6494,12.36,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.30 08:22:36.91 +33:02:32.4
189.35946 32.52491 galactic Cnc Second-epoch detections are separated by 0.7" 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 | target | 08:22:36.91 +33:02:32.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.377+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:36.91 +33:02:32.4: 13.28 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:36.91 +33:02:32.4: 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!
Don'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,2461199.6494,12.30,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.49 08:17:23.35 +35:10:26.2
186.61689 31.94828 galactic Lyn Second-epoch detections are separated by 1.6" 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 | 08:17:23.35 +35:10:26.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.440+/-0.031 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:23.35 +35:10:26.2: 13.48 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:23.35 +35:10:26.2: 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!
Don'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,2461199.6494,12.49,0.05,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
target 20260608.1494 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.71 08:19:32.52 +34:31:14.7
187.48344 32.23603 galactic Lyn 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 | 08:19:32.52 +34:31:14.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.383+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:32.52 +34:31:14.7: 13.77 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:32.52 +34:31:14.7: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461199.6494,12.71,0.05,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 20260608.1494 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.53 08:14:36.92 +34:20:36.7
187.41628 31.20641 galactic Lyn 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 | 08:14:36.92 +34:20:36.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.339+/-0.029 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:14:36.92 +34:20:36.7: 13.51 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:14:36.92 +34:20:36.7: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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,2461199.6494,12.53,0.05,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
target 20260608.1494 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.61 08:18:12.71 +34:08:55.0
187.83892 31.88513 galactic Lyn Second-epoch detections are separated by 1.3" 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 | 08:18:12.71 +34:08:55.0 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:12.71 +34:08:55.0: 13.79 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:12.71 +34:08:55.0: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 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,2461199.6494,12.61,0.05,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
target 20260608.1494 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.56 08:15:50.19 +35:03:52.1
186.66033 31.61447 galactic Lyn Second-epoch detections are separated by 2.0" 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 | 08:15:50.19 +35:03:52.1 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:15:50.19 +35:03:52.1: 13.53 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:15:50.19 +35:03:52.1: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 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,2461199.6494,12.56,0.05,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
target 20260608.1494 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.50 08:19:22.24 +33:50:04.1
188.26391 32.04758 galactic Lyn Second-epoch detections are separated by 1.0" 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 | ATO J124.8469+33.8339 | 08:19:22.24 +33:50:04.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.419+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:22.24 +33:50:04.1: 13.53 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:22.24 +33:50:04.1: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 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 J124.8469+33.8339,2461199.6494,12.50,0.05,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
ATO J124.8469+33.8339 20260608.1494 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 06 08.1494 2461199.6494 12.70 08:11:25.07 +33:41:01.7
187.97866 30.40581 galactic Lyn Second-epoch detections are separated by 0.6" 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 | 08:11:25.07 +33:41:01.7 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.033 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:11:25.07 +33:41:01.7: 13.81 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:11:25.07 +33:41:01.7: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461199.6494,12.70,0.05,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 20260608.1494 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.62 08:21:22.94 +33:26:34.3
188.82744 32.36587 galactic Lyn Second-epoch detections are separated by 0.8" 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 | 08:21:22.94 +33:26:34.3 (user input) | T | P | (position from user input) J-Ks=0.627+/-0.024 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:22.94 +33:26:34.3: 13.82 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:22.94 +33:26:34.3: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461199.6494,12.62,0.05,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
target 20260608.1494 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.40 08:16:44.61 +35:52:49.6
185.77034 31.97182 galactic Lyn Second-epoch detections are separated by 2.4" and 8.0 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 | 08:16:44.61 +35:52:49.6 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.608+/-0.030 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:44.61 +35:52:49.6: 13.43 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:44.61 +35:52:49.6: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 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,2461199.6494,12.40,0.05,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
target 20260608.1494 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.27 08:18:32.50 +35:55:57.6
185.80026 32.33879 galactic Lyn Second-epoch detections are separated by 1.7" and 7.8 pix
The object was found in VSX 0" Gaia DR3 904493896057318784
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.050 G 13.080 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:32.50 +35:55:57.6: 13.12 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:32.50 +35:55:57.6: 13.22 +/- 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!
Don'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 904493896057318784,2461199.6494,12.27,0.05,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
Gaia DR3 904493896057318784 20260608.1494 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 06 08.1494 2461199.6494 12.57 08:16:42.55 +33:45:17.1
188.20497 31.49116 galactic Lyn Second-epoch detections are separated by 1.8" 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 | target | 08:16:42.55 +33:45:17.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.555+/-0.029 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:42.55 +33:45:17.1: 13.65 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:42.55 +33:45:17.1: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461199.6494,12.57,0.05,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
target 20260608.1494 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.71 08:19:13.23 +33:35:55.7
188.52596 31.96313 galactic Lyn Second-epoch detections are separated by 1.4" and 7.7 pix
The object was found in VSX 1" Gaia DR3 901802364608119936
Type: ROT
# Max. Min./Amp. JD0 Period
13.430 G 13.450 G G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:13.23 +33:35:55.7: 13.66 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:13.23 +33:35:55.7: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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
Gaia DR3 901802364608119936,2461199.6494,12.71,0.05,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 901802364608119936 20260608.1494 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.64 08:17:37.34 +33:04:14.1
189.03750 31.51459 galactic Cnc Second-epoch detections are separated by 2.5" and 8.2 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 | 08:17:37.34 +33:04:14.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.688+/-0.026 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:37.34 +33:04:14.1: 13.65 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:37.34 +33:04:14.1: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461199.6494,12.64,0.05,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
target 20260608.1494 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.61 08:16:20.96 +35:39:32.8
186.00496 31.84647 galactic Lyn Second-epoch detections are separated by 3.2" and 8.2 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 | 08:16:20.96 +35:39:32.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.571+/-0.024 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:20.96 +35:39:32.8: 13.65 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:20.96 +35:39:32.8: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461199.6494,12.61,0.05,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
target 20260608.1494 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.43 08:16:57.77 +34:38:56.8
187.19671 31.74702 galactic Lyn Second-epoch detections are separated by 1.8" 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 | 08:16:57.77 +34:38:56.8 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.029 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:57.77 +34:38:56.8: 13.65 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:57.77 +34:38:56.8: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461199.6494,12.43,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.56 08:17:39.32 +35:34:25.0
186.17040 32.08743 galactic Lyn Second-epoch detections are separated by 2.5" and 8.0 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 | 08:17:39.32 +35:34:25.0 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.298+/-0.032 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:39.32 +35:34:25.0: 13.63 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:39.32 +35:34:25.0: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461199.6494,12.56,0.05,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
target 20260608.1494 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.46 08:20:36.95 +33:04:22.5
189.20925 32.12451 galactic Cnc Second-epoch detections are separated by 0.5" 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 | 08:20:36.95 +33:04:22.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.499+/-0.026 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:36.95 +33:04:22.5: 13.63 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:36.95 +33:04:22.5: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461199.6494,12.46,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.60 08:19:08.06 +35:08:53.8
186.73759 32.29096 galactic Lyn Second-epoch detections are separated by 0.5" and 7.6 pix
The object was found in VSX 1" Gaia DR3 904199574834819840
Type: ROT
# Max. Min./Amp. JD0 Period
13.410 G 13.450 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:08.06 +35:08:53.8: 13.64 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:08.06 +35:08:53.8: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 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
Gaia DR3 904199574834819840,2461199.6494,12.60,0.05,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 904199574834819840 20260608.1494 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.18 08:21:18.17 +33:33:26.0
188.69113 32.37579 galactic Lyn Second-epoch detections are separated by 0.4" 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 | 08:21:18.17 +33:33:26.0 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.327+/-0.025 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:18.17 +33:33:26.0: 13.18 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:18.17 +33:33:26.0: 13.15 +/- 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!
Don'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,2461199.6494,12.18,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.54 08:19:47.60 +34:32:38.3
187.47013 32.29164 galactic Lyn Second-epoch detections are separated by 1.7" 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 | 08:19:47.60 +34:32:38.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.381+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:47.60 +34:32:38.3: 13.63 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:47.60 +34:32:38.3: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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,2461199.6494,12.54,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.18 08:17:41.84 +34:14:27.8
187.70451 31.80250 galactic Lyn Second-epoch detections are separated by 0.7" 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 | 08:17:41.84 +34:14:27.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.306+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:41.84 +34:14:27.8: 13.17 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:41.84 +34:14:27.8: 13.21 +/- 0.02 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,2461199.6494,12.18,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.17 08:22:04.76 +34:00:12.0
188.21853 32.63308 galactic Lyn Second-epoch detections are separated by 1.1" 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 | 08:22:04.76 +34:00:12.0 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.026 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:04.76 +34:00:12.0: 13.18 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:04.76 +34:00:12.0: 13.20 +/- 0.02 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,2461199.6494,12.17,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.18 08:18:58.87 +34:27:14.1
187.53021 32.10854 galactic Lyn Second-epoch detections are separated by 1.4" 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 | 08:18:58.87 +34:27:14.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.389+/-0.025 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:58.87 +34:27:14.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:58.87 +34:27:14.1: 13.14 +/- 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!
Don'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,2461199.6494,12.18,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.52 08:11:31.03 +33:16:36.4
188.44181 30.32572 galactic Lyn Second-epoch detections are separated by 0.4" 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 | 08:11:31.03 +33:16:36.4 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.283+/-0.033 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:11:31.03 +33:16:36.4: 13.64 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:11:31.03 +33:16:36.4: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 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,2461199.6494,12.52,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.16 08:19:42.25 +33:12:27.5
189.00208 31.97044 galactic Lyn 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 | 08:19:42.25 +33:12:27.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.469+/-0.030 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:42.25 +33:12:27.5: 13.16 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:42.25 +33:12:27.5: 13.12 +/- 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!
Don'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,2461199.6494,12.16,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.21 08:16:31.47 +34:02:21.4
187.86995 31.52005 galactic Lyn Second-epoch detections are separated by 1.0" 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 | target | 08:16:31.47 +34:02:21.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.514+/-0.029 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:31.47 +34:02:21.4: 13.15 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:31.47 +34:02:21.4: 13.15 +/- 0.02 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,2461199.6494,12.21,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.47 08:20:13.36 +33:39:38.5
188.51137 32.18037 galactic Lyn Second-epoch detections are separated by 1.5" and 8.0 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 | 08:20:13.36 +33:39:38.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.538+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:13.36 +33:39:38.5: 13.61 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:13.36 +33:39:38.5: 13.61 +/- 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!
Don'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,2461199.6494,12.47,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.08 08:19:18.44 +34:09:08.9
187.89485 32.10680 galactic Lyn Second-epoch detections are separated by 0.8" 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 | target | 08:19:18.44 +34:09:08.9 (user input) | T | P | (position from user input) J-Ks=0.782+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:18.44 +34:09:08.9: 13.15 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:18.44 +34:09:08.9: 13.10 +/- 0.02 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!
Don'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,2461199.6494,12.08,0.05,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 20260608.1494 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.37 08:20:06.98 +33:43:04.4
188.43962 32.17188 galactic Lyn Second-epoch detections are separated by 0.4" and 7.8 pix
The object was found in VSX 1" Gaia DR3 901816658259266176
Type: RS
# Max. Min./Amp. JD0 Period
13.130 G 13.220 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:06.98 +33:43:04.4: 13.62 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:06.98 +33:43:04.4: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 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
Gaia DR3 901816658259266176,2461199.6494,12.37,0.05,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
Gaia DR3 901816658259266176 20260608.1494 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 06 08.1494 2461199.6494 12.82 08:15:55.13 +33:37:41.3
188.30386 31.30161 galactic Lyn Second-epoch detections are separated by 0.9" 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 | 08:15:55.13 +33:37:41.3 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.371+/-0.034 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:15:55.13 +33:37:41.3: 13.99 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:15:55.13 +33:37:41.3: 14.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
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,2461199.6494,12.82,0.05,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
target 20260608.1494 12.82CV 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 06 08.1494 2461199.6494 12.48 08:17:38.37 +33:06:38.0
188.99297 31.52763 galactic Cnc Second-epoch detections are separated by 0.4" 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 | 08:17:38.37 +33:06:38.0 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.659+/-0.027 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:38.37 +33:06:38.0: 13.62 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:38.37 +33:06:38.0: 13.64 +/- 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!
Don'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,2461199.6494,12.48,0.05,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 20260608.1494 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.63 08:14:54.07 +33:39:39.7
188.20775 31.10366 galactic Lyn Second-epoch detections are separated by 0.4" and 7.8 pix
The object was found in VSX 1" ASASSN-V J081454.02+333939.2
Type: ROT
# Max. Min./Amp. JD0 Period
14.060 g Y 0.110 g 2458609.67800 7.175500000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:14:54.07 +33:39:39.7: 13.59 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:14:54.07 +33:39:39.7: 13.61 +/- 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
ASASSN-V J081454.02+333939.2,2461199.6494,12.63,0.05,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
ASASSN-V J081454.02+333939.2 20260608.1494 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.46 08:19:23.10 +33:34:48.7
188.55663 31.99217 galactic Lyn Second-epoch detections are separated by 2.5" and 8.0 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 | 08:19:23.10 +33:34:48.7 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.314+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:23.10 +33:34:48.7: 13.62 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:23.10 +33:34:48.7: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 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,2461199.6494,12.46,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.65 08:18:27.49 +33:44:42.5
188.31514 31.84256 galactic Lyn 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 | 08:18:27.49 +33:44:42.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.251+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:27.49 +33:44:42.5: 13.62 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:27.49 +33:44:42.5: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 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,2461199.6494,12.65,0.05,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
target 20260608.1494 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 11.48 08:20:01.09 +34:01:21.9
188.08326 32.22104 galactic Lyn Second-epoch detections are separated by 0.6" 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 | ATO J124.9933+34.0232 | 08:20:01.07 +34:01:23.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G9 (LAMOST DR5)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:01.09 +34:01:21.9: 12.44 +/- 0.01 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:01.09 +34:01:21.9: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 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 J124.9933+34.0232,2461199.6494,11.48,0.05,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 J124.9933+34.0232 20260608.1494 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.55 08:21:01.24 +33:17:46.3
188.97585 32.25872 galactic Lyn Second-epoch detections are separated by 0.9" 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 | 08:21:01.24 +33:17:46.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.305+/-0.030 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:01.24 +33:17:46.3: 13.60 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:01.24 +33:17:46.3: 13.60 +/- 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
target,2461199.6494,12.55,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.13 08:18:45.96 +33:52:55.7
188.17539 31.93625 galactic Lyn Second-epoch detections are separated by 2.0" 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 | target | 08:18:45.96 +33:52:55.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.381+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:45.96 +33:52:55.7: 13.13 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:45.96 +33:52:55.7: 13.18 +/- 0.02 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,2461199.6494,12.13,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.48 08:19:27.22 +34:22:04.1
187.65495 32.18441 galactic Lyn Second-epoch detections are separated by 1.3" 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 | 08:19:27.22 +34:22:04.1 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.029 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:27.22 +34:22:04.1: 13.59 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:27.22 +34:22:04.1: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 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,2461199.6494,12.48,0.05,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 20260608.1494 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.59 08:15:06.32 +33:26:21.0
188.47121 31.09195 galactic Lyn Second-epoch detections are separated by 0.8" 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 | 08:15:06.32 +33:26:21.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.294+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:15:06.32 +33:26:21.0: 13.58 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:15:06.32 +33:26:21.0: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 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,2461199.6494,12.59,0.05,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
target 20260608.1494 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.56 08:20:22.14 +34:03:18.9
188.06509 32.29915 galactic Lyn Second-epoch detections are separated by 0.7" 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 | 08:20:22.14 +34:03:18.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.406+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:22.14 +34:03:18.9: 13.58 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:22.14 +34:03:18.9: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 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,2461199.6494,12.56,0.05,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
target 20260608.1494 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.15 08:18:59.76 +34:54:19.4
187.01076 32.21081 galactic Lyn Second-epoch detections are separated by 0.9" 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 | 08:18:59.76 +34:54:19.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.610+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:59.76 +34:54:19.4: 13.12 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:59.76 +34:54:19.4: 13.19 +/- 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!
Don'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,2461199.6494,12.15,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.16 08:19:58.41 +34:39:43.8
187.34327 32.35370 galactic Lyn Second-epoch detections are separated by 0.7" 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 | 08:19:58.41 +34:39:43.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.355+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:58.41 +34:39:43.8: 13.12 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:58.41 +34:39:43.8: 13.14 +/- 0.02 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!
Don'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,2461199.6494,12.16,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.19 08:20:33.25 +33:40:26.4
188.51463 32.25057 galactic Lyn Second-epoch detections are separated by 1.1" 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 | 08:20:33.25 +33:40:26.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.246+/-0.032 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:33.25 +33:40:26.4: 13.12 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:33.25 +33:40:26.4: 13.13 +/- 0.02 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!
Don'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,2461199.6494,12.19,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.47 08:21:07.53 +33:24:45.2
188.84785 32.30677 galactic Lyn Second-epoch detections are separated by 1.4" 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 | 08:21:07.53 +33:24:45.2 (user input) | T | P | (position from user input) J-Ks=0.281+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:07.53 +33:24:45.2: 13.57 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:07.53 +33:24:45.2: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 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,2461199.6494,12.47,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.38 08:21:24.58 +33:59:45.1
188.19064 32.49608 galactic Lyn Second-epoch detections are separated by 0.3" 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 | 08:21:24.58 +33:59:45.1 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:24.58 +33:59:45.1: 13.42 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:24.58 +33:59:45.1: 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!
Don'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,2461199.6494,12.38,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.38 08:16:46.13 +34:52:08.9
186.93402 31.75730 galactic Lyn Second-epoch detections are separated by 1.4" 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 | target | 08:16:46.13 +34:52:08.9 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.249+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:46.13 +34:52:08.9: 13.42 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:46.13 +34:52:08.9: 13.46 +/- 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!
Don'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,2461199.6494,12.38,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.16 08:17:05.24 +34:04:17.3
187.86472 31.64090 galactic Lyn Second-epoch detections are separated by 1.3" 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 | 08:17:05.24 +34:04:17.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.406+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:05.24 +34:04:17.3: 13.12 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:05.24 +34:04:17.3: 13.20 +/- 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!
Don'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,2461199.6494,12.16,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.69 08:17:37.24 +34:42:01.7
187.17333 31.89032 galactic Lyn Second-epoch detections are separated by 2.4" 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 | 08:17:37.24 +34:42:01.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.576+/-0.029 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:37.24 +34:42:01.7: 13.97 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:37.24 +34:42:01.7: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
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,2461199.6494,12.69,0.05,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
target 20260608.1494 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.51 08:09:51.75 +33:35:16.1
187.99413 30.06841 galactic Lyn Second-epoch detections are separated by 2.4" and 8.1 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 | 08:09:51.75 +33:35:16.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.439+/-0.025 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:09:51.75 +33:35:16.1: 13.43 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:09:51.75 +33:35:16.1: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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,2461199.6494,12.51,0.05,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
target 20260608.1494 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.38 08:22:50.48 +33:37:46.5
188.69322 32.70425 galactic Lyn Second-epoch detections are separated by 0.7" and 7.8 pix
The object was found in VSX 3" Gaia DR3 901757456429245824
Type: ROT
# Max. Min./Amp. JD0 Period
12.890 G 12.920 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:50.48 +33:37:46.5: 13.42 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:50.48 +33:37:46.5: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 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 901757456429245824,2461199.6494,12.38,0.05,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
Gaia DR3 901757456429245824 20260608.1494 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 06 08.1494 2461199.6494 11.94 08:16:04.15 +34:02:55.4
187.83356 31.43048 galactic Lyn Second-epoch detections are separated by 1.1" 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 | 08:16:04.15 +34:02:55.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.388+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:04.15 +34:02:55.4: 12.88 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:04.15 +34:02:55.4: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 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,2461199.6494,11.94,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.38 08:17:21.40 +33:21:25.9
188.69542 31.52878 galactic Lyn 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 | 08:17:21.40 +33:21:25.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.362+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:21.40 +33:21:25.9: 13.41 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:21.40 +33:21:25.9: 13.42 +/- 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!
Don'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,2461199.6494,12.38,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.41 08:17:05.59 +35:17:16.2
186.47041 31.91407 galactic Lyn Second-epoch detections are separated by 1.7" 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 | 08:17:05.59 +35:17:16.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.400+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:05.59 +35:17:16.2: 13.43 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:05.59 +35:17:16.2: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 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,2461199.6494,12.41,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 11.88 08:21:21.02 +33:55:58.9
188.26000 32.47009 galactic Lyn Second-epoch detections are separated by 1.0" 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 | 08:21:21.02 +33:55:58.9 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.031 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:21.02 +33:55:58.9: 12.85 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:21.02 +33:55:58.9: 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
target,2461199.6494,11.88,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.40 08:19:10.89 +33:54:45.2
188.16367 32.02713 galactic Lyn Second-epoch detections are separated by 2.7" and 8.1 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 | 08:19:10.89 +33:54:45.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.490+/-0.029 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:10.89 +33:54:45.2: 13.43 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:10.89 +33:54:45.2: 13.46 +/- 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!
Don'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,2461199.6494,12.40,0.05,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
target 20260608.1494 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.14 08:20:38.43 +33:09:17.4
189.11660 32.14863 galactic Lyn Second-epoch detections are separated by 1.2" 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 | 08:20:38.43 +33:09:17.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.429+/-0.024 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:38.43 +33:09:17.4: 13.10 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:38.43 +33:09:17.4: 13.13 +/- 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!
Don'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,2461199.6494,12.14,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.13 08:17:35.81 +34:53:43.5
186.94810 31.92871 galactic Lyn Second-epoch detections are separated by 2.5" and 8.1 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 | 08:17:35.81 +34:53:43.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.338+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:35.81 +34:53:43.5: 13.09 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:35.81 +34:53:43.5: 13.11 +/- 0.02 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,2461199.6494,12.13,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.43 08:22:49.96 +33:40:00.0
188.64978 32.71078 galactic Lyn Second-epoch detections are separated by 1.9" 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 | target | 08:22:49.96 +33:40:00.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.340+/-0.027 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:49.96 +33:40:00.0: 13.40 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:49.96 +33:40:00.0: 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!
Don'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,2461199.6494,12.43,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.13 08:21:14.01 +33:58:17.5
188.20912 32.45506 galactic Lyn Second-epoch detections are separated by 1.6" 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 | ATO J125.3063+33.9673 | 08:21:14.01 +33:58:17.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.357+/-0.029 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:14.01 +33:58:17.5: 13.09 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:14.01 +33:58:17.5: 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!
Don'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 J125.3063+33.9673,2461199.6494,12.13,0.05,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
ATO J125.3063+33.9673 20260608.1494 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 06 08.1494 2461199.6494 12.62 08:11:52.34 +33:13:19.8
188.52445 30.38411 galactic Lyn Second-epoch detections are separated by 1.9" and 8.0 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 | 08:11:52.34 +33:13:19.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.387+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:11:52.34 +33:13:19.8: 13.57 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:11:52.34 +33:13:19.8: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 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,2461199.6494,12.62,0.05,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
target 20260608.1494 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.45 08:21:33.20 +33:18:56.1
188.98381 32.37149 galactic Lyn 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 | 08:21:33.20 +33:18:56.1 (user input) | T | P | (position from user input) J-Ks=0.582+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:33.20 +33:18:56.1: 13.41 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:33.20 +33:18:56.1: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 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,2461199.6494,12.45,0.05,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 20260608.1494 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.11 08:21:21.26 +33:05:50.3
189.22378 32.28063 galactic Cnc 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 | ATO J125.3375+33.0983 | 08:21:21.26 +33:05:50.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:21.26 +33:05:50.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:21.26 +33:05:50.3: 13.07 +/- 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
ATO J125.3375+33.0983,2461199.6494,12.11,0.05,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 J125.3375+33.0983 20260608.1494 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.53 08:15:42.59 +34:39:17.7
187.12187 31.49727 galactic Lyn Second-epoch detections are separated by 0.3" 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 | 08:15:42.59 +34:39:17.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.322+/-0.029 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:15:42.59 +34:39:17.7: 13.54 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:15:42.59 +34:39:17.7: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 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,2461199.6494,12.53,0.05,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
target 20260608.1494 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.46 08:16:50.59 +34:42:52.7
187.11513 31.73772 galactic Lyn Second-epoch detections are separated by 2.5" 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 | 08:16:50.59 +34:42:52.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.417+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:50.59 +34:42:52.7: 13.59 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:50.59 +34:42:52.7: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 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,2461199.6494,12.46,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.53 08:16:29.95 +34:47:10.1
187.01463 31.68484 galactic Lyn Second-epoch detections are separated by 1.9" 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 | target | 08:16:29.95 +34:47:10.1 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.340+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:29.95 +34:47:10.1: 13.55 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:29.95 +34:47:10.1: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 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,2461199.6494,12.53,0.05,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
target 20260608.1494 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 11.88 08:18:23.98 +34:40:39.3
187.24149 32.04139 galactic Lyn Second-epoch detections are separated by 0.3" 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 | 08:18:23.98 +34:40:39.3 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.625+/-0.022 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:23.98 +34:40:39.3: 12.83 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:23.98 +34:40:39.3: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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,2461199.6494,11.88,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 11.90 08:18:05.08 +35:07:52.6
186.70247 32.07776 galactic Lyn Second-epoch detections are separated by 1.6" 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 | 08:18:05.08 +35:07:52.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.384+/-0.029 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:05.08 +35:07:52.6: 12.83 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:05.08 +35:07:52.6: 12.88 +/- 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!
Don'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,2461199.6494,11.90,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 11.89 08:15:53.80 +33:32:50.9
188.39429 31.27801 galactic Lyn Second-epoch detections are separated by 0.8" 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 | 08:15:53.80 +33:32:50.9 (user input) | T | P | (position from user input) J-Ks=0.658+/-0.029 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:15:53.80 +33:32:50.9: 12.83 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:15:53.80 +33:32:50.9: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 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,2461199.6494,11.89,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.88 08:18:54.90 +33:05:01.6
189.09809 31.78076 galactic Cnc 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 | 08:18:54.90 +33:05:01.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.458+/-0.029 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:54.90 +33:05:01.6: 14.13 +/- 0.06 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:54.90 +33:05:01.6: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
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,2461199.6494,12.88,0.05,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 20260608.1494 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.15 08:17:32.05 +34:49:32.2
187.02497 31.90076 galactic Lyn Second-epoch detections are separated by 1.5" 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 | 08:17:32.05 +34:49:32.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.709+/-0.025 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:32.05 +34:49:32.2: 13.09 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:32.05 +34:49:32.2: 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!
Don'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,2461199.6494,12.15,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.10 08:19:33.25 +33:54:06.1
188.19688 32.09996 galactic Lyn 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 | 08:19:33.25 +33:54:06.1 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.322+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:33.25 +33:54:06.1: 13.08 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:33.25 +33:54:06.1: 13.13 +/- 0.02 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,2461199.6494,12.10,0.05,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
target 20260608.1494 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.07 08:19:15.89 +33:45:34.7
188.34392 32.00907 galactic Lyn Second-epoch detections are separated by 0.9" 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 | 08:19:15.89 +33:45:34.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.590+/-0.029 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:15.89 +33:45:34.7: 13.07 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:15.89 +33:45:34.7: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 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,2461199.6494,12.07,0.05,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 20260608.1494 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 11.86 08:20:56.69 +34:02:46.7
188.10694 32.41342 galactic Lyn Second-epoch detections are separated by 0.3" 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 | 08:20:56.69 +34:02:46.7 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.569+/-0.027 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:56.69 +34:02:46.7: 12.80 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:56.69 +34:02:46.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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,2461199.6494,11.86,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.71 08:19:20.41 +33:28:24.5
188.67648 31.95841 galactic Lyn Second-epoch detections are separated by 3.4" and 8.2 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 | 08:19:20.41 +33:28:24.5 (user input) | T | P | (position from user input) J-Ks=0.575+/-0.025 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:20.41 +33:28:24.5: 13.79 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:20.41 +33:28:24.5: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461199.6494,12.71,0.05,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 20260608.1494 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.81 08:21:07.85 +33:14:32.9
189.04395 32.26873 galactic Lyn Second-epoch detections are separated by 4.6" 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 | ATO J125.2820+33.2422 | 08:21:07.85 +33:14:32.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.378+/-0.032 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:07.85 +33:14:32.9: 14.14 +/- 0.06 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:07.85 +33:14:32.9: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
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 J125.2820+33.2422,2461199.6494,12.81,0.05,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
ATO J125.2820+33.2422 20260608.1494 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.68 08:19:40.26 +33:09:22.2
189.05914 31.95164 galactic Lyn Second-epoch detections are separated by 4.6" and 8.2 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 J124.9176+33.1562 | 08:19:40.26 +33:09:22.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.643+/-0.029 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:40.26 +33:09:22.2: 13.81 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:40.26 +33:09:22.2: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 J124.9176+33.1562,2461199.6494,12.68,0.05,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
ATO J124.9176+33.1562 20260608.1494 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 06 08.1494 2461199.6494 12.60 08:18:25.97 +33:34:41.7
188.50478 31.79879 galactic Lyn Second-epoch detections are separated by 1.5" 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 | 08:18:25.97 +33:34:41.7 (user input) | T | P | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.312+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:25.97 +33:34:41.7: 13.82 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:25.97 +33:34:41.7: 13.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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,2461199.6494,12.60,0.05,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
target 20260608.1494 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.62 08:18:33.53 +34:43:18.5
187.19912 32.08306 galactic Lyn Second-epoch detections are separated by 5.9" 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 | ATO J124.6464+34.7208 | 08:18:33.53 +34:43:18.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K3 (LAMOST DR5)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:33.53 +34:43:18.5: 13.77 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:33.53 +34:43:18.5: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 J124.6464+34.7208,2461199.6494,12.62,0.05,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 J124.6464+34.7208 20260608.1494 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.56 08:16:12.75 +33:20:26.0
188.64780 31.29273 galactic Lyn Second-epoch detections are separated by 2.1" 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 | 08:16:12.75 +33:20:26.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:12.75 +33:20:26.0: 13.53 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:12.75 +33:20:26.0: 13.57 +/- 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!
Don'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,2461199.6494,12.56,0.05,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
target 20260608.1494 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.35 08:17:24.84 +34:35:28.7
187.28745 31.82453 galactic Lyn Second-epoch detections are separated by 0.9" 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 | 08:17:24.84 +34:35:28.7 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:24.84 +34:35:28.7: 13.38 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:24.84 +34:35:28.7: 13.40 +/- 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!
Don'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,2461199.6494,12.35,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.43 08:21:56.55 +35:43:30.2
186.20968 32.97081 galactic Lyn Second-epoch detections are separated by 1.0" 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 | target | 08:21:56.55 +35:43:30.2 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.343+/-0.024 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:56.55 +35:43:30.2: 13.39 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:56.55 +35:43:30.2: 13.40 +/- 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!
Don'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,2461199.6494,12.43,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.74 08:20:49.59 +33:31:29.0
188.70180 32.27174 galactic Lyn Second-epoch detections are separated by 1.9" 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 | target | 08:20:49.59 +33:31:29.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.378+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:49.59 +33:31:29.0: 13.97 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:49.59 +33:31:29.0: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.04
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,2461199.6494,12.74,0.05,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 20260608.1494 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.44 08:16:54.89 +35:24:04.2
186.33079 31.90316 galactic Lyn Second-epoch detections are separated by 2.4" and 8.0 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 | 08:16:54.89 +35:24:04.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.329+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:54.89 +35:24:04.2: 13.38 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:54.89 +35:24:04.2: 13.45 +/- 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!
Don'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,2461199.6494,12.44,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.05 08:19:56.18 +33:38:58.7
188.50800 32.11984 galactic Lyn Second-epoch detections are separated by 0.5" 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 | 08:19:56.18 +33:38:58.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.657+/-0.027 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:56.18 +33:38:58.7: 13.06 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:56.18 +33:38:58.7: 13.00 +/- 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,2461199.6494,12.05,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.51 08:20:03.60 +34:50:11.8
187.14620 32.40894 galactic Lyn 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 | target | 08:20:03.60 +34:50:11.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:03.60 +34:50:11.8: 13.43 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:03.60 +34:50:11.8: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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,2461199.6494,12.51,0.05,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
target 20260608.1494 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.11 08:16:55.68 +34:31:58.5
187.32793 31.71391 galactic Lyn Second-epoch detections are separated by 1.7" 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 | 08:16:55.68 +34:31:58.5 (user input) | T | P | (position from user input) J-Ks=0.313+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:55.68 +34:31:58.5: 13.06 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:55.68 +34:31:58.5: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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,2461199.6494,12.11,0.05,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
target 20260608.1494 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.08 08:17:30.67 +33:35:21.2
188.43963 31.61469 galactic Lyn Second-epoch detections are separated by 0.5" 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 | ATO J124.3779+33.5892 | 08:17:30.67 +33:35:21.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.315+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:30.67 +33:35:21.2: 13.05 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:30.67 +33:35:21.2: 13.08 +/- 0.02 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 J124.3779+33.5892,2461199.6494,12.08,0.05,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 J124.3779+33.5892 20260608.1494 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.43 08:20:23.35 +33:19:47.7
188.90106 32.13814 galactic Lyn Second-epoch detections are separated by 0.8" 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 | 08:20:23.35 +33:19:47.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.334+/-0.027 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:23.35 +33:19:47.7: 13.54 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:23.35 +33:19:47.7: 13.58 +/- 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!
Don'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,2461199.6494,12.43,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.54 08:21:33.96 +33:50:36.0
188.37550 32.49366 galactic Lyn Second-epoch detections are separated by 1.4" 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 | 08:21:33.96 +33:50:36.0 (user input) | T | P | (position from user input) J-Ks=0.286+/-0.033 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:33.96 +33:50:36.0: 13.79 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:33.96 +33:50:36.0: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 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,2461199.6494,12.54,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.65 08:18:07.56 +33:41:57.3
188.34889 31.76475 galactic Lyn 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 | target | 08:18:07.56 +33:41:57.3 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.502+/-0.025 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:07.56 +33:41:57.3: 13.83 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:07.56 +33:41:57.3: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461199.6494,12.65,0.05,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
target 20260608.1494 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.07 08:16:56.15 +33:57:55.9
187.97728 31.58593 galactic Lyn Second-epoch detections are separated by 1.3" 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 | 08:16:56.15 +33:57:55.9 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.358+/-0.029 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:56.15 +33:57:55.9: 13.05 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:56.15 +33:57:55.9: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 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,2461199.6494,12.07,0.05,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 20260608.1494 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.47 08:19:26.35 +35:04:03.5
186.84663 32.33452 galactic Lyn Second-epoch detections are separated by 2.1" 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 | 08:19:26.35 +35:04:03.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.342+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:26.35 +35:04:03.5: 13.38 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:26.35 +35:04:03.5: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 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,2461199.6494,12.47,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.48 08:23:15.88 +33:41:01.1
188.65392 32.80218 galactic Lyn Second-epoch detections are separated by 1.7" 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 | 08:23:15.88 +33:41:01.1 (user input) | T | P | (position from user input) J-Ks=0.598+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:23:15.88 +33:41:01.1: 13.52 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:23:15.88 +33:41:01.1: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 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,2461199.6494,12.48,0.05,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 20260608.1494 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.09 08:15:58.79 +34:42:40.0
187.07236 31.56404 galactic Lyn Second-epoch detections are separated by 1.7" 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 | 08:15:58.79 +34:42:40.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.685+/-0.026 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:15:58.79 +34:42:40.0: 13.04 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:15:58.79 +34:42:40.0: 13.03 +/- 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,2461199.6494,12.09,0.05,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 20260608.1494 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.08 08:17:37.33 +33:24:43.7
188.64812 31.59561 galactic Lyn Second-epoch detections are separated by 0.6" 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 | ATO J124.4055+33.4122 | 08:17:37.33 +33:24:43.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.399+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:37.33 +33:24:43.7: 13.03 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:37.33 +33:24:43.7: 13.03 +/- 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
ATO J124.4055+33.4122,2461199.6494,12.08,0.05,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 J124.4055+33.4122 20260608.1494 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.54 08:22:46.63 +33:23:16.0
188.96952 32.63679 galactic Lyn Second-epoch detections are separated by 1.6" 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 | 08:22:46.63 +33:23:16.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.334+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:46.63 +33:23:16.0: 13.37 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:46.63 +33:23:16.0: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 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,2461199.6494,12.54,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.35 08:20:04.70 +33:11:41.8
189.03820 32.04358 galactic Lyn Second-epoch detections are separated by 0.5" and 7.7 pix
The object was found in VSX 1" ASASSN-V J082004.66+331142.3
Type: ROT
# Max. Min./Amp. JD0 Period
13.910 g Y 0.180 g 2459255.66200 6.265600000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:04.70 +33:11:41.8: 13.36 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:04.70 +33:11:41.8: 13.32 +/- 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!
Don'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 J082004.66+331142.3,2461199.6494,12.35,0.05,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
ASASSN-V J082004.66+331142.3 20260608.1494 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 06 08.1494 2461199.6494 12.45 08:22:39.97 +33:17:20.7
189.07738 32.59180 galactic Lyn Second-epoch detections are separated by 0.2" 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 | 08:22:39.97 +33:17:20.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.345+/-0.031 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:39.97 +33:17:20.7: 13.34 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:39.97 +33:17:20.7: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 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,2461199.6494,12.45,0.05,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 20260608.1494 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.28 08:18:28.90 +34:48:24.7
187.09707 32.08631 galactic Lyn Second-epoch detections are separated by 1.5" 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 | 08:18:28.90 +34:48:24.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.423+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:28.90 +34:48:24.7: 13.34 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:28.90 +34:48:24.7: 13.30 +/- 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!
Don'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,2461199.6494,12.28,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.31 08:15:39.78 +33:25:13.3
188.52510 31.20041 galactic Lyn Second-epoch detections are separated by 1.8" and 8.0 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 | 08:15:39.78 +33:25:13.3 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.528+/-0.024 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:15:39.78 +33:25:13.3: 13.35 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:15:39.78 +33:25:13.3: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 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,2461199.6494,12.31,0.05,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 20260608.1494 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.38 08:14:35.28 +36:06:32.0
185.39856 31.59447 galactic Lyn Second-epoch detections are separated by 1.2" 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 J123.6467+36.1088 | 08:14:35.28 +36:06:32.0 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) SpType: M1 (LAMOST DR5) J-Ks=1.089+/-0.028 (M)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:14:35.28 +36:06:32.0: 13.34 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:14:35.28 +36:06:32.0: 13.36 +/- 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!
Don'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 J123.6467+36.1088,2461199.6494,12.38,0.05,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 J123.6467+36.1088 20260608.1494 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 06 08.1494 2461199.6494 12.06 08:22:56.71 +33:35:58.3
188.73378 32.71859 galactic Lyn Second-epoch detections are separated by 1.1" 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 | 08:22:56.71 +33:35:58.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.393+/-0.025 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:56.71 +33:35:58.3: 13.03 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:56.71 +33:35:58.3: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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,2461199.6494,12.06,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.30 08:16:44.74 +35:07:35.4
186.63751 31.80955 galactic Lyn Second-epoch detections are separated by 1.2" and 7.8 pix
The object was found in VSX 1" Gaia DR3 902895279166421888
Type: VAR
# Max. Min./Amp. JD0 Period
13.130 G 13.280 G 0.480367000000 F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:44.74 +35:07:35.4: 13.33 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:44.74 +35:07:35.4: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 902895279166421888,2461199.6494,12.30,0.05,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 902895279166421888 20260608.1494 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 06 08.1494 2461199.6494 11.78 08:18:13.59 +33:56:11.9
188.08274 31.83976 galactic Lyn Second-epoch detections are separated by 0.4" 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 | ATO J124.5565+33.9336 | 08:18:13.59 +33:56:11.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.344+/-0.025 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:13.59 +33:56:11.9: 12.73 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:13.59 +33:56:11.9: 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 J124.5565+33.9336,2461199.6494,11.78,0.05,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 J124.5565+33.9336 20260608.1494 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 06 08.1494 2461199.6494 12.30 08:17:31.70 +34:51:09.2
186.99370 31.90555 galactic Lyn Second-epoch detections are separated by 1.3" 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 | 08:17:31.70 +34:51:09.2 (user input) | T | P | (position from user input) J-Ks=0.282+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:31.70 +34:51:09.2: 13.34 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:31.70 +34:51:09.2: 13.36 +/- 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!
Don'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,2461199.6494,12.30,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.76 08:19:37.23 +34:02:00.7
188.04893 32.14319 galactic Lyn Second-epoch detections are separated by 1.6" 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 | 08:19:37.23 +34:02:00.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.393+/-0.034 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:37.23 +34:02:00.7: 13.96 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:37.23 +34:02:00.7: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.04
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,2461199.6494,12.76,0.05,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
target 20260608.1494 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 11.76 08:20:46.03 +33:46:45.5
188.40519 32.31758 galactic Lyn Second-epoch detections are separated by 0.4" 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 | 08:20:46.03 +33:46:45.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.298+/-0.030 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:46.03 +33:46:45.5: 12.72 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:46.03 +33:46:45.5: 12.70 +/- 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
target,2461199.6494,11.76,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 11.79 08:22:03.28 +33:34:56.4
188.70418 32.53402 galactic Lyn Second-epoch detections are separated by 0.4" and 7.7 pix
The object was found in VSX21" Gaia DR3 901767111516587008
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.380 G 14.430 G A
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:03.28 +33:34:56.4: 12.71 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:03.28 +33:34:56.4: 12.73 +/- 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 901767111516587008,2461199.6494,11.79,0.05,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 901767111516587008 20260608.1494 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.32 08:17:46.18 +34:37:24.5
187.26978 31.90305 galactic Lyn 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 | target | 08:17:46.18 +34:37:24.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.636+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:46.18 +34:37:24.5: 13.33 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:46.18 +34:37:24.5: 13.30 +/- 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!
Don'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,2461199.6494,12.32,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.41 08:16:13.40 +33:35:02.0
188.37174 31.35275 galactic Lyn Second-epoch detections are separated by 1.0" 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 | 08:16:13.40 +33:35:02.0 (user input) | T | P | (position from user input) J-Ks=0.281+/-0.030 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:13.40 +33:35:02.0: 13.32 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:13.40 +33:35:02.0: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 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,2461199.6494,12.41,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.67 08:18:22.00 +33:13:13.6
188.91004 31.70154 galactic Lyn Second-epoch detections are separated by 1.5" and 8.0 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 | 08:18:22.00 +33:13:13.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.281+/-0.029 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:22.00 +33:13:13.6: 13.92 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:22.00 +33:13:13.6: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.04
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,2461199.6494,12.67,0.05,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
target 20260608.1494 12.67CV 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 06 08.1494 2461199.6494 12.60 08:19:48.49 +33:08:59.6
189.07427 31.97808 galactic Lyn 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 | target | 08:19:48.49 +33:08:59.6 (user input) | T | P | (position from user input) SpType: A2/4 2015MNRAS.449.1401H LAMOST J081948.52+330859.8 J-Ks=0.098+/-0.038 (A)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:48.49 +33:08:59.6: 13.77 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:48.49 +33:08:59.6: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461199.6494,12.60,0.05,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
target 20260608.1494 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.64 08:14:08.36 +34:05:45.0
187.67081 31.05290 galactic Lyn Second-epoch detections are separated by 1.0" 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 | target | 08:14:08.36 +34:05:45.0 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.033 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:14:08.36 +34:05:45.0: 13.78 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:14:08.36 +34:05:45.0: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461199.6494,12.64,0.05,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
target 20260608.1494 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.47 08:19:58.90 +34:41:10.8
187.31578 32.36061 galactic Lyn Second-epoch detections are separated by 0.7" 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 | 08:19:58.90 +34:41:10.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.314+/-0.030 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:58.90 +34:41:10.8: 13.51 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:58.90 +34:41:10.8: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 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,2461199.6494,12.47,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.68 08:19:33.24 +34:53:17.9
187.05986 32.31879 galactic Lyn Second-epoch detections are separated by 0.4" 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 | 08:19:33.24 +34:53:17.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.484+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:33.24 +34:53:17.9: 13.77 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:33.24 +34:53:17.9: 13.78 +/- 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!
Don'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,2461199.6494,12.68,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.74 08:16:30.97 +34:23:20.3
187.47004 31.59861 galactic Lyn Second-epoch detections are separated by 3.3" and 8.0 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 | 08:16:30.97 +34:23:20.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.521+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:30.97 +34:23:20.3: 13.91 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:30.97 +34:23:20.3: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.04
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,2461199.6494,12.74,0.05,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 20260608.1494 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.81 08:22:07.37 +33:17:26.4
189.04483 32.48162 galactic Lyn Second-epoch detections are separated by 1.5" 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 | 08:22:07.37 +33:17:26.4 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.540+/-0.025 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:07.37 +33:17:26.4: 13.90 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:07.37 +33:17:26.4: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 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,2461199.6494,12.81,0.05,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 20260608.1494 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.24 08:19:15.88 +35:03:30.5
186.84812 32.29768 galactic Lyn Second-epoch detections are separated by 1.3" 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 | 08:19:15.88 +35:03:30.5 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.030 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:15.88 +35:03:30.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:15.88 +35:03:30.5: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461199.6494,12.24,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.32 08:17:34.21 +34:20:20.8
187.58513 31.79913 galactic Lyn Second-epoch detections are separated by 0.4" 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 | 08:17:34.21 +34:20:20.8 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.027 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:34.21 +34:20:20.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:34.21 +34:20:20.8: 13.33 +/- 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!
Don'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,2461199.6494,12.32,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.29 08:19:25.79 +34:07:48.8
187.92718 32.12649 galactic Lyn Second-epoch detections are separated by 0.0" 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 | 08:19:25.79 +34:07:48.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.609+/-0.029 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:25.79 +34:07:48.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:25.79 +34:07:48.8: 13.37 +/- 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!
Don'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,2461199.6494,12.29,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.43 08:18:10.53 +35:04:01.3
186.78125 32.08194 galactic Lyn Second-epoch detections are separated by 1.0" 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 | target | 08:18:10.53 +35:04:01.3 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.584+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:10.53 +35:04:01.3: 13.52 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:10.53 +35:04:01.3: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 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,2461199.6494,12.43,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.37 08:17:16.28 +33:49:01.3
188.16583 31.61926 galactic Lyn Second-epoch detections are separated by 0.3" 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 | ATO J124.3179+33.8168 | 08:17:16.28 +33:49:01.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.392+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:16.28 +33:49:01.3: 13.32 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:16.28 +33:49:01.3: 13.30 +/- 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!
Don'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 J124.3179+33.8168,2461199.6494,12.37,0.05,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 J124.3179+33.8168 20260608.1494 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 06 08.1494 2461199.6494 12.40 08:19:50.53 +35:08:00.8
186.79130 32.42916 galactic Lyn Second-epoch detections are separated by 1.0" 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 | 08:19:50.53 +35:08:00.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.340+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:50.53 +35:08:00.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:50.53 +35:08:00.8: 13.39 +/- 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!
Don'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,2461199.6494,12.40,0.05,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
target 20260608.1494 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.83 08:14:59.88 +33:17:48.6
188.62619 31.03594 galactic Lyn Second-epoch detections are separated by 1.1" 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 | 08:14:59.88 +33:17:48.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.267+/-0.033 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:14:59.88 +33:17:48.6: 13.93 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:14:59.88 +33:17:48.6: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461199.6494,12.83,0.05,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 20260608.1494 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 11.96 08:17:13.16 +33:16:24.4
188.78287 31.48105 galactic Lyn Second-epoch detections are separated by 0.4" 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 | 08:17:13.16 +33:16:24.4 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.341+/-0.027 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:13.16 +33:16:24.4: 13.00 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:13.16 +33:16:24.4: 12.98 +/- 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,2461199.6494,11.96,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.68 08:18:43.34 +34:30:00.5
187.46302 32.06680 galactic Lyn Second-epoch detections are separated by 0.8" 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 | target | 08:18:43.34 +34:30:00.5 (user input) | T | P | (position from user input) J-Ks=0.552+/-0.026 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:43.34 +34:30:00.5: 13.78 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:43.34 +34:30:00.5: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461199.6494,12.68,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.70 08:20:42.49 +34:41:27.4
187.34888 32.50739 galactic Lyn Second-epoch detections are separated by 3.0" 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 | Large-amplitude variable Gaia DR2 904124945483200256 | 08:20:42.49 +34:41:27.4 (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) SpType: F9 (LAMOST DR5) J-Ks=0.365+/-0.032 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:42.49 +34:41:27.4: 13.75 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:42.49 +34:41:27.4: 13.80 +/- 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!
Don'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 904124945483200256,2461199.6494,12.70,0.05,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 904124945483200256 20260608.1494 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.04 08:20:11.83 +33:13:08.0
189.01756 32.07334 galactic Lyn 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 | 08:20:11.83 +33:13:08.0 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.338+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:11.83 +33:13:08.0: 12.99 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:11.83 +33:13:08.0: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 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
target,2461199.6494,12.04,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 11.97 08:21:57.10 +33:13:05.0
189.11887 32.43014 galactic Lyn Second-epoch detections are separated by 0.9" 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 | 08:21:57.10 +33:13:05.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.290+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:57.10 +33:13:05.0: 12.99 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:57.10 +33:13:05.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 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,2461199.6494,11.97,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.60 08:16:09.78 +34:20:29.7
187.50466 31.51684 galactic Lyn Second-epoch detections are separated by 0.5" 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 | 08:16:09.78 +34:20:29.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.378+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:09.78 +34:20:29.7: 13.71 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:09.78 +34:20:29.7: 13.86 +/- 0.05 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!
Don'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,2461199.6494,12.60,0.05,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
target 20260608.1494 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.04 08:16:55.75 +34:08:28.9
187.77600 31.62509 galactic Lyn Second-epoch detections are separated by 2.0" 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 | 08:16:55.75 +34:08:28.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.341+/-0.027 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:55.75 +34:08:28.9: 12.99 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:55.75 +34:08:28.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 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
target,2461199.6494,12.04,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.66 08:16:09.31 +34:38:31.4
187.16087 31.58358 galactic Lyn Second-epoch detections are separated by 1.0" 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 | 08:16:09.31 +34:38:31.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.380+/-0.027 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:09.31 +34:38:31.4: 13.74 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:09.31 +34:38:31.4: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461199.6494,12.66,0.05,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
target 20260608.1494 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.48 08:20:48.80 +34:20:32.1
187.75788 32.45243 galactic Lyn Second-epoch detections are separated by 0.4" 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 | 08:20:48.80 +34:20:32.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.286+/-0.033 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:48.80 +34:20:32.1: 13.51 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:48.80 +34:20:32.1: 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!
Don'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,2461199.6494,12.48,0.05,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 20260608.1494 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.51 08:14:57.20 +34:26:19.4
187.32678 31.29624 galactic Lyn Second-epoch detections are separated by 2.9" 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 | 08:14:57.20 +34:26:19.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.348+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:14:57.20 +34:26:19.4: 13.51 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:14:57.20 +34:26:19.4: 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!
Don'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,2461199.6494,12.51,0.05,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
target 20260608.1494 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 11.96 08:21:26.83 +33:29:51.6
188.76791 32.39154 galactic Lyn Second-epoch detections are separated by 0.5" 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 | 08:21:26.83 +33:29:51.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.627+/-0.023 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:26.83 +33:29:51.6: 12.98 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:26.83 +33:29:51.6: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 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
target,2461199.6494,11.96,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.02 08:20:36.67 +33:44:46.2
188.43470 32.27850 galactic Lyn Second-epoch detections are separated by 1.1" 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 | 08:20:36.67 +33:44:46.2 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.363+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:36.67 +33:44:46.2: 12.97 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:36.67 +33:44:46.2: 12.90 +/- 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!
Don'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,2461199.6494,12.02,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.39 08:17:35.66 +34:15:50.1
187.67263 31.78696 galactic Lyn Second-epoch detections are separated by 0.6" 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 | ATO J124.3987+34.2642 | 08:17:35.66 +34:15:50.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.459+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:35.66 +34:15:50.1: 13.50 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:35.66 +34:15:50.1: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 J124.3987+34.2642,2461199.6494,12.39,0.05,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
ATO J124.3987+34.2642 20260608.1494 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 06 08.1494 2461199.6494 12.22 08:18:12.84 +35:05:10.2
186.76122 32.09379 galactic Lyn Second-epoch detections are separated by 0.1" 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 | 08:18:12.84 +35:05:10.2 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.569+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:12.84 +35:05:10.2: 13.29 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:12.84 +35:05:10.2: 13.18 +/- 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!
Don'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,2461199.6494,12.22,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.36 08:17:44.72 +34:39:39.5
187.22540 31.90652 galactic Lyn 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 | 08:17:44.72 +34:39:39.5 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:44.72 +34:39:39.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:44.72 +34:39:39.5: 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!
Don'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,2461199.6494,12.36,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.21 08:16:41.73 +34:49:32.9
186.97976 31.73298 galactic Lyn Second-epoch detections are separated by 2.4" and 8.1 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 | 08:16:41.73 +34:49:32.9 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:41.73 +34:49:32.9: 13.28 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:41.73 +34:49:32.9: 13.26 +/- 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!
Don'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,2461199.6494,12.21,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.78 08:18:12.95 +33:06:10.2
189.03551 31.64301 galactic Cnc Second-epoch detections are separated by 0.6" 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 | 08:18:12.95 +33:06:10.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.314+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:12.95 +33:06:10.2: 14.08 +/- 0.06 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:12.95 +33:06:10.2: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.04
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,2461199.6494,12.78,0.05,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
target 20260608.1494 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.30 08:15:31.11 +34:45:00.1
187.00279 31.48048 galactic Lyn Second-epoch detections are separated by 0.7" 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 | target | 08:15:31.11 +34:45:00.1 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.354+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:15:31.11 +34:45:00.1: 13.28 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:15:31.11 +34:45:00.1: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461199.6494,12.30,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.26 08:13:43.13 +34:09:03.7
187.58432 30.98130 galactic Lyn Second-epoch detections are separated by 0.7" 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 | target | 08:13:43.13 +34:09:03.7 (user input) | T | P | (position from user input) J-Ks=0.507+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:13:43.13 +34:09:03.7: 13.26 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:13:43.13 +34:09:03.7: 13.26 +/- 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!
Don'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,2461199.6494,12.26,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.28 08:18:27.64 +34:13:48.5
187.75908 31.95370 galactic Lyn 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 | target | 08:18:27.64 +34:13:48.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.391+/-0.027 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:27.64 +34:13:48.5: 13.27 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:27.64 +34:13:48.5: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 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,2461199.6494,12.28,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.21 08:16:42.66 +34:31:55.4
187.31706 31.67018 galactic Lyn Second-epoch detections are separated by 1.5" 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 | ATO J124.1776+34.5322 | 08:16:42.66 +34:31:55.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.008+/-0.026 (M)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:42.66 +34:31:55.4: 13.27 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:42.66 +34:31:55.4: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 J124.1776+34.5322,2461199.6494,12.21,0.05,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
ATO J124.1776+34.5322 20260608.1494 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 06 08.1494 2461199.6494 12.71 08:16:30.82 +34:16:36.7
187.59804 31.57252 galactic Lyn Second-epoch detections are separated by 3.7" 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 | target | 08:16:30.82 +34:16:36.7 (user input) | T | P | (position from user input) J-Ks=0.448+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:30.82 +34:16:36.7: 14.06 +/- 0.06 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:30.82 +34:16:36.7: 14.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.04
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,2461199.6494,12.71,0.05,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 20260608.1494 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.22 08:17:43.08 +33:21:54.1
188.70741 31.60394 galactic Lyn Second-epoch detections are separated by 0.8" 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 | 08:17:43.08 +33:21:54.1 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.451+/-0.027 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:43.08 +33:21:54.1: 13.24 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:43.08 +33:21:54.1: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 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,2461199.6494,12.22,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.34 08:18:44.02 +33:40:15.1
188.41580 31.88116 galactic Lyn Second-epoch detections are separated by 0.7" 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 | 08:18:44.02 +33:40:15.1 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:44.02 +33:40:15.1: 13.27 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:44.02 +33:40:15.1: 13.26 +/- 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!
Don'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,2461199.6494,12.34,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 11.99 08:20:05.63 +33:22:44.6
188.82777 32.08952 galactic Lyn Second-epoch detections are separated by 0.4" 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 | 08:20:05.63 +33:22:44.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.359+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:05.63 +33:22:44.6: 12.97 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:05.63 +33:22:44.6: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 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,2461199.6494,11.99,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.32 08:17:26.85 +34:49:31.0
187.02071 31.88334 galactic Lyn 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 | 08:17:26.85 +34:49:31.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.610+/-0.025 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:26.85 +34:49:31.0: 13.26 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:26.85 +34:49:31.0: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461199.6494,12.32,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.72 08:18:14.60 +33:41:02.8
188.37286 31.78498 galactic Lyn 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 | 08:18:14.60 +33:41:02.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.447+/-0.026 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:14.60 +33:41:02.8: 13.89 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:14.60 +33:41:02.8: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461199.6494,12.72,0.05,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 20260608.1494 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.93 08:22:01.57 +33:09:19.1
189.19547 32.43088 galactic Lyn Second-epoch detections are separated by 4.2" 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 | target | 08:22:01.57 +33:09:19.1 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.359+/-0.034 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:01.57 +33:09:19.1: 14.07 +/- 0.06 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:01.57 +33:09:19.1: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.04
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,2461199.6494,12.93,0.05,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 20260608.1494 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.57 08:16:31.64 +33:44:21.1
188.21233 31.45077 galactic Lyn Second-epoch detections are separated by 0.7" 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 | 08:16:31.64 +33:44:21.1 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.313+/-0.031 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:31.64 +33:44:21.1: 13.70 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:31.64 +33:44:21.1: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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,2461199.6494,12.57,0.05,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
target 20260608.1494 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.38 08:18:45.92 +34:48:25.0
187.11206 32.14314 galactic Lyn Second-epoch detections are separated by 0.5" 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 | 08:18:45.92 +34:48:25.0 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:45.92 +34:48:25.0: 13.48 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:45.92 +34:48:25.0: 13.40 +/- 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!
Don'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,2461199.6494,12.38,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.48 08:21:46.63 +33:51:39.4
188.36677 32.54033 galactic Lyn Second-epoch detections are separated by 0.8" 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 | target | 08:21:46.63 +33:51:39.4 (user input) | T | P | (position from user input) J-Ks=0.561+/-0.026 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:46.63 +33:51:39.4: 13.48 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:46.63 +33:51:39.4: 13.40 +/- 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!
Don'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,2461199.6494,12.48,0.05,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 20260608.1494 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.40 08:16:10.15 +35:10:07.7
186.55848 31.70390 galactic Lyn Second-epoch detections are separated by 1.9" 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 | 08:16:10.15 +35:10:07.7 (user input) | T | P | (position from user input) J-Ks=0.501+/-0.030 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:10.15 +35:10:07.7: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:10.15 +35:10:07.7: 13.39 +/- 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!
Don'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,2461199.6494,12.40,0.05,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
target 20260608.1494 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.40 08:21:23.89 +33:54:48.4
188.28526 32.47538 galactic Lyn Second-epoch detections are separated by 0.5" 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 | 08:21:23.89 +33:54:48.4 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.029 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:23.89 +33:54:48.4: 13.45 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:23.89 +33:54:48.4: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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,2461199.6494,12.40,0.05,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
target 20260608.1494 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.50 08:22:39.87 +33:29:34.4
188.84162 32.63764 galactic Lyn Second-epoch detections are separated by 1.3" 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 | ATO J125.6582+33.4939 | 08:22:39.87 +33:29:34.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.541+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:39.87 +33:29:34.4: 13.44 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:39.87 +33:29:34.4: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 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 J125.6582+33.4939,2461199.6494,12.50,0.05,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
ATO J125.6582+33.4939 20260608.1494 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 06 08.1494 2461199.6494 12.43 08:18:06.10 +34:12:14.5
187.76927 31.87551 galactic Lyn Second-epoch detections are separated by 1.0" 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 | target | 08:18:06.10 +34:12:14.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.658+/-0.027 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:06.10 +34:12:14.5: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:06.10 +34:12:14.5: 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!
Don'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,2461199.6494,12.43,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.38 08:16:59.34 +33:10:55.3
188.87348 31.41247 galactic Lyn Second-epoch detections are separated by 1.0" 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 | target | 08:16:59.34 +33:10:55.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.283+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:59.34 +33:10:55.3: 13.45 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:59.34 +33:10:55.3: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 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,2461199.6494,12.38,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.64 08:20:06.47 +35:04:28.8
186.87322 32.46967 galactic Lyn Second-epoch detections are separated by 1.3" 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 | 08:20:06.47 +35:04:28.8 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.339+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:06.47 +35:04:28.8: 13.71 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:06.47 +35:04:28.8: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461199.6494,12.64,0.05,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
target 20260608.1494 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.26 08:17:02.21 +34:14:27.8
187.66798 31.66958 galactic Lyn Second-epoch detections are separated by 1.1" 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 J124.2659+34.2408 | 08:17:02.21 +34:14:27.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.301+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:02.21 +34:14:27.8: 13.25 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:02.21 +34:14:27.8: 13.25 +/- 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!
Don'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 J124.2659+34.2408,2461199.6494,12.26,0.05,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
ATO J124.2659+34.2408 20260608.1494 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 06 08.1494 2461199.6494 12.77 08:20:14.67 +34:20:43.2
187.72365 32.33858 galactic Lyn Second-epoch detections are separated by 3.3" and 8.1 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 | 08:20:14.67 +34:20:43.2 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.328+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:14.67 +34:20:43.2: 14.03 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:14.67 +34:20:43.2: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
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,2461199.6494,12.77,0.05,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 20260608.1494 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.56 08:13:35.32 +33:04:21.2
188.79582 30.69528 galactic Cnc Second-epoch detections are separated by 1.4" 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 | 08:13:35.32 +33:04:21.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.576+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:13:35.32 +33:04:21.2: 13.70 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:13:35.32 +33:04:21.2: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461199.6494,12.56,0.05,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
target 20260608.1494 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.22 08:16:24.88 +34:15:07.9
187.62072 31.54696 galactic Lyn Second-epoch detections are separated by 2.8" 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 | ATO J124.1036+34.2523 | 08:16:24.88 +34:15:07.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.554+/-0.025 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:24.88 +34:15:07.9: 13.23 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:24.88 +34:15:07.9: 13.17 +/- 0.02 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!
Don'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 J124.1036+34.2523,2461199.6494,12.22,0.05,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
ATO J124.1036+34.2523 20260608.1494 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 06 08.1494 2461199.6494 12.17 08:17:21.26 +33:50:18.5
188.14602 31.64100 galactic Lyn Second-epoch detections are separated by 1.4" 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 | 08:17:21.26 +33:50:18.5 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:21.26 +33:50:18.5: 13.23 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:21.26 +33:50:18.5: 13.19 +/- 0.03 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!
Don'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,2461199.6494,12.17,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.31 08:18:43.98 +35:43:47.2
186.04468 32.33441 galactic Lyn Second-epoch detections are separated by 2.1" 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 | 08:18:43.98 +35:43:47.2 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.391+/-0.026 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:43.98 +35:43:47.2: 13.22 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:43.98 +35:43:47.2: 13.23 +/- 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!
Don'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,2461199.6494,12.31,0.05,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 20260608.1494 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.29 08:17:37.84 +33:11:01.6
188.90902 31.54328 galactic Lyn Second-epoch detections are separated by 0.8" 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 | Large-amplitude variable Gaia DR2 901690764176725760 | 08:17:37.84 +33:11:01.6 (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) SpType: K1 (LAMOST DR5) J-Ks=0.536+/-0.027 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:37.84 +33:11:01.6: 13.23 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:37.84 +33:11:01.6: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 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 901690764176725760,2461199.6494,12.29,0.05,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
Large-amplitude variable Gaia DR2 901690764176725760 20260608.1494 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 06 08.1494 2461199.6494 12.27 08:22:47.16 +33:07:47.0
189.26831 32.57981 galactic Lyn Second-epoch detections are separated by 2.2" 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 | 08:22:47.16 +33:07:47.0 (user input) | T | P | (position from user input) J-Ks=0.265+/-0.030 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:47.16 +33:07:47.0: 13.25 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:47.16 +33:07:47.0: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 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,2461199.6494,12.27,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.14 08:19:34.60 +34:24:03.6
187.62336 32.21652 galactic Lyn Second-epoch detections are separated by 3.4" 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 | 08:19:34.60 +34:24:03.6 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.343+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:34.60 +34:24:03.6: 13.22 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:34.60 +34:24:03.6: 13.24 +/- 0.03 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!
Don'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,2461199.6494,12.14,0.05,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
target 20260608.1494 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 06 08.1494 2461199.6494 12.58 08:17:11.07 +33:34:33.6
188.43600 31.54545 galactic Lyn Second-epoch detections are separated by 1.9" 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 | 08:17:11.07 +33:34:33.6 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.492+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:11.07 +33:34:33.6: 13.70 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:11.07 +33:34:33.6: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 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,2461199.6494,12.58,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.70 08:11:14.93 +33:20:34.8
188.35140 30.28782 galactic Lyn Second-epoch detections are separated by 0.6" 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 | 08:11:14.93 +33:20:34.8 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.657+/-0.026 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:11:14.93 +33:20:34.8: 13.71 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:11:14.93 +33:20:34.8: 13.65 +/- 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!
Don'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,2461199.6494,12.70,0.05,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 20260608.1494 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.45 08:17:25.57 +34:20:49.9
187.56796 31.77201 galactic Lyn Second-epoch detections are separated by 1.7" 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 | ATO J124.3565+34.3473 | 08:17:25.57 +34:20:49.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.338+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:25.57 +34:20:49.9: 13.44 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:25.57 +34:20:49.9: 13.49 +/- 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!
Don'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 J124.3565+34.3473,2461199.6494,12.45,0.05,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 J124.3565+34.3473 20260608.1494 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.56 08:20:17.88 +34:56:26.7
187.03816 32.47903 galactic Lyn 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 | 08:20:17.88 +34:56:26.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.424+/-0.027 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:17.88 +34:56:26.7: 13.71 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:17.88 +34:56:26.7: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.65 +/- 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,2461199.6494,12.56,0.05,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
target 20260608.1494 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.61 08:21:17.38 +34:00:03.0
188.17833 32.47294 galactic Lyn Second-epoch detections are separated by 2.5" and 7.2 pix
The object was found in VSX 0" Gaia DR3 901827996972860416
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.490 G 13.520 G A
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:17.38 +34:00:03.0: 13.70 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:17.38 +34:00:03.0: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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
Gaia DR3 901827996972860416,2461199.6494,12.61,0.05,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 901827996972860416 20260608.1494 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.51 08:18:19.87 +33:24:04.3
188.70146 31.73686 galactic Lyn Second-epoch detections are separated by 2.3" and 8.0 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 | 08:18:19.87 +33:24:04.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.317+/-0.027 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:19.87 +33:24:04.3: 13.45 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:19.87 +33:24:04.3: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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,2461199.6494,12.51,0.05,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
target 20260608.1494 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.64 08:20:17.85 +34:40:13.1
187.35105 32.42049 galactic Lyn Second-epoch detections are separated by 0.1" and 7.7 pix
The object was found in VSX 1" Gaia DR3 904119585363970944
Type: RS
# Max. Min./Amp. JD0 Period
13.480 G 13.540 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:17.85 +34:40:13.1: 13.70 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:17.85 +34:40:13.1: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 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
Gaia DR3 904119585363970944,2461199.6494,12.64,0.05,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
Gaia DR3 904119585363970944 20260608.1494 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.53 08:20:27.84 +34:31:34.7
187.52638 32.42252 galactic Lyn 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 | target | 08:20:27.84 +34:31:34.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.353+/-0.029 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:27.84 +34:31:34.7: 13.68 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:27.84 +34:31:34.7: 13.68 +/- 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!
Don'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,2461199.6494,12.53,0.05,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
target 20260608.1494 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.79 08:22:38.90 +33:07:28.3
189.26647 32.55056 galactic Lyn Second-epoch detections are separated by 4.0" and 8.2 pix
The object was found in VSX 0" Gaia DR3 901548789738859648
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.640 G 13.670 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:22:38.90 +33:07:28.3: 13.87 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:22:38.90 +33:07:28.3: 13.78 +/- 0.04 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!
Don'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 901548789738859648,2461199.6494,12.79,0.05,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 901548789738859648 20260608.1494 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.59 08:19:20.27 +34:29:34.7
187.50448 32.18888 galactic Lyn Second-epoch detections are separated by 1.3" 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 | 08:19:20.27 +34:29:34.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.452+/-0.027 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:20.27 +34:29:34.7: 13.69 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:20.27 +34:29:34.7: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 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,2461199.6494,12.59,0.05,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
target 20260608.1494 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.23 08:20:31.97 +35:18:38.1
186.62157 32.60452 galactic Lyn Second-epoch detections are separated by 1.2" and 7.4 pix
The object was found in VSX 4" HAT-178-0001734
Type: VAR
# Max. Min./Amp. JD0 Period
13.061 V Y 0.014 V 38.523148000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:31.97 +35:18:38.1: 13.21 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:31.97 +35:18:38.1: 13.29 +/- 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!
Don'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
HAT-178-0001734,2461199.6494,12.23,0.05,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
HAT-178-0001734 20260608.1494 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 06 08.1494 2461199.6494 12.61 08:17:15.68 +34:52:54.1
186.94597 31.85858 galactic Lyn Second-epoch detections are separated by 0.2" 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 | 08:17:15.68 +34:52:54.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.434+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:15.68 +34:52:54.1: 13.69 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:15.68 +34:52:54.1: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 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,2461199.6494,12.61,0.05,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
target 20260608.1494 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.90 08:20:31.24 +33:38:06.6
188.55746 32.23494 galactic Lyn Second-epoch detections are separated by 1.4" 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 | 08:20:31.24 +33:38:06.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.450+/-0.034 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:31.24 +33:38:06.6: 14.19 +/- 0.06 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:31.24 +33:38:06.6: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.04
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,2461199.6494,12.90,0.05,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 20260608.1494 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.60 08:16:16.96 +35:09:56.3
186.56812 31.72583 galactic Lyn Second-epoch detections are separated by 2.7" 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 | target | 08:16:16.96 +35:09:56.3 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.032 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:16.96 +35:09:56.3: 13.68 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:16.96 +35:09:56.3: 13.66 +/- 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!
Don'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,2461199.6494,12.60,0.05,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
target 20260608.1494 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.65 08:16:46.47 +33:24:58.2
188.59449 31.42468 galactic Lyn Second-epoch detections are separated by 0.9" and 7.8 pix
The object was found in VSX 0" Gaia DR3 902448327690237568
Type: E
# Max. Min./Amp. JD0 Period
13.550 G 13.650 G 0.503220000000 F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:46.47 +33:24:58.2: 13.66 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:46.47 +33:24:58.2: 13.71 +/- 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!
Don'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 902448327690237568,2461199.6494,12.65,0.05,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 902448327690237568 20260608.1494 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.65 08:15:25.78 +34:36:10.6
187.16586 31.42934 galactic Lyn Second-epoch detections are separated by 1.4" 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 | 08:15:25.78 +34:36:10.6 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.337+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:15:25.78 +34:36:10.6: 13.67 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:15:25.78 +34:36:10.6: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 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,2461199.6494,12.65,0.05,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
target 20260608.1494 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.72 08:21:01.98 +33:40:55.4
188.53210 32.34941 galactic Lyn Second-epoch detections are separated by 2.4" 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 | 08:21:01.98 +33:40:55.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.506+/-0.025 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:01.98 +33:40:55.4: 14.04 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:01.98 +33:40:55.4: 14.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.04
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,2461199.6494,12.72,0.05,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 20260608.1494 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.17 08:19:46.62 +33:37:59.6
188.51789 32.08380 galactic Lyn Second-epoch detections are separated by 0.4" 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 | 08:19:46.62 +33:37:59.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.294+/-0.031 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:46.62 +33:37:59.6: 13.21 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:46.62 +33:37:59.6: 13.19 +/- 0.02 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!
Don'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,2461199.6494,12.17,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.22 08:18:06.93 +33:36:21.3
188.45505 31.74095 galactic Lyn Second-epoch detections are separated by 0.9" 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 | 08:18:06.93 +33:36:21.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:06.93 +33:36:21.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:06.93 +33:36:21.3: 13.21 +/- 0.03 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!
Don'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,2461199.6494,12.22,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.64 08:16:43.93 +33:43:11.7
188.24600 31.48766 galactic Lyn Second-epoch detections are separated by 0.7" and 7.6 pix
The object was found in VSX 1" CSS_J081643.8+334311
Type: EA
# Max. Min./Amp. JD0 Period
13.660 CV Y 0.460 CV 0.599233000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:16:43.93 +33:43:11.7: 13.66 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:16:43.93 +33:43:11.7: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 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
CSS_J081643.8+334311,2461199.6494,12.64,0.05,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
CSS_J081643.8+334311 20260608.1494 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.76 08:20:20.12 +33:33:00.8
188.64477 32.17795 galactic Lyn Second-epoch detections are separated by 1.1" 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 | 08:20:20.12 +33:33:00.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.391+/-0.033 (G)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:20:20.12 +33:33:00.8: 14.03 +/- 0.05 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:20:20.12 +33:33:00.8: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
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,2461199.6494,12.76,0.05,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
target 20260608.1494 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.17 08:19:29.24 +34:36:32.3
187.37877 32.24448 galactic Lyn Second-epoch detections are separated by 1.4" 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 | target | 08:19:29.24 +34:36:32.3 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.308+/-0.027 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:19:29.24 +34:36:32.3: 13.19 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:19:29.24 +34:36:32.3: 13.14 +/- 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!
Don'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,2461199.6494,12.17,0.05,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 20260608.1494 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 06 08.1494 2461199.6494 12.60 08:18:40.33 +33:29:22.3
188.61997 31.82666 galactic Lyn Second-epoch detections are separated by 1.4" 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 | 08:18:40.33 +33:29:22.3 (user input) | T | P | (position from user input) J-Ks=0.274+/-0.028 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:18:40.33 +33:29:22.3: 13.65 +/- 0.04 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:18:40.33 +33:29:22.3: 13.70 +/- 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!
Don'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,2461199.6494,12.60,0.05,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
target 20260608.1494 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1494 2461199.6494 12.43 08:17:14.01 +33:49:19.7
188.15785 31.61281 galactic Lyn Second-epoch detections are separated by 1.8" and 8.0 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 J124.3179+33.8168 | 08:17:14.01 +33:49:19.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.522+/-0.030 (K)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:17:14.01 +33:49:19.7: 13.44 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:17:14.01 +33:49:19.7: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 J124.3179+33.8168,2461199.6494,12.43,0.05,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
ATO J124.3179+33.8168 20260608.1494 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 06 08.1494 2461199.6494 12.87 08:21:10.19 +33:26:44.4
188.81221 32.32336 galactic Lyn Second-epoch detections are separated by 2.9" and 8.0 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 | 08:21:10.19 +33:26:44.4 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.315+/-0.030 (F)
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:21:10.19 +33:26:44.4: 14.17 +/- 0.06 detection
Forced photometry on wcs_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:21:10.19 +33:26:44.4: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
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,2461199.6494,12.87,0.05,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
target 20260608.1494 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
ERROR running VaST on the field Lyn-06-Q1b1x1 (wrong field? clouds? very bad focus?)
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.72163340 22.02.2026 05:18:59.126 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
First image: 2461093.72163340 22.02.2026 05:18:59.126 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Last image: 2461199.64967128 08.06.2026 03:35:21.599 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Lyn-06-Q1b1x1_233240_TTUQ1b1x1_826851_r1aPi9WG/fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 217
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 16 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 54036
Objects passed selection criteria: 53830
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: 32999.8
Average stars matched: 31778.8 (96.3 %)
Memory usage VmPeak: 155016 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 7 23:36:43 CDT 2026
Host name: tau
############################################################
**** FOUND 09:09:01.42 +41:44:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09663_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 09663_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12434_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12434_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07498_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07498_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 03493_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 03493_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 15465_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 15465_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 11589_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11589_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 11250_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11250_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 09771_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 09771_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 15116_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 15116_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07927_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07927_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08222_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08222_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05697_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05697_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 19499_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 19499_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 19548_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 19548_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07861_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07861_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06752_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06752_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04233_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04233_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 18340_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 18340_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12594_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12594_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 17642_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 17642_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 03869_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 03869_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 15090_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 15090_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06291_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06291_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 11665_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11665_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10269_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10269_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08472_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08472_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 11249_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11249_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06142_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06142_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04659_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04659_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 09372_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 09372_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06960_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06960_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 09573_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 09573_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07233_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07233_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07303_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07303_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04453_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04453_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07596_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07596_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06622_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06622_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07568_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07568_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08800_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08800_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04986_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04986_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08241_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08241_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10776_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10776_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06469_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06469_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08995_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08995_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13708_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13708_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12231_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12231_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06966_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06966_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05550_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05550_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08542_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08542_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13810_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13810_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 09475_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 09475_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12815_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12815_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07920_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07920_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06475_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06475_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 09483_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 09483_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05724_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05724_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 16153_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 16153_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08188_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08188_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08371_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08371_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04291_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04291_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13829_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13829_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06639_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06639_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08414_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08414_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05800_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05800_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05005_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05005_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 03884_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 03884_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12800_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12800_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12992_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12992_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13411_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13411_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12405_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12405_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 15140_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 15140_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06876_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06876_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04191_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04191_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13440_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13440_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08226_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08226_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07512_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07512_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08818_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08818_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06119_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06119_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04682_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04682_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04400_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04400_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06740_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06740_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12785_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12785_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05783_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05783_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09784_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
The candidate 09784_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055 did not pass the final checks
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Considering the candidate 12191_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12191_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 17898_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 17898_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06199_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06199_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 16761_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 16761_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06916_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06916_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13176_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13176_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 52435_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
The candidate 52435_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:16:46.88 +40:07:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11962_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11962_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06907_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06907_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05214_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05214_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07716_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07716_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07363_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07363_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08932_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08932_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 14549_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 14549_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06692_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06692_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 15712_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
The candidate 15712_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:25:31.39 +35:24:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13053_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13053_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05961_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05961_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05211_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05211_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04556_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04556_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04729_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04729_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13239_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13239_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06302_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06302_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 21104_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 21104_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06310_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06310_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 15304_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 15304_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08568_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08568_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13630_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13630_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08976_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08976_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07413_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07413_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06264_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06264_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12336_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12336_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07022_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07022_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04912_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04912_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04371_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04371_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10014_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10014_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12363_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12363_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13574_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13574_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11252_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11252_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04799_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04799_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14554_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 14554_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10858_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10858_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09474_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 09474_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14711_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 14711_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08059_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08059_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 14893_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 14893_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05750_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05750_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05323_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05323_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 11560_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11560_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12319_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12319_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04618_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04618_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04443_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04443_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 11055_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11055_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 09869_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 09869_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12685_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12685_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10432_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10432_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 11726_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11726_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05963_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05963_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07275_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07275_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10451_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10451_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 14844_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 14844_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12542_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12542_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13567_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13567_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04347_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04347_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13332_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13332_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10349_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10349_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10137_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10137_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 11984_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11984_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10687_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10687_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05723_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05723_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07147_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07147_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05511_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05511_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13497_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13497_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07286_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07286_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04171_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04171_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07796_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07796_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13226_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13226_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07758_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07758_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 15611_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 15611_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08069_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08069_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05782_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05782_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10071_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10071_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04881_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04881_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 14521_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 14521_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10395_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10395_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10541_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10541_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04781_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04781_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10517_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10517_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08189_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08189_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 18361_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 18361_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 04793_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 04793_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 03915_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 03915_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10845_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10845_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06896_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06896_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06494_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06494_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 10916_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 10916_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13757_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13757_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08571_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08571_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05859_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05859_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12257_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12257_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 11485_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11485_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 03926_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 03926_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 11456_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 11456_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 15748_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 15748_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 13831_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 13831_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06776_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06776_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 15605_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 15605_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06141_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06141_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12556_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12556_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06993_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06993_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06842_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06842_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06858_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06858_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 07687_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 07687_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 06414_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06414_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 12028_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 12028_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 15573_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
The candidate 15573_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:20:12.10 +35:16:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06279_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 06279_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 08099_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 08099_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
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Considering the candidate 05734_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
Preparing report for the candidate 05734_fd_Lyn-06-Q1b1x1_2026-06-07_22-35-21_20.00sec_0.00C_LIGHTs_0055
make_report_in_HTML.sh Phase 2 (HTML assembly): 11s
make_report_in_HTML.sh TOTAL: 387s
Prepared the HTML report for the field Lyn-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:22:36.91 +33:02:32.4
08:20:36.95 +33:04:22.5
08:21:21.26 +33:05:50.3
08:22:47.16 +33:07:47.0
08:22:38.90 +33:07:28.3
08:22:01.57 +33:09:19.1
08:18:54.90 +33:05:01.6
08:17:37.34 +33:04:14.1
08:20:38.43 +33:09:17.4
08:18:12.95 +33:06:10.2
08:19:48.49 +33:08:59.6
08:19:40.26 +33:09:22.2
08:21:57.10 +33:13:05.0
08:17:38.37 +33:06:38.0
08:20:04.70 +33:11:41.8
08:20:11.83 +33:13:08.0
08:19:42.25 +33:12:27.5
08:21:07.85 +33:14:32.9
08:22:39.97 +33:17:20.7
08:13:35.32 +33:04:21.2
08:17:37.84 +33:11:01.6
08:22:07.37 +33:17:26.4
08:16:59.34 +33:10:55.3
08:18:22.00 +33:13:13.6
08:21:01.24 +33:17:46.3
08:21:33.20 +33:18:56.1
08:22:46.63 +33:23:16.0
08:20:23.35 +33:19:47.7
08:17:13.16 +33:16:24.4
08:20:05.63 +33:22:44.6
08:21:07.53 +33:24:45.2
08:21:22.94 +33:26:34.3
08:17:43.08 +33:21:54.1
08:17:21.40 +33:21:25.9
08:21:10.19 +33:26:44.4
08:14:59.88 +33:17:48.6
08:22:39.87 +33:29:34.4
08:16:12.75 +33:20:26.0
08:11:52.34 +33:13:19.8
08:18:19.87 +33:24:04.3
08:17:37.33 +33:24:43.7
08:21:26.83 +33:29:51.6
08:19:20.41 +33:28:24.5
08:16:46.47 +33:24:58.2
08:11:31.03 +33:16:36.4
08:20:49.59 +33:31:29.0
08:22:03.28 +33:34:56.4
08:18:40.33 +33:29:22.3
08:21:18.17 +33:33:26.0
08:15:39.78 +33:25:13.3
08:22:56.71 +33:35:58.3
08:20:20.12 +33:33:00.8
08:15:06.32 +33:26:21.0
08:22:50.48 +33:37:46.5
08:11:14.93 +33:20:34.8
08:19:23.10 +33:34:48.7
08:22:49.96 +33:40:00.0
08:23:15.88 +33:41:01.1
08:18:25.97 +33:34:41.7
08:19:13.23 +33:35:55.7
08:20:31.24 +33:38:06.6
08:19:46.62 +33:37:59.6
08:18:06.93 +33:36:21.3
08:15:53.80 +33:32:50.9
08:17:11.07 +33:34:33.6
08:17:30.67 +33:35:21.2
08:19:56.18 +33:38:58.7
08:20:13.36 +33:39:38.5
08:20:33.25 +33:40:26.4
08:21:01.98 +33:40:55.4
08:16:13.40 +33:35:02.0
08:18:44.02 +33:40:15.1
08:20:06.98 +33:43:04.4
08:20:36.67 +33:44:46.2
08:18:14.60 +33:41:02.8
08:15:55.13 +33:37:41.3
08:18:07.56 +33:41:57.3
08:20:46.03 +33:46:45.5
08:18:33.85 +33:44:02.0
08:19:15.89 +33:45:34.7
08:18:27.49 +33:44:42.5
08:14:54.07 +33:39:39.7
08:16:43.93 +33:43:11.7
08:21:33.96 +33:50:36.0
08:21:46.63 +33:51:39.4
08:16:31.64 +33:44:21.1
08:16:42.55 +33:45:17.1
08:09:51.75 +33:35:16.1
08:19:22.24 +33:50:04.1
08:17:16.28 +33:49:01.3
08:21:23.89 +33:54:48.4
08:17:14.01 +33:49:19.7
08:21:21.02 +33:55:58.9
08:17:21.26 +33:50:18.5
08:11:25.07 +33:41:01.7
08:19:33.25 +33:54:06.1
08:18:45.96 +33:52:55.7
08:19:10.89 +33:54:45.2
08:21:14.01 +33:58:17.5
08:22:04.76 +34:00:12.0
08:21:24.58 +33:59:45.1
08:18:13.59 +33:56:11.9
08:21:17.38 +34:00:03.0
08:20:01.09 +34:01:21.9
08:20:56.69 +34:02:46.7
08:16:56.15 +33:57:55.9
08:19:37.23 +34:02:00.7
08:20:22.14 +34:03:18.9
08:16:31.47 +34:02:21.4
08:19:25.79 +34:07:48.8
08:17:05.24 +34:04:17.3
08:16:04.15 +34:02:55.4
08:19:18.44 +34:09:08.9
08:16:27.40 +34:05:41.0
08:18:12.71 +34:08:55.0
08:16:55.75 +34:08:28.9
08:14:08.36 +34:05:45.0
08:18:06.10 +34:12:14.5
08:18:27.64 +34:13:48.5
08:17:41.84 +34:14:27.8
08:13:43.13 +34:09:03.7
08:17:02.21 +34:14:27.8
08:20:48.80 +34:20:32.1
08:17:35.66 +34:15:50.1
08:16:24.88 +34:15:07.9
08:20:14.67 +34:20:43.2
08:16:30.82 +34:16:36.7
08:19:27.22 +34:22:04.1
08:19:34.60 +34:24:03.6
08:17:34.21 +34:20:20.8
08:17:25.57 +34:20:49.9
08:16:09.78 +34:20:29.7
08:18:58.87 +34:27:14.1
08:14:36.92 +34:20:36.7
08:16:30.97 +34:23:20.3
08:19:20.27 +34:29:34.7
08:20:27.84 +34:31:34.7
08:18:43.34 +34:30:00.5
08:19:32.52 +34:31:14.7
08:19:47.60 +34:32:38.3
08:14:57.20 +34:26:19.4
08:16:55.68 +34:31:58.5
08:16:42.66 +34:31:55.4
08:19:29.24 +34:36:32.3
08:17:24.84 +34:35:28.7
08:19:58.41 +34:39:43.8
08:20:17.85 +34:40:13.1
08:20:42.49 +34:41:27.4
08:17:46.18 +34:37:24.5
08:19:58.90 +34:41:10.8
08:18:23.98 +34:40:39.3
08:17:27.79 +34:37:59.7
08:17:44.72 +34:39:39.5
08:15:25.78 +34:36:10.6
08:16:57.77 +34:38:56.8
08:16:09.31 +34:38:31.4
08:18:33.53 +34:43:18.5
08:15:42.59 +34:39:17.7
08:17:37.24 +34:42:01.7
08:16:50.59 +34:42:52.7
08:15:58.79 +34:42:40.0
08:20:03.60 +34:50:11.8
08:18:45.92 +34:48:25.0
08:18:28.90 +34:48:24.7
08:15:31.11 +34:45:00.1
08:16:29.95 +34:47:10.1
08:17:32.05 +34:49:32.2
08:17:26.85 +34:49:31.0
08:16:41.73 +34:49:32.9
08:19:33.24 +34:53:17.9
08:17:31.70 +34:51:09.2
08:18:59.76 +34:54:19.4
08:20:17.88 +34:56:26.7
08:16:46.13 +34:52:08.9
08:17:35.81 +34:53:43.5
08:17:15.68 +34:52:54.1
08:20:06.47 +35:04:28.8
08:19:26.35 +35:04:03.5
08:19:15.88 +35:03:30.5
08:18:10.53 +35:04:01.3
08:18:12.84 +35:05:10.2
08:19:50.53 +35:08:00.8
08:19:08.06 +35:08:53.8
08:15:50.19 +35:03:52.1
08:18:05.08 +35:07:52.6
08:16:44.74 +35:07:35.4
08:17:23.35 +35:10:26.2
08:16:16.96 +35:09:56.3
08:16:10.15 +35:10:07.7
08:20:31.97 +35:18:38.1
08:17:05.59 +35:17:16.2
08:16:54.89 +35:24:04.2
08:17:39.32 +35:34:25.0
08:21:56.55 +35:43:30.2
08:16:20.96 +35:39:32.8
08:18:43.98 +35:43:47.2
08:16:44.61 +35:52:49.6
08:18:32.50 +35:55:57.6
08:14:35.28 +36:06:32.0
########### Completed Lyn-06-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 ####
08:16:27.40 +34:05:41.0
08:17:27.79 +34:37:59.7
08:18:33.85 +33:44:02.0
08:22:36.91 +33:02:32.4
08:17:23.35 +35:10:26.2
08:19:32.52 +34:31:14.7
08:14:36.92 +34:20:36.7
08:18:12.71 +34:08:55.0
08:15:50.19 +35:03:52.1
08:19:22.24 +33:50:04.1
08:11:25.07 +33:41:01.7
08:21:22.94 +33:26:34.3
08:16:44.61 +35:52:49.6
08:18:32.50 +35:55:57.6
08:16:42.55 +33:45:17.1
08:19:13.23 +33:35:55.7
08:17:37.34 +33:04:14.1
08:16:20.96 +35:39:32.8
08:16:57.77 +34:38:56.8
08:17:39.32 +35:34:25.0
08:20:36.95 +33:04:22.5
08:19:08.06 +35:08:53.8
08:21:18.17 +33:33:26.0
08:19:47.60 +34:32:38.3
08:17:41.84 +34:14:27.8
08:22:04.76 +34:00:12.0
08:18:58.87 +34:27:14.1
08:11:31.03 +33:16:36.4
08:19:42.25 +33:12:27.5
08:16:31.47 +34:02:21.4
08:20:13.36 +33:39:38.5
08:19:18.44 +34:09:08.9
08:20:06.98 +33:43:04.4
08:15:55.13 +33:37:41.3
08:17:38.37 +33:06:38.0
08:14:54.07 +33:39:39.7
08:19:23.10 +33:34:48.7
08:18:27.49 +33:44:42.5
08:20:01.09 +34:01:21.9
08:21:01.24 +33:17:46.3
08:18:45.96 +33:52:55.7
08:19:27.22 +34:22:04.1
08:15:06.32 +33:26:21.0
08:20:22.14 +34:03:18.9
08:18:59.76 +34:54:19.4
08:19:58.41 +34:39:43.8
08:20:33.25 +33:40:26.4
08:21:07.53 +33:24:45.2
08:21:24.58 +33:59:45.1
08:16:46.13 +34:52:08.9
08:17:05.24 +34:04:17.3
08:17:37.24 +34:42:01.7
08:09:51.75 +33:35:16.1
08:22:50.48 +33:37:46.5
08:16:04.15 +34:02:55.4
08:17:21.40 +33:21:25.9
08:17:05.59 +35:17:16.2
08:21:21.02 +33:55:58.9
08:19:10.89 +33:54:45.2
08:20:38.43 +33:09:17.4
08:17:35.81 +34:53:43.5
08:22:49.96 +33:40:00.0
08:21:14.01 +33:58:17.5
08:11:52.34 +33:13:19.8
08:21:33.20 +33:18:56.1
08:21:21.26 +33:05:50.3
08:15:42.59 +34:39:17.7
08:16:50.59 +34:42:52.7
08:16:29.95 +34:47:10.1
08:18:23.98 +34:40:39.3
08:18:05.08 +35:07:52.6
08:15:53.80 +33:32:50.9
08:18:54.90 +33:05:01.6
08:17:32.05 +34:49:32.2
08:19:33.25 +33:54:06.1
08:19:15.89 +33:45:34.7
08:20:56.69 +34:02:46.7
08:19:20.41 +33:28:24.5
08:21:07.85 +33:14:32.9
08:19:40.26 +33:09:22.2
08:18:25.97 +33:34:41.7
08:18:33.53 +34:43:18.5
08:16:12.75 +33:20:26.0
08:17:24.84 +34:35:28.7
08:21:56.55 +35:43:30.2
08:20:49.59 +33:31:29.0
08:16:54.89 +35:24:04.2
08:19:56.18 +33:38:58.7
08:20:03.60 +34:50:11.8
08:16:55.68 +34:31:58.5
08:17:30.67 +33:35:21.2
08:20:23.35 +33:19:47.7
08:21:33.96 +33:50:36.0
08:18:07.56 +33:41:57.3
08:16:56.15 +33:57:55.9
08:19:26.35 +35:04:03.5
08:23:15.88 +33:41:01.1
08:15:58.79 +34:42:40.0
08:17:37.33 +33:24:43.7
08:22:46.63 +33:23:16.0
08:20:04.70 +33:11:41.8
08:22:39.97 +33:17:20.7
08:18:28.90 +34:48:24.7
08:15:39.78 +33:25:13.3
08:14:35.28 +36:06:32.0
08:22:56.71 +33:35:58.3
08:16:44.74 +35:07:35.4
08:18:13.59 +33:56:11.9
08:17:31.70 +34:51:09.2
08:19:37.23 +34:02:00.7
08:20:46.03 +33:46:45.5
08:22:03.28 +33:34:56.4
08:17:46.18 +34:37:24.5
08:16:13.40 +33:35:02.0
08:18:22.00 +33:13:13.6
08:19:48.49 +33:08:59.6
08:14:08.36 +34:05:45.0
08:19:58.90 +34:41:10.8
08:19:33.24 +34:53:17.9
08:16:30.97 +34:23:20.3
08:22:07.37 +33:17:26.4
08:19:15.88 +35:03:30.5
08:17:34.21 +34:20:20.8
08:19:25.79 +34:07:48.8
08:18:10.53 +35:04:01.3
08:17:16.28 +33:49:01.3
08:19:50.53 +35:08:00.8
08:14:59.88 +33:17:48.6
08:17:13.16 +33:16:24.4
08:18:43.34 +34:30:00.5
08:20:42.49 +34:41:27.4
08:20:11.83 +33:13:08.0
08:21:57.10 +33:13:05.0
08:16:09.78 +34:20:29.7
08:16:55.75 +34:08:28.9
08:16:09.31 +34:38:31.4
08:20:48.80 +34:20:32.1
08:14:57.20 +34:26:19.4
08:21:26.83 +33:29:51.6
08:20:36.67 +33:44:46.2
08:17:35.66 +34:15:50.1
08:18:12.84 +35:05:10.2
08:17:44.72 +34:39:39.5
08:16:41.73 +34:49:32.9
08:18:12.95 +33:06:10.2
08:15:31.11 +34:45:00.1
08:13:43.13 +34:09:03.7
08:18:27.64 +34:13:48.5
08:16:42.66 +34:31:55.4
08:16:30.82 +34:16:36.7
08:17:43.08 +33:21:54.1
08:18:44.02 +33:40:15.1
08:20:05.63 +33:22:44.6
08:17:26.85 +34:49:31.0
08:18:14.60 +33:41:02.8
08:22:01.57 +33:09:19.1
08:16:31.64 +33:44:21.1
08:18:45.92 +34:48:25.0
08:21:46.63 +33:51:39.4
08:16:10.15 +35:10:07.7
08:21:23.89 +33:54:48.4
08:22:39.87 +33:29:34.4
08:18:06.10 +34:12:14.5
08:16:59.34 +33:10:55.3
08:20:06.47 +35:04:28.8
08:17:02.21 +34:14:27.8
08:20:14.67 +34:20:43.2
08:13:35.32 +33:04:21.2
08:16:24.88 +34:15:07.9
08:17:21.26 +33:50:18.5
08:18:43.98 +35:43:47.2
08:17:37.84 +33:11:01.6
08:22:47.16 +33:07:47.0
08:19:34.60 +34:24:03.6
08:17:11.07 +33:34:33.6
08:11:14.93 +33:20:34.8
08:17:25.57 +34:20:49.9
08:20:17.88 +34:56:26.7
08:21:17.38 +34:00:03.0
08:18:19.87 +33:24:04.3
08:20:17.85 +34:40:13.1
08:20:27.84 +34:31:34.7
08:22:38.90 +33:07:28.3
08:19:20.27 +34:29:34.7
08:20:31.97 +35:18:38.1
08:17:15.68 +34:52:54.1
08:20:31.24 +33:38:06.6
08:16:16.96 +35:09:56.3
08:16:46.47 +33:24:58.2
08:15:25.78 +34:36:10.6
08:21:01.98 +33:40:55.4
08:19:46.62 +33:37:59.6
08:18:06.93 +33:36:21.3
08:16:43.93 +33:43:11.7
08:20:20.12 +33:33:00.8
08:19:29.24 +34:36:32.3
08:18:40.33 +33:29:22.3
08:17:14.01 +33:49:19.7
08:21:10.19 +33:26:44.4
###################################################################################
08:16:27.40 +34:05:41.0 -- not an asteroid (will add it to exclusion list)
08:17:27.79 +34:37:59.7 -- not an asteroid (will add it to exclusion list)
08:18:33.85 +33:44:02.0 -- not an asteroid (will add it to exclusion list)
08:22:36.91 +33:02:32.4 -- not an asteroid (will add it to exclusion list)
08:17:23.35 +35:10:26.2 -- not an asteroid (will add it to exclusion list)
08:19:32.52 +34:31:14.7 -- not an asteroid (will add it to exclusion list)
08:14:36.92 +34:20:36.7 -- not an asteroid (will add it to exclusion list)
08:18:12.71 +34:08:55.0 -- not an asteroid (will add it to exclusion list)
08:15:50.19 +35:03:52.1 -- not an asteroid (will add it to exclusion list)
08:19:22.24 +33:50:04.1 -- not an asteroid (will add it to exclusion list)
08:11:25.07 +33:41:01.7 -- not an asteroid (will add it to exclusion list)
08:21:22.94 +33:26:34.3 -- not an asteroid (will add it to exclusion list)
08:16:44.61 +35:52:49.6 -- not an asteroid (will add it to exclusion list)
08:18:32.50 +35:55:57.6 -- not an asteroid (will add it to exclusion list)
08:16:42.55 +33:45:17.1 -- not an asteroid (will add it to exclusion list)
08:19:13.23 +33:35:55.7 -- not an asteroid (will add it to exclusion list)
08:17:37.34 +33:04:14.1 -- not an asteroid (will add it to exclusion list)
08:16:20.96 +35:39:32.8 -- not an asteroid (will add it to exclusion list)
08:16:57.77 +34:38:56.8 -- not an asteroid (will add it to exclusion list)
08:17:39.32 +35:34:25.0 -- not an asteroid (will add it to exclusion list)
08:20:36.95 +33:04:22.5 -- not an asteroid (will add it to exclusion list)
08:19:08.06 +35:08:53.8 -- not an asteroid (will add it to exclusion list)
08:21:18.17 +33:33:26.0 -- not an asteroid (will add it to exclusion list)
08:19:47.60 +34:32:38.3 -- not an asteroid (will add it to exclusion list)
08:17:41.84 +34:14:27.8 -- not an asteroid (will add it to exclusion list)
08:22:04.76 +34:00:12.0 -- not an asteroid (will add it to exclusion list)
08:18:58.87 +34:27:14.1 -- not an asteroid (will add it to exclusion list)
08:11:31.03 +33:16:36.4 -- not an asteroid (will add it to exclusion list)
08:19:42.25 +33:12:27.5 -- not an asteroid (will add it to exclusion list)
08:16:31.47 +34:02:21.4 -- not an asteroid (will add it to exclusion list)
08:20:13.36 +33:39:38.5 -- not an asteroid (will add it to exclusion list)
08:19:18.44 +34:09:08.9 -- not an asteroid (will add it to exclusion list)
08:20:06.98 +33:43:04.4 -- not an asteroid (will add it to exclusion list)
08:15:55.13 +33:37:41.3 -- not an asteroid (will add it to exclusion list)
08:17:38.37 +33:06:38.0 -- not an asteroid (will add it to exclusion list)
08:14:54.07 +33:39:39.7 -- not an asteroid (will add it to exclusion list)
08:19:23.10 +33:34:48.7 -- not an asteroid (will add it to exclusion list)
08:18:27.49 +33:44:42.5 -- not an asteroid (will add it to exclusion list)
08:20:01.09 +34:01:21.9 -- not an asteroid (will add it to exclusion list)
08:21:01.24 +33:17:46.3 -- not an asteroid (will add it to exclusion list)
08:18:45.96 +33:52:55.7 -- not an asteroid (will add it to exclusion list)
08:19:27.22 +34:22:04.1 -- not an asteroid (will add it to exclusion list)
08:15:06.32 +33:26:21.0 -- not an asteroid (will add it to exclusion list)
08:20:22.14 +34:03:18.9 -- not an asteroid (will add it to exclusion list)
08:18:59.76 +34:54:19.4 -- not an asteroid (will add it to exclusion list)
08:19:58.41 +34:39:43.8 -- not an asteroid (will add it to exclusion list)
08:20:33.25 +33:40:26.4 -- not an asteroid (will add it to exclusion list)
08:21:07.53 +33:24:45.2 -- not an asteroid (will add it to exclusion list)
08:21:24.58 +33:59:45.1 -- not an asteroid (will add it to exclusion list)
08:16:46.13 +34:52:08.9 -- not an asteroid (will add it to exclusion list)
08:17:05.24 +34:04:17.3 -- not an asteroid (will add it to exclusion list)
08:17:37.24 +34:42:01.7 -- not an asteroid (will add it to exclusion list)
08:09:51.75 +33:35:16.1 -- not an asteroid (will add it to exclusion list)
08:22:50.48 +33:37:46.5 -- not an asteroid (will add it to exclusion list)
08:16:04.15 +34:02:55.4 -- not an asteroid (will add it to exclusion list)
08:17:21.40 +33:21:25.9 -- not an asteroid (will add it to exclusion list)
08:17:05.59 +35:17:16.2 -- not an asteroid (will add it to exclusion list)
08:21:21.02 +33:55:58.9 -- not an asteroid (will add it to exclusion list)
08:19:10.89 +33:54:45.2 -- not an asteroid (will add it to exclusion list)
08:20:38.43 +33:09:17.4 -- not an asteroid (will add it to exclusion list)
08:17:35.81 +34:53:43.5 -- not an asteroid (will add it to exclusion list)
08:22:49.96 +33:40:00.0 -- not an asteroid (will add it to exclusion list)
08:21:14.01 +33:58:17.5 -- not an asteroid (will add it to exclusion list)
08:11:52.34 +33:13:19.8 -- not an asteroid (will add it to exclusion list)
08:21:33.20 +33:18:56.1 -- not an asteroid (will add it to exclusion list)
08:21:21.26 +33:05:50.3 -- not an asteroid (will add it to exclusion list)
08:15:42.59 +34:39:17.7 -- not an asteroid (will add it to exclusion list)
08:16:50.59 +34:42:52.7 -- not an asteroid (will add it to exclusion list)
08:16:29.95 +34:47:10.1 -- not an asteroid (will add it to exclusion list)
08:18:23.98 +34:40:39.3 -- not an asteroid (will add it to exclusion list)
08:18:05.08 +35:07:52.6 -- not an asteroid (will add it to exclusion list)
08:15:53.80 +33:32:50.9 -- not an asteroid (will add it to exclusion list)
08:18:54.90 +33:05:01.6 -- not an asteroid (will add it to exclusion list)
08:17:32.05 +34:49:32.2 -- not an asteroid (will add it to exclusion list)
08:19:33.25 +33:54:06.1 -- not an asteroid (will add it to exclusion list)
08:19:15.89 +33:45:34.7 -- not an asteroid (will add it to exclusion list)
08:20:56.69 +34:02:46.7 -- not an asteroid (will add it to exclusion list)
08:19:20.41 +33:28:24.5 -- not an asteroid (will add it to exclusion list)
08:21:07.85 +33:14:32.9 -- not an asteroid (will add it to exclusion list)
08:19:40.26 +33:09:22.2 -- not an asteroid (will add it to exclusion list)
08:18:25.97 +33:34:41.7 -- not an asteroid (will add it to exclusion list)
08:18:33.53 +34:43:18.5 -- not an asteroid (will add it to exclusion list)
08:16:12.75 +33:20:26.0 -- not an asteroid (will add it to exclusion list)
08:17:24.84 +34:35:28.7 -- not an asteroid (will add it to exclusion list)
08:21:56.55 +35:43:30.2 -- not an asteroid (will add it to exclusion list)
08:20:49.59 +33:31:29.0 -- not an asteroid (will add it to exclusion list)
08:16:54.89 +35:24:04.2 -- not an asteroid (will add it to exclusion list)
08:19:56.18 +33:38:58.7 -- not an asteroid (will add it to exclusion list)
08:20:03.60 +34:50:11.8 -- not an asteroid (will add it to exclusion list)
08:16:55.68 +34:31:58.5 -- not an asteroid (will add it to exclusion list)
08:17:30.67 +33:35:21.2 -- not an asteroid (will add it to exclusion list)
08:20:23.35 +33:19:47.7 -- not an asteroid (will add it to exclusion list)
08:21:33.96 +33:50:36.0 -- not an asteroid (will add it to exclusion list)
08:18:07.56 +33:41:57.3 -- not an asteroid (will add it to exclusion list)
08:16:56.15 +33:57:55.9 -- not an asteroid (will add it to exclusion list)
08:19:26.35 +35:04:03.5 -- not an asteroid (will add it to exclusion list)
08:23:15.88 +33:41:01.1 -- not an asteroid (will add it to exclusion list)
08:15:58.79 +34:42:40.0 -- not an asteroid (will add it to exclusion list)
08:17:37.33 +33:24:43.7 -- not an asteroid (will add it to exclusion list)
08:22:46.63 +33:23:16.0 -- not an asteroid (will add it to exclusion list)
08:20:04.70 +33:11:41.8 -- not an asteroid (will add it to exclusion list)
08:22:39.97 +33:17:20.7 -- not an asteroid (will add it to exclusion list)
08:18:28.90 +34:48:24.7 -- not an asteroid (will add it to exclusion list)
08:15:39.78 +33:25:13.3 -- not an asteroid (will add it to exclusion list)
08:14:35.28 +36:06:32.0 -- not an asteroid (will add it to exclusion list)
08:22:56.71 +33:35:58.3 -- not an asteroid (will add it to exclusion list)
08:16:44.74 +35:07:35.4 -- not an asteroid (will add it to exclusion list)
08:18:13.59 +33:56:11.9 -- not an asteroid (will add it to exclusion list)
08:17:31.70 +34:51:09.2 -- not an asteroid (will add it to exclusion list)
08:19:37.23 +34:02:00.7 -- not an asteroid (will add it to exclusion list)
08:20:46.03 +33:46:45.5 -- not an asteroid (will add it to exclusion list)
08:22:03.28 +33:34:56.4 -- not an asteroid (will add it to exclusion list)
08:17:46.18 +34:37:24.5 -- not an asteroid (will add it to exclusion list)
08:16:13.40 +33:35:02.0 -- not an asteroid (will add it to exclusion list)
08:18:22.00 +33:13:13.6 -- not an asteroid (will add it to exclusion list)
08:19:48.49 +33:08:59.6 -- not an asteroid (will add it to exclusion list)
08:14:08.36 +34:05:45.0 -- not an asteroid (will add it to exclusion list)
08:19:58.90 +34:41:10.8 -- not an asteroid (will add it to exclusion list)
08:19:33.24 +34:53:17.9 -- not an asteroid (will add it to exclusion list)
08:16:30.97 +34:23:20.3 -- not an asteroid (will add it to exclusion list)
08:22:07.37 +33:17:26.4 -- not an asteroid (will add it to exclusion list)
08:19:15.88 +35:03:30.5 -- not an asteroid (will add it to exclusion list)
08:17:34.21 +34:20:20.8 -- not an asteroid (will add it to exclusion list)
08:19:25.79 +34:07:48.8 -- not an asteroid (will add it to exclusion list)
08:18:10.53 +35:04:01.3 -- not an asteroid (will add it to exclusion list)
08:17:16.28 +33:49:01.3 -- not an asteroid (will add it to exclusion list)
08:19:50.53 +35:08:00.8 -- not an asteroid (will add it to exclusion list)
08:14:59.88 +33:17:48.6 -- not an asteroid (will add it to exclusion list)
08:17:13.16 +33:16:24.4 -- not an asteroid (will add it to exclusion list)
08:18:43.34 +34:30:00.5 -- not an asteroid (will add it to exclusion list)
08:20:42.49 +34:41:27.4 -- not an asteroid (will add it to exclusion list)
08:20:11.83 +33:13:08.0 -- not an asteroid (will add it to exclusion list)
08:21:57.10 +33:13:05.0 -- not an asteroid (will add it to exclusion list)
08:16:09.78 +34:20:29.7 -- not an asteroid (will add it to exclusion list)
08:16:55.75 +34:08:28.9 -- not an asteroid (will add it to exclusion list)
08:16:09.31 +34:38:31.4 -- not an asteroid (will add it to exclusion list)
08:20:48.80 +34:20:32.1 -- not an asteroid (will add it to exclusion list)
08:14:57.20 +34:26:19.4 -- not an asteroid (will add it to exclusion list)
08:21:26.83 +33:29:51.6 -- not an asteroid (will add it to exclusion list)
08:20:36.67 +33:44:46.2 -- not an asteroid (will add it to exclusion list)
08:17:35.66 +34:15:50.1 -- not an asteroid (will add it to exclusion list)
08:18:12.84 +35:05:10.2 -- not an asteroid (will add it to exclusion list)
08:17:44.72 +34:39:39.5 -- not an asteroid (will add it to exclusion list)
08:16:41.73 +34:49:32.9 -- not an asteroid (will add it to exclusion list)
08:18:12.95 +33:06:10.2 -- not an asteroid (will add it to exclusion list)
08:15:31.11 +34:45:00.1 -- not an asteroid (will add it to exclusion list)
08:13:43.13 +34:09:03.7 -- not an asteroid (will add it to exclusion list)
08:18:27.64 +34:13:48.5 -- not an asteroid (will add it to exclusion list)
08:16:42.66 +34:31:55.4 -- not an asteroid (will add it to exclusion list)
08:16:30.82 +34:16:36.7 -- not an asteroid (will add it to exclusion list)
08:17:43.08 +33:21:54.1 -- not an asteroid (will add it to exclusion list)
08:18:44.02 +33:40:15.1 -- not an asteroid (will add it to exclusion list)
08:20:05.63 +33:22:44.6 -- not an asteroid (will add it to exclusion list)
08:17:26.85 +34:49:31.0 -- not an asteroid (will add it to exclusion list)
08:18:14.60 +33:41:02.8 -- not an asteroid (will add it to exclusion list)
08:22:01.57 +33:09:19.1 -- not an asteroid (will add it to exclusion list)
08:16:31.64 +33:44:21.1 -- not an asteroid (will add it to exclusion list)
08:18:45.92 +34:48:25.0 -- not an asteroid (will add it to exclusion list)
08:21:46.63 +33:51:39.4 -- not an asteroid (will add it to exclusion list)
08:16:10.15 +35:10:07.7 -- not an asteroid (will add it to exclusion list)
08:21:23.89 +33:54:48.4 -- not an asteroid (will add it to exclusion list)
08:22:39.87 +33:29:34.4 -- not an asteroid (will add it to exclusion list)
08:18:06.10 +34:12:14.5 -- not an asteroid (will add it to exclusion list)
08:16:59.34 +33:10:55.3 -- not an asteroid (will add it to exclusion list)
08:20:06.47 +35:04:28.8 -- not an asteroid (will add it to exclusion list)
08:17:02.21 +34:14:27.8 -- not an asteroid (will add it to exclusion list)
08:20:14.67 +34:20:43.2 -- not an asteroid (will add it to exclusion list)
08:13:35.32 +33:04:21.2 -- not an asteroid (will add it to exclusion list)
08:16:24.88 +34:15:07.9 -- not an asteroid (will add it to exclusion list)
08:17:21.26 +33:50:18.5 -- not an asteroid (will add it to exclusion list)
08:18:43.98 +35:43:47.2 -- not an asteroid (will add it to exclusion list)
08:17:37.84 +33:11:01.6 -- not an asteroid (will add it to exclusion list)
08:22:47.16 +33:07:47.0 -- not an asteroid (will add it to exclusion list)
08:19:34.60 +34:24:03.6 -- not an asteroid (will add it to exclusion list)
08:17:11.07 +33:34:33.6 -- not an asteroid (will add it to exclusion list)
08:11:14.93 +33:20:34.8 -- not an asteroid (will add it to exclusion list)
08:17:25.57 +34:20:49.9 -- not an asteroid (will add it to exclusion list)
08:20:17.88 +34:56:26.7 -- not an asteroid (will add it to exclusion list)
08:21:17.38 +34:00:03.0 -- not an asteroid (will add it to exclusion list)
08:18:19.87 +33:24:04.3 -- not an asteroid (will add it to exclusion list)
08:20:17.85 +34:40:13.1 -- not an asteroid (will add it to exclusion list)
08:20:27.84 +34:31:34.7 -- not an asteroid (will add it to exclusion list)
08:22:38.90 +33:07:28.3 -- not an asteroid (will add it to exclusion list)
08:19:20.27 +34:29:34.7 -- not an asteroid (will add it to exclusion list)
08:20:31.97 +35:18:38.1 -- not an asteroid (will add it to exclusion list)
08:17:15.68 +34:52:54.1 -- not an asteroid (will add it to exclusion list)
08:20:31.24 +33:38:06.6 -- not an asteroid (will add it to exclusion list)
08:16:16.96 +35:09:56.3 -- not an asteroid (will add it to exclusion list)
08:16:46.47 +33:24:58.2 -- not an asteroid (will add it to exclusion list)
08:15:25.78 +34:36:10.6 -- not an asteroid (will add it to exclusion list)
08:21:01.98 +33:40:55.4 -- not an asteroid (will add it to exclusion list)
08:19:46.62 +33:37:59.6 -- not an asteroid (will add it to exclusion list)
08:18:06.93 +33:36:21.3 -- not an asteroid (will add it to exclusion list)
08:16:43.93 +33:43:11.7 -- not an asteroid (will add it to exclusion list)
08:20:20.12 +33:33:00.8 -- not an asteroid (will add it to exclusion list)
08:19:29.24 +34:36:32.3 -- not an asteroid (will add it to exclusion list)
08:18:40.33 +33:29:22.3 -- not an asteroid (will add it to exclusion list)
08:17:14.01 +33:49:19.7 -- not an asteroid (will add it to exclusion list)
08:21:10.19 +33:26:44.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
08:09:51.75 +33:35:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:14.93 +33:20:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:25.07 +33:41:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:31.03 +33:16:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:11:52.34 +33:13:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:35.32 +33:04:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:13:43.13 +34:09:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:08.36 +34:05:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:35.28 +36:06:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:36.92 +34:20:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:54.07 +33:39:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:57.20 +34:26:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:59.88 +33:17:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:06.32 +33:26:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:25.78 +34:36:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:31.11 +34:45:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:39.78 +33:25:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:42.59 +34:39:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:50.19 +35:03:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:53.80 +33:32:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:55.13 +33:37:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:15:58.79 +34:42:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:04.15 +34:02:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:09.31 +34:38:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:09.78 +34:20:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:10.15 +35:10:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:12.75 +33:20:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:13.40 +33:35:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:16.96 +35:09:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:20.96 +35:39:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:24.88 +34:15:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:27.40 +34:05:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:29.95 +34:47:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:30.82 +34:16:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:30.97 +34:23:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:31.47 +34:02:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:31.64 +33:44:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:41.73 +34:49:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:42.55 +33:45:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:42.66 +34:31:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:43.93 +33:43:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:44.61 +35:52:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:44.74 +35:07:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:46.13 +34:52:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:46.47 +33:24:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:50.59 +34:42:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:54.89 +35:24:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:55.68 +34:31:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:55.75 +34:08:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:56.15 +33:57:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:57.77 +34:38:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:59.34 +33:10:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:02.21 +34:14:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:05.24 +34:04:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:05.59 +35:17:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:11.07 +33:34:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:13.16 +33:16:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:14.01 +33:49:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:15.68 +34:52:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:16.28 +33:49:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:21.26 +33:50:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:21.40 +33:21:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:23.35 +35:10:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:24.84 +34:35:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:25.57 +34:20:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:26.85 +34:49:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:27.79 +34:37:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:30.67 +33:35:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:31.70 +34:51:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:32.05 +34:49:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:34.21 +34:20:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:35.66 +34:15:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:35.81 +34:53:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:37.24 +34:42:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:37.33 +33:24:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:37.34 +33:04:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:37.84 +33:11:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:38.37 +33:06:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:39.32 +35:34:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:41.84 +34:14:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:43.08 +33:21:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:44.72 +34:39:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:46.18 +34:37:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:05.08 +35:07:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:06.10 +34:12:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:06.93 +33:36:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:07.56 +33:41:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:10.53 +35:04:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:12.71 +34:08:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:12.84 +35:05:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:12.95 +33:06:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:13.59 +33:56:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:14.60 +33:41:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:19.87 +33:24:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:22.00 +33:13:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:23.98 +34:40:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:25.97 +33:34:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:27.49 +33:44:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:27.64 +34:13:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:28.90 +34:48:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:32.50 +35:55:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:33.53 +34:43:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:33.85 +33:44:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:40.33 +33:29:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:43.34 +34:30:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:43.98 +35:43:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:44.02 +33:40:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:45.92 +34:48:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:45.96 +33:52:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:54.90 +33:05:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:58.87 +34:27:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:59.76 +34:54:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:08.06 +35:08:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:10.89 +33:54:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:13.23 +33:35:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:15.88 +35:03:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:15.89 +33:45:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:18.44 +34:09:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:20.27 +34:29:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:20.41 +33:28:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:22.24 +33:50:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:23.10 +33:34:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:25.79 +34:07:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:26.35 +35:04:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:27.22 +34:22:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:29.24 +34:36:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:32.52 +34:31:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:33.24 +34:53:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:33.25 +33:54:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:34.60 +34:24:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:37.23 +34:02:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:40.26 +33:09:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:42.25 +33:12:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:46.62 +33:37:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:47.60 +34:32:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:48.49 +33:08:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:50.53 +35:08:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:56.18 +33:38:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:58.41 +34:39:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:58.90 +34:41:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:01.09 +34:01:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:03.60 +34:50:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:04.70 +33:11:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:05.63 +33:22:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:06.47 +35:04:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:06.98 +33:43:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:11.83 +33:13:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:13.36 +33:39:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:14.67 +34:20:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:17.85 +34:40:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:17.88 +34:56:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:20.12 +33:33:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:22.14 +34:03:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:23.35 +33:19:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:27.84 +34:31:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:31.24 +33:38:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:31.97 +35:18:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:33.25 +33:40:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:36.67 +33:44:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:36.95 +33:04:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:38.43 +33:09:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:42.49 +34:41:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:46.03 +33:46:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:48.80 +34:20:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:49.59 +33:31:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:56.69 +34:02:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:01.24 +33:17:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:01.98 +33:40:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:07.53 +33:24:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:07.85 +33:14:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:10.19 +33:26:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:14.01 +33:58:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:17.38 +34:00:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:18.17 +33:33:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:21.02 +33:55:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:21.26 +33:05:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:22.94 +33:26:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:23.89 +33:54:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:24.58 +33:59:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:26.83 +33:29:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:33.20 +33:18:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:33.96 +33:50:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:46.63 +33:51:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:56.55 +35:43:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:57.10 +33:13:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:01.57 +33:09:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:03.28 +33:34:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:04.76 +34:00:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:07.37 +33:17:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:36.91 +33:02:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:38.90 +33:07:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:39.87 +33:29:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:39.97 +33:17:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:46.63 +33:23:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:47.16 +33:07:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:49.96 +33:40:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:50.48 +33:37:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:56.71 +33:35:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:15.88 +33:41:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
08:09:51.75 +33:35:16.1 -- not a known variable star
08:11:14.93 +33:20:34.8 -- not a known variable star
08:11:25.07 +33:41:01.7 -- not a known variable star
08:11:31.03 +33:16:36.4 -- not a known variable star
08:11:52.34 +33:13:19.8 -- not a known variable star
08:13:35.32 +33:04:21.2 -- not a known variable star
08:13:43.13 +34:09:03.7 -- not a known variable star
08:14:08.36 +34:05:45.0 -- not a known variable star
08:14:35.28 +36:06:32.0 -- not a known variable star
08:14:36.92 +34:20:36.7 -- not a known variable star
08:14:54.07 +33:39:39.7 -- a known variable star
08:14:57.20 +34:26:19.4 -- not a known variable star
08:14:59.88 +33:17:48.6 -- not a known variable star
08:15:06.32 +33:26:21.0 -- not a known variable star
08:15:25.78 +34:36:10.6 -- not a known variable star
08:15:31.11 +34:45:00.1 -- not a known variable star
08:15:39.78 +33:25:13.3 -- not a known variable star
08:15:42.59 +34:39:17.7 -- not a known variable star
08:15:50.19 +35:03:52.1 -- not a known variable star
08:15:53.80 +33:32:50.9 -- not a known variable star
08:15:55.13 +33:37:41.3 -- not a known variable star
08:15:58.79 +34:42:40.0 -- not a known variable star
08:16:04.15 +34:02:55.4 -- not a known variable star
08:16:09.31 +34:38:31.4 -- not a known variable star
08:16:09.78 +34:20:29.7 -- not a known variable star
08:16:10.15 +35:10:07.7 -- not a known variable star
08:16:12.75 +33:20:26.0 -- not a known variable star
08:16:13.40 +33:35:02.0 -- not a known variable star
08:16:16.96 +35:09:56.3 -- not a known variable star
08:16:20.96 +35:39:32.8 -- not a known variable star
08:16:24.88 +34:15:07.9 -- not a known variable star
08:16:27.40 +34:05:41.0 -- not a known variable star
08:16:29.95 +34:47:10.1 -- not a known variable star
08:16:30.82 +34:16:36.7 -- not a known variable star
08:16:30.97 +34:23:20.3 -- not a known variable star
08:16:31.47 +34:02:21.4 -- not a known variable star
08:16:31.64 +33:44:21.1 -- not a known variable star
08:16:41.73 +34:49:32.9 -- not a known variable star
08:16:42.55 +33:45:17.1 -- not a known variable star
08:16:42.66 +34:31:55.4 -- not a known variable star
08:16:43.93 +33:43:11.7 -- a known variable star
08:16:44.61 +35:52:49.6 -- not a known variable star
08:16:44.74 +35:07:35.4 -- a known variable star
08:16:46.13 +34:52:08.9 -- not a known variable star
08:16:46.47 +33:24:58.2 -- a known variable star
08:16:50.59 +34:42:52.7 -- not a known variable star
08:16:54.89 +35:24:04.2 -- not a known variable star
08:16:55.68 +34:31:58.5 -- not a known variable star
08:16:55.75 +34:08:28.9 -- not a known variable star
08:16:56.15 +33:57:55.9 -- not a known variable star
08:16:57.77 +34:38:56.8 -- not a known variable star
08:16:59.34 +33:10:55.3 -- not a known variable star
08:17:02.21 +34:14:27.8 -- not a known variable star
08:17:05.24 +34:04:17.3 -- not a known variable star
08:17:05.59 +35:17:16.2 -- not a known variable star
08:17:11.07 +33:34:33.6 -- not a known variable star
08:17:13.16 +33:16:24.4 -- not a known variable star
08:17:14.01 +33:49:19.7 -- not a known variable star
08:17:15.68 +34:52:54.1 -- not a known variable star
08:17:16.28 +33:49:01.3 -- not a known variable star
08:17:21.26 +33:50:18.5 -- not a known variable star
08:17:21.40 +33:21:25.9 -- not a known variable star
08:17:23.35 +35:10:26.2 -- not a known variable star
08:17:24.84 +34:35:28.7 -- not a known variable star
08:17:25.57 +34:20:49.9 -- not a known variable star
08:17:26.85 +34:49:31.0 -- not a known variable star
08:17:27.79 +34:37:59.7 -- not a known variable star
08:17:30.67 +33:35:21.2 -- not a known variable star
08:17:31.70 +34:51:09.2 -- not a known variable star
08:17:32.05 +34:49:32.2 -- not a known variable star
08:17:34.21 +34:20:20.8 -- not a known variable star
08:17:35.66 +34:15:50.1 -- not a known variable star
08:17:35.81 +34:53:43.5 -- not a known variable star
08:17:37.24 +34:42:01.7 -- not a known variable star
08:17:37.33 +33:24:43.7 -- not a known variable star
08:17:37.34 +33:04:14.1 -- not a known variable star
08:17:37.84 +33:11:01.6 -- not a known variable star
08:17:38.37 +33:06:38.0 -- not a known variable star
08:17:39.32 +35:34:25.0 -- not a known variable star
08:17:41.84 +34:14:27.8 -- not a known variable star
08:17:43.08 +33:21:54.1 -- not a known variable star
08:17:44.72 +34:39:39.5 -- not a known variable star
08:17:46.18 +34:37:24.5 -- not a known variable star
08:18:05.08 +35:07:52.6 -- not a known variable star
08:18:06.10 +34:12:14.5 -- not a known variable star
08:18:06.93 +33:36:21.3 -- not a known variable star
08:18:07.56 +33:41:57.3 -- not a known variable star
08:18:10.53 +35:04:01.3 -- not a known variable star
08:18:12.71 +34:08:55.0 -- not a known variable star
08:18:12.84 +35:05:10.2 -- not a known variable star
08:18:12.95 +33:06:10.2 -- not a known variable star
08:18:13.59 +33:56:11.9 -- not a known variable star
08:18:14.60 +33:41:02.8 -- not a known variable star
08:18:19.87 +33:24:04.3 -- not a known variable star
08:18:22.00 +33:13:13.6 -- not a known variable star
08:18:23.98 +34:40:39.3 -- not a known variable star
08:18:25.97 +33:34:41.7 -- not a known variable star
08:18:27.49 +33:44:42.5 -- not a known variable star
08:18:27.64 +34:13:48.5 -- not a known variable star
08:18:28.90 +34:48:24.7 -- not a known variable star
08:18:32.50 +35:55:57.6 -- a known variable star
08:18:33.53 +34:43:18.5 -- not a known variable star
08:18:33.85 +33:44:02.0 -- not a known variable star
08:18:40.33 +33:29:22.3 -- not a known variable star
08:18:43.34 +34:30:00.5 -- not a known variable star
08:18:43.98 +35:43:47.2 -- not a known variable star
08:18:44.02 +33:40:15.1 -- not a known variable star
08:18:45.92 +34:48:25.0 -- not a known variable star
08:18:45.96 +33:52:55.7 -- not a known variable star
08:18:54.90 +33:05:01.6 -- not a known variable star
08:18:58.87 +34:27:14.1 -- not a known variable star
08:18:59.76 +34:54:19.4 -- not a known variable star
08:19:08.06 +35:08:53.8 -- a known variable star
08:19:10.89 +33:54:45.2 -- not a known variable star
08:19:13.23 +33:35:55.7 -- a known variable star
08:19:15.88 +35:03:30.5 -- not a known variable star
08:19:15.89 +33:45:34.7 -- not a known variable star
08:19:18.44 +34:09:08.9 -- not a known variable star
08:19:20.27 +34:29:34.7 -- not a known variable star
08:19:20.41 +33:28:24.5 -- not a known variable star
08:19:22.24 +33:50:04.1 -- not a known variable star
08:19:23.10 +33:34:48.7 -- not a known variable star
08:19:25.79 +34:07:48.8 -- not a known variable star
08:19:26.35 +35:04:03.5 -- not a known variable star
08:19:27.22 +34:22:04.1 -- not a known variable star
08:19:29.24 +34:36:32.3 -- not a known variable star
08:19:32.52 +34:31:14.7 -- not a known variable star
08:19:33.24 +34:53:17.9 -- not a known variable star
08:19:33.25 +33:54:06.1 -- not a known variable star
08:19:34.60 +34:24:03.6 -- not a known variable star
08:19:37.23 +34:02:00.7 -- not a known variable star
08:19:40.26 +33:09:22.2 -- not a known variable star
08:19:42.25 +33:12:27.5 -- not a known variable star
08:19:46.62 +33:37:59.6 -- not a known variable star
08:19:47.60 +34:32:38.3 -- not a known variable star
08:19:48.49 +33:08:59.6 -- not a known variable star
08:19:50.53 +35:08:00.8 -- not a known variable star
08:19:56.18 +33:38:58.7 -- not a known variable star
08:19:58.41 +34:39:43.8 -- not a known variable star
08:19:58.90 +34:41:10.8 -- not a known variable star
08:20:01.09 +34:01:21.9 -- not a known variable star
08:20:03.60 +34:50:11.8 -- not a known variable star
08:20:04.70 +33:11:41.8 -- a known variable star
08:20:05.63 +33:22:44.6 -- not a known variable star
08:20:06.47 +35:04:28.8 -- not a known variable star
08:20:06.98 +33:43:04.4 -- a known variable star
08:20:11.83 +33:13:08.0 -- not a known variable star
08:20:13.36 +33:39:38.5 -- not a known variable star
08:20:14.67 +34:20:43.2 -- not a known variable star
08:20:17.85 +34:40:13.1 -- a known variable star
08:20:17.88 +34:56:26.7 -- not a known variable star
08:20:20.12 +33:33:00.8 -- not a known variable star
08:20:22.14 +34:03:18.9 -- not a known variable star
08:20:23.35 +33:19:47.7 -- not a known variable star
08:20:27.84 +34:31:34.7 -- not a known variable star
08:20:31.24 +33:38:06.6 -- not a known variable star
08:20:31.97 +35:18:38.1 -- a known variable star
08:20:33.25 +33:40:26.4 -- not a known variable star
08:20:36.67 +33:44:46.2 -- not a known variable star
08:20:36.95 +33:04:22.5 -- not a known variable star
08:20:38.43 +33:09:17.4 -- not a known variable star
08:20:42.49 +34:41:27.4 -- not a known variable star
08:20:46.03 +33:46:45.5 -- not a known variable star
08:20:48.80 +34:20:32.1 -- not a known variable star
08:20:49.59 +33:31:29.0 -- not a known variable star
08:20:56.69 +34:02:46.7 -- not a known variable star
08:21:01.24 +33:17:46.3 -- not a known variable star
08:21:01.98 +33:40:55.4 -- not a known variable star
08:21:07.53 +33:24:45.2 -- not a known variable star
08:21:07.85 +33:14:32.9 -- not a known variable star
08:21:10.19 +33:26:44.4 -- not a known variable star
08:21:14.01 +33:58:17.5 -- not a known variable star
08:21:17.38 +34:00:03.0 -- a known variable star
08:21:18.17 +33:33:26.0 -- not a known variable star
08:21:21.02 +33:55:58.9 -- not a known variable star
08:21:21.26 +33:05:50.3 -- not a known variable star
08:21:22.94 +33:26:34.3 -- not a known variable star
08:21:23.89 +33:54:48.4 -- not a known variable star
08:21:24.58 +33:59:45.1 -- not a known variable star
08:21:26.83 +33:29:51.6 -- not a known variable star
08:21:33.20 +33:18:56.1 -- not a known variable star
08:21:33.96 +33:50:36.0 -- not a known variable star
08:21:46.63 +33:51:39.4 -- not a known variable star
08:21:56.55 +35:43:30.2 -- not a known variable star
08:21:57.10 +33:13:05.0 -- not a known variable star
08:22:01.57 +33:09:19.1 -- not a known variable star
08:22:03.28 +33:34:56.4 -- a known variable star
08:22:04.76 +34:00:12.0 -- not a known variable star
08:22:07.37 +33:17:26.4 -- not a known variable star
08:22:36.91 +33:02:32.4 -- not a known variable star
08:22:38.90 +33:07:28.3 -- a known variable star
08:22:39.87 +33:29:34.4 -- not a known variable star
08:22:39.97 +33:17:20.7 -- not a known variable star
08:22:46.63 +33:23:16.0 -- not a known variable star
08:22:47.16 +33:07:47.0 -- not a known variable star
08:22:49.96 +33:40:00.0 -- not a known variable star
08:22:50.48 +33:37:46.5 -- a known variable star
08:22:56.71 +33:35:58.3 -- not a known variable star
08:23:15.88 +33:41:01.1 -- not a known variable star
Found 184 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
199 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 199 (excluding asteroids and hot pixels, 184 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)2461199.64916384 -observatory V36
06:43:28.70 +25:00:33.2 Mercury (0.1mag)
07:42:38.29 +23:23:16.6 Venus (-4.0mag)
02:49:29.05 +15:42:15.9 Mars (1.3mag)
07:48:24.11 +21:31:32.6 Jupiter (-1.9mag)
00:49:21.71 +02:48:36.9 Saturn (0.9mag)
04:00:11.80 +20:25:26.1 Uranus (5.8mag)
00:16:08.38 +00:16:47.5 Neptune (7.8mag)
20:33:21.54 -23:04:31.8 Pluto (14.5mag)
23:00:52.43 -05:53:51.3 Moon (-10.4mag)
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Positions of selected moons from JPL HORIZONS for JD(UT)2461199.64916384:
07:48:24.16 +21:31:34.6 Io (6.0mag)
07:48:23.66 +21:31:36.1 Europa (6.2mag)
07:48:08.25 +21:32:19.7 Ganymede (5.6mag)
07:48:43.09 +21:30:31.5 Callisto (6.7mag)
07:48:41.62 +21:07:50.1 Himalia (15.6mag)
07:48:28.45 +21:31:19.4 Thebe (16.5mag)
07:48:41.13 +21:23:17.7 Elara (17.5mag)
07:50:34.67 +21:43:15.9 Pasiphae (17.7mag)
07:54:59.31 +21:33:14.8 Carme (18.9mag)
00:49:12.20 +02:48:36.1 Titan (8.7mag)
00:49:18.81 +02:48:50.3 Rhea (9.9mag)
00:49:54.01 +02:50:46.0 Iapetus (11.3mag)
00:49:17.54 +02:48:14.0 Hyperion (14.7mag)
00:50:04.02 +02:50:33.8 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 7 23:36 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461199.64916384:
17:26:47.93 -35:14:01.2 JWST
14:21:19.35 +57:46:57.9 Chandra
18:24:02.66 -28:53:17.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 7 23:36 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461199.64916384 -observatory V36
18:43:32.54 -32:39:02.4 13.6mag P/2010 H2 (Vales)
05:53:25.57 -68:03:52.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:49:02.55 +31:58:02.8 17.5mag C/2017 K2 (PANSTARRS)
17:14:45.05 +15:20:58.8 17.8mag C/2021 G2 (ATLAS)
21:11:51.86 -49:30:35.9 16.9mag P/2021 N1 (ZTF)
23:12:38.61 +31:35:25.1 17.2mag C/2022 E2 (ATLAS)
05:33:59.18 +26:58:31.0 16.5mag C/2022 N2 (PANSTARRS)
09:29:41.72 +31:05:03.4 16.6mag C/2022 QE78 (ATLAS)
08:50:31.30 +03:55:47.2 17.7mag C/2022 R6 (PANSTARRS)
18:28:15.12 +21:36:05.3 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:19:23.39 -11:00:30.9 17.6mag P/2023 B1 (PANSTARRS)
22:14:26.81 +66:31:32.8 17.7mag C/2023 H5 (Lemmon)
17:46:29.99 -06:41:05.3 13.7mag C/2023 R1 (PANSTARRS)
13:18:07.34 +83:00:13.4 17.9mag C/2023 X2 (Lemmon)
07:10:21.07 +64:18:27.5 17.7mag C/2024 A1 (ATLAS)
06:47:12.11 +27:49:49.1 13.6mag C/2024 E1 (Wierzchos)
15:37:19.50 +13:31:20.8 17.4mag C/2024 G6 (ATLAS)
20:13:04.57 +31:07:18.6 14.0mag C/2024 J3 (ATLAS)
04:17:58.81 -15:57:18.1 16.0mag C/2024 T5 (ATLAS)
06:05:52.12 +34:29:58.1 17.9mag C/2025 J1 (Borisov)
11:34:55.69 +52:45:06.5 17.4mag C/2025 L1 (ATLAS)
06:44:53.20 -10:52:03.9 14.1mag C/2025 R3 (PANSTARRS)
09:24:07.48 +23:20:26.3 17.9mag C/2025 V2 (Rankin)
12:39:42.17 +04:41:28.4 17.2mag C/2025 Y1 (ATLAS)
18:12:57.59 +75:07:20.7 17.9mag C/2026 A2 (Bok)
02:00:35.12 +43:24:43.4 16.1mag C/2026 B2 (Sun-Gao)
11:11:18.21 -03:44:57.7 16.5mag A/2026 E1
20:23:34.07 -08:33:58.4 8.7mag 10P/Tempel
11:01:59.69 -00:58:02.4 16.0mag 29P/Schwassmann-Wachmann
03:11:38.99 +25:38:22.7 17.7mag 47P/Ashbrook-Jackson
08:59:52.98 +23:46:55.9 16.9mag 63P/Wild
00:26:53.26 -06:22:13.5 15.7mag 65P/Gunn
06:43:17.53 +33:25:31.9 16.9mag 76P/West-Kohoutek-Ikemura
03:09:04.23 +17:12:39.1 13.8mag 78P/Gehrels
01:20:39.55 +04:50:22.0 15.6mag 88P/Howell
04:54:29.59 +30:17:58.8 15.2mag 93P/Lovas
02:42:49.26 +27:37:07.7 17.6mag 114P/Wiseman-Skiff
06:50:26.32 +33:02:23.8 15.6mag 123P/West-Hartley
09:50:06.01 +14:39:25.3 16.5mag 124P/Mrkos
03:58:57.59 +19:14:50.8 16.4mag 128P/Shoemaker-Holt
04:33:28.35 +19:04:56.8 17.7mag 131P/Mueller
05:58:06.91 +18:40:14.4 14.6mag 141P/Machholz
06:00:45.02 +17:40:22.6 14.6mag 141P-A/Machholz
04:53:51.61 +16:10:02.9 11.6mag 141P-D/Machholz
02:57:38.72 -24:42:21.3 16.8mag 161P/Hartley-IRAS
03:41:23.80 +23:47:29.0 14.9mag 162P/SidingSpring
19:36:38.35 +01:42:57.2 16.9mag 169P/NEAT
00:18:12.75 +02:27:23.2 17.9mag 220P/McNaught
16:52:13.15 -08:28:40.8 16.4mag 235P/LINEAR
07:34:33.23 +35:29:38.0 17.5mag 240P/NEAT
00:32:13.81 -02:29:18.2 16.4mag 260P/McNaught
04:04:06.01 +32:28:22.0 17.6mag 295P/LINEAR
23:51:57.36 -09:46:06.7 17.6mag 320P/McNaught
15:15:15.56 +08:06:04.9 17.4mag 391P/Kowalski
08:07:06.03 +20:44:55.0 17.9mag 450P/LONEOS
06:59:53.88 +41:41:59.3 17.8mag 493P/LONEOS
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
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
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
-rw-r--r-- 1 apache apache 189K Jun 7 23:36 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:39:35.110 +15:17:58.28 AT 2026nsc 2026-05-09.80 20.76
16:42:48.680 +20:27:18.30 AT 2026nsb 2026-05-09.80 20.54
13:34:03.440 +31:37:31.73 AT 2026nsa 2026-05-07.80 21.26
13:50:28.150 +02:34:54.72 AT 2026nrz 2026-05-22.72 21.54
13:43:59.750 +03:47:21.63 AT 2026nry 2026-05-22.69 22.05
13:17:26.150 -01:26:00.12 AT 2026nrx 2026-05-21.64 21.7
00:35:20.216 -08:28:38.64 AT 2026nrw 2026-05-19.42 18.74
23:50:43.016 -01:09:12.25 AT 2026nrv 2026-05-23.48 19.5028
22:36:47.715 +37:31:34.81 AT 2026nru 2026-05-22.43 19.4626
23:58:04.247 +20:56:44.66 AT 2026nrt 2026-05-23.48 20.1237
16:08:58.229 +36:53:23.76 AT 2026nrs 2026-05-21.36 20.3819
19:44:04.734 +84:44:44.91 SN 2026nrr 2026-05-25.47 17.808
21:42:24.388 -20:21:08.51 SN 2026nrq 2026-05-25.56 18.623
22:03:20.669 -84:55:27.45 AT 2026nrp 2026-05-22.30 19.244
23:07:53.376 -39:04:26.84 AT 2026nro 2026-05-22.38 19.567
00:40:07.848 -39:10:21.32 AT 2026nrn 2026-05-12.41 18.737
23:05:28.381 -21:25:50.28 AT 2026nrm 2026-05-25.58 18.887
19:27:28.750 -48:42:52.35 AT 2026nrl 2026-05-22.24 19.107
12:33:38.422 +12:02:05.88 AT 2026nrk 2026-05-25.29 21.322
12:32:27.199 +02:39:54.51 AT 2026nrj 2026-05-25.29 21.0728
-rw-r--r-- 1 apache apache 30K Jun 7 23:36 tns_transients_list.txt
