This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf
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 14.1636 2461205.6636 11.91 09:59:01.05 +14:36:16.5
221.34071 48.05281 galactic Leo Second-epoch detections are separated by 0.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.44 Nysa -0 1 1 11.5 0 -0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:59:01.05 +14:36:16.5: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:59:01.05 +14:36:16.5: 16.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 59 01.05 +14 36 16.5 11.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461205.6636,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260614.1636 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.64 09:24:05.66 +17:00:58.8
213.61584 41.24676 galactic Leo Second-epoch detections are separated by 0.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.82 Alkmene -0 -1 2 13.1 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:24:05.66 +17:00:58.8: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:24:05.66 +17:00:58.8: 15.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 24 05.66 +17 00 58.8 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461205.6636,12.64,0.05,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
VARIABLE_NAME 20260614.1636 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 14.1636 2461205.6636 12.84 09:34:19.79 +15:54:01.5
216.25147 43.10513 galactic Leo Second-epoch detections are separated by 1.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.337 Devosa -0 -0 0 13.9 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:34:19.79 +15:54:01.5: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:34:19.79 +15:54:01.5: 16.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 34 19.79 +15 54 01.5 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461205.6636,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260614.1636 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.84 09:42:33.04 +10:07:03.6
224.54738 42.46573 galactic Leo Second-epoch detections are separated by 8.4" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:42:33.04 +10:07:03.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:42:33.04 +10:07:03.6: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:42:33.04 +10:07:03.6: 16.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 42 33.04 +10 07 03.6 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.71 10:05:49.23 +16:23:10.4
219.85548 50.27033 galactic Leo Second-epoch detections are separated by 0.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:05:49.23 +16:23:10.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.460+/-0.029 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:05:49.23 +16:23:10.4: 13.51 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:05:49.23 +16:23:10.4: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 05 49.23 +16 23 10.4 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.71,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.90 10:08:11.07 +18:11:00.1
217.54882 51.46595 galactic Leo Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:11.07 +18:11:00.1 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.259+/-0.033 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:11.07 +18:11:00.1: 14.05 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:11.07 +18:11:00.1: 14.07 +/- 0.06 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!
TCP 2026 06 14.1636* 10 08 11.07 +18 11 00.1 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.90,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.89 10:09:44.00 +18:06:01.7
217.88629 51.77959 galactic Leo Second-epoch detections are separated by 0.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:44.00 +18:06:01.7 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.031 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:44.00 +18:06:01.7: 14.20 +/- 0.07 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:44.00 +18:06:01.7: 14.11 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 44.00 +18 06 01.7 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.89,0.05,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 20260614.1636 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.65 10:09:00.33 +17:01:14.6
219.39421 51.21850 galactic Leo Second-epoch detections are separated by 1.2" and 5.6 pix
The object was found in VSX 0" NSVS 10268408
Type: EA
# Max. Min./Amp. JD0 Period
13.600 V 14.300 V 2454969.08000 2.119660000000
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:00.33 +17:01:14.6: 13.53 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:00.33 +17:01:14.6: 13.67 +/- 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!
TCP 2026 06 14.1636* 10 09 00.33 +17 01 14.6 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 10268408,2461205.6636,12.65,0.05,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
NSVS 10268408 20260614.1636 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 14.1636 2461205.6636 12.61 09:48:43.33 +11:00:10.0
224.43099 44.21979 galactic Leo Second-epoch detections are separated by 0.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:48:43.33 +11:00:10.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.458+/-0.037 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:48:43.33 +11:00:10.0: 13.60 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:48:43.33 +11:00:10.0: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 48 43.33 +11 00 10.0 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.61,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.31 10:12:32.91 +17:01:37.5
219.90503 52.00382 galactic Leo Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:32.91 +17:01:37.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.415+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:32.91 +17:01:37.5: 13.35 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:32.91 +17:01:37.5: 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!
TCP 2026 06 14.1636* 10 12 32.91 +17 01 37.5 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.31,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.22 10:11:25.30 +17:45:26.5
218.64122 52.02869 galactic Leo Second-epoch detections are separated by 1.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:25.30 +17:45:26.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.278+/-0.028 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:25.30 +17:45:26.5: 13.15 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:25.30 +17:45:26.5: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 11 25.30 +17 45 26.5 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.22,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.38 10:09:16.57 +15:42:59.3
221.34070 50.76641 galactic Leo Second-epoch detections are separated by 1.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:16.57 +15:42:59.3 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.588+/-0.031 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:16.57 +15:42:59.3: 13.18 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:16.57 +15:42:59.3: 13.30 +/- 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!
TCP 2026 06 14.1636* 10 09 16.57 +15 42 59.3 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.38,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.16 10:12:07.19 +17:51:42.3
218.58241 52.22158 galactic Leo Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:07.19 +17:51:42.3 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.372+/-0.032 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:07.19 +17:51:42.3: 13.18 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:07.19 +17:51:42.3: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 12 07.19 +17 51 42.3 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.16,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.03 10:09:14.66 +18:05:49.9
217.82364 51.67001 galactic Leo Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:14.66 +18:05:49.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.348+/-0.028 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:14.66 +18:05:49.9: 12.89 +/- 0.02 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:14.66 +18:05:49.9: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 14.66 +18 05 49.9 12.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.56 10:07:32.34 +16:01:55.1
220.62094 50.51017 galactic Leo Second-epoch detections are separated by 1.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:32.34 +16:01:55.1 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.032 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:07:32.34 +16:01:55.1: 13.40 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:07:32.34 +16:01:55.1: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 07 32.34 +16 01 55.1 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.56,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.79 09:36:12.89 +15:24:11.5
217.12142 43.33144 galactic Leo Second-epoch detections are separated by 2.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:36:12.89 +15:24:11.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.367+/-0.031 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:36:12.89 +15:24:11.5: 13.85 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:36:12.89 +15:24:11.5: 13.66 +/- 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!
TCP 2026 06 14.1636* 09 36 12.89 +15 24 11.5 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.79,0.05,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
target 20260614.1636 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 14.1636 2461205.6636 12.79 10:12:39.69 +17:21:26.2
219.42462 52.15410 galactic Leo Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:39.69 +17:21:26.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.524+/-0.030 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:39.69 +17:21:26.2: 13.84 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:39.69 +17:21:26.2: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 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!
TCP 2026 06 14.1636* 10 12 39.69 +17 21 26.2 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.79,0.05,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
target 20260614.1636 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 14.1636 2461205.6636 12.66 09:24:22.65 +16:19:53.7
214.49391 41.05613 galactic Leo Second-epoch detections are separated by 1.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:24:22.65 +16:19:53.7 (user input) | T | P | (position from user input) J-Ks=0.611+/-0.025 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:24:22.65 +16:19:53.7: 13.55 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:24:22.65 +16:19:53.7: 13.44 +/- 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!
TCP 2026 06 14.1636* 09 24 22.65 +16 19 53.7 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.66,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.31 10:10:33.44 +17:35:44.7
218.76146 51.77769 galactic Leo Second-epoch detections are separated by 0.5" and 5.5 pix
The object was found in VSX 2" Gaia DR3 622575614297953024
Type: ROT
# Max. Min./Amp. JD0 Period
12.860 G 12.880 G K
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:33.44 +17:35:44.7: 13.29 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:33.44 +17:35:44.7: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 33.44 +17 35 44.7 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 622575614297953024,2461205.6636,12.31,0.05,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
Gaia DR3 622575614297953024 20260614.1636 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 14.1636 2461205.6636 12.37 10:10:20.06 +17:21:07.8
219.09424 51.63755 galactic Leo Second-epoch detections are separated by 1.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:20.06 +17:21:07.8 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:20.06 +17:21:07.8: 13.29 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:20.06 +17:21:07.8: 13.47 +/- 0.04 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!
TCP 2026 06 14.1636* 10 10 20.06 +17 21 07.8 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.37,0.05,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
target 20260614.1636 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 14.1636 2461205.6636 12.51 10:12:27.87 +16:27:45.6
220.73521 51.76633 galactic Leo Second-epoch detections are separated by 0.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:27.87 +16:27:45.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:27.87 +16:27:45.6: 13.52 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:27.87 +16:27:45.6: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 12 27.87 +16 27 45.6 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.51,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.53 09:31:40.40 +10:11:05.2
222.83108 40.11894 galactic Leo Second-epoch detections are separated by 3.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:40.40 +10:11:05.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.314+/-0.040 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:40.40 +10:11:05.2: 13.50 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:40.40 +10:11:05.2: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 31 40.40 +10 11 05.2 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.53,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.60 10:10:52.56 +17:37:45.2
218.75664 51.86062 galactic Leo Second-epoch detections are separated by 0.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J152.7163+17.6250 | 10:10:52.56 +17:37:45.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.376+/-0.032 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:52.56 +17:37:45.2: 13.53 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:52.56 +17:37:45.2: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 52.56 +17 37 45.2 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J152.7163+17.6250,2461205.6636,12.60,0.05,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
ATO J152.7163+17.6250 20260614.1636 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 14.1636 2461205.6636 12.34 09:48:40.57 +09:41:57.1
226.02319 43.60029 galactic Leo Second-epoch detections are separated by 0.9" and 5.5 pix
The object was found in VSX 1" Gaia DR3 3879067097125093760
Type: ROT
# Max. Min./Amp. JD0 Period
13.190 G 13.220 G G
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:48:40.57 +09:41:57.1: 13.31 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:48:40.57 +09:41:57.1: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 48 40.57 +09 41 57.1 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3879067097125093760,2461205.6636,12.34,0.05,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
Gaia DR3 3879067097125093760 20260614.1636 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 14.1636 2461205.6636 12.39 10:13:06.84 +17:18:37.6
219.56180 52.23647 galactic Leo Second-epoch detections are separated by 0.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:13:06.84 +17:18:37.6 (user input) | T | P | (position from user input) SpType: B6 (LAMOST DR5) J-Ks=-0.130+/-0.047 (B)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:13:06.84 +17:18:37.6: 13.29 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:13:06.84 +17:18:37.6: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 13 06.84 +17 18 37.6 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 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 14.1636 2461205.6636 12.36 09:48:37.65 +08:56:43.2
226.92522 43.22730 galactic Leo Second-epoch detections are separated by 1.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:48:37.65 +08:56:43.2 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:48:37.65 +08:56:43.2: 13.53 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:48:37.65 +08:56:43.2: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 48 37.65 +08 56 43.2 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.36,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.91 09:29:25.02 +17:51:57.2
213.16475 42.73704 galactic Leo Second-epoch detections are separated by 1.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:29:25.02 +17:51:57.2 (user input) | T | P | (position from user input) J-Ks=0.318+/-0.031 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:29:25.02 +17:51:57.2: 14.09 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:29:25.02 +17:51:57.2: 13.88 +/- 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!
TCP 2026 06 14.1636* 09 29 25.02 +17 51 57.2 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.89 09:30:32.98 +16:15:39.2
215.32763 42.40202 galactic Leo Second-epoch detections are separated by 1.7" and 5.0 pix
The object was found in VSX 3" Gaia DR3 631111604101949056
Type: ROT
# Max. Min./Amp. JD0 Period
13.730 G 13.760 G K
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:32.98 +16:15:39.2: 14.21 +/- 0.07 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:32.98 +16:15:39.2: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 30 32.98 +16 15 39.2 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 631111604101949056,2461205.6636,12.89,0.05,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
Gaia DR3 631111604101949056 20260614.1636 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.83 09:29:58.07 +18:10:51.0
212.82559 42.97053 galactic Leo Second-epoch detections are separated by 3.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 633121030319171328 | 09:29:58.07 +18:10:51.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.594+/-0.039 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:29:58.07 +18:10:51.0: 13.88 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:29:58.07 +18:10:51.0: 13.72 +/- 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!
TCP 2026 06 14.1636* 09 29 58.07 +18 10 51.0 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 633121030319171328,2461205.6636,12.83,0.05,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
Large-amplitude variable Gaia DR2 633121030319171328 20260614.1636 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 14.1636 2461205.6636 12.84 09:26:20.01 +17:50:56.8
212.83375 42.04502 galactic Leo Second-epoch detections are separated by 1.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:26:20.01 +17:50:56.8 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.284+/-0.030 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:26:20.01 +17:50:56.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:26:20.01 +17:50:56.8: 13.73 +/- 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!
TCP 2026 06 14.1636* 09 26 20.01 +17 50 56.8 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.84 09:28:03.79 +16:44:23.6
214.42716 42.02795 galactic Leo Second-epoch detections are separated by 1.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:28:03.79 +16:44:23.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:28:03.79 +16:44:23.6: 13.87 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:28:03.79 +16:44:23.6: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 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!
TCP 2026 06 14.1636* 09 28 03.79 +16 44 23.6 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.82 10:11:22.40 +17:30:48.7
219.00203 51.92772 galactic Leo Second-epoch detections are separated by 1.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:22.40 +17:30:48.7 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.389+/-0.036 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:22.40 +17:30:48.7: 14.12 +/- 0.07 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:22.40 +17:30:48.7: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 11 22.40 +17 30 48.7 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.82,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.41 09:31:13.35 +10:54:31.8
221.91880 40.34583 galactic Leo Second-epoch detections are separated by 1.8" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:13.35 +10:54:31.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.286+/-0.037 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:13.35 +10:54:31.8: 13.27 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:13.35 +10:54:31.8: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 31 13.35 +10 54 31.8 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.41,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.98 09:32:22.82 +16:20:24.4
215.45266 42.83879 galactic Leo Second-epoch detections are separated by 0.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:32:22.82 +16:20:24.4 (user input) | T | P | (position from user input) SpType: M2 (LAMOST DR5) J-Ks=0.337+/-0.036 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:32:22.82 +16:20:24.4: 14.04 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:32:22.82 +16:20:24.4: 14.03 +/- 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!
TCP 2026 06 14.1636* 09 32 22.82 +16 20 24.4 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.53 10:09:21.09 +17:09:53.5
219.23108 51.34966 galactic Leo Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:21.09 +17:09:53.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.340+/-0.035 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:21.09 +17:09:53.5: 13.49 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:21.09 +17:09:53.5: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 21.09 +17 09 53.5 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.53,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.28 09:31:38.57 +10:27:13.4
222.51280 40.23404 galactic Leo Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:38.57 +10:27:13.4 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.502+/-0.030 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:38.57 +10:27:13.4: 13.25 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:38.57 +10:27:13.4: 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!
TCP 2026 06 14.1636* 09 31 38.57 +10 27 13.4 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.28,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.36 10:10:11.60 +17:16:57.6
219.17760 51.58026 galactic Leo Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:11.60 +17:16:57.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.333+/-0.032 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:11.60 +17:16:57.6: 13.24 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:11.60 +17:16:57.6: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 11.60 +17 16 57.6 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.36,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.31 10:12:59.58 +16:38:04.5
220.55945 51.95021 galactic Leo Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:59.58 +16:38:04.5 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.618+/-0.029 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:59.58 +16:38:04.5: 13.25 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:59.58 +16:38:04.5: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 12 59.58 +16 38 04.5 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.31,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.10 09:34:00.01 +09:20:00.1
224.16575 40.23592 galactic Leo Second-epoch detections are separated by 1.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:34:00.01 +09:20:00.1 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.381+/-0.038 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:34:00.01 +09:20:00.1: 13.02 +/- 0.02 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:34:00.01 +09:20:00.1: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 34 00.01 +09 20 00.1 12.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.10,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.84 09:31:48.57 +15:27:27.0
216.48955 42.37465 galactic Leo Second-epoch detections are separated by 0.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:48.57 +15:27:27.0 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=0.797+/-0.028 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:48.57 +15:27:27.0: 13.90 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:48.57 +15:27:27.0: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 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!
TCP 2026 06 14.1636* 09 31 48.57 +15 27 27.0 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.88 10:10:49.80 +17:59:38.3
218.19986 51.98411 galactic Leo Second-epoch detections are separated by 1.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:49.80 +17:59:38.3 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.370+/-0.048 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:49.80 +17:59:38.3: 13.87 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:49.80 +17:59:38.3: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 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!
TCP 2026 06 14.1636* 10 10 49.80 +17 59 38.3 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.88,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.60 10:10:03.37 +17:26:02.0
218.93217 51.60658 galactic Leo Second-epoch detections are separated by 2.4" and 5.1 pix
The object was found in VSX 1" Gaia DR3 622478440662209152
Type: ROT
# Max. Min./Amp. JD0 Period
13.330 G 13.370 G K
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:03.37 +17:26:02.0: 13.48 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:03.37 +17:26:02.0: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 03.37 +17 26 02.0 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 622478440662209152,2461205.6636,12.60,0.05,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 622478440662209152 20260614.1636 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 14.1636 2461205.6636 12.77 10:11:42.93 +17:03:10.8
219.74286 51.82973 galactic Leo Second-epoch detections are separated by 1.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:42.93 +17:03:10.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.374+/-0.032 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:42.93 +17:03:10.8: 13.87 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:42.93 +17:03:10.8: 13.97 +/- 0.06 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!
TCP 2026 06 14.1636* 10 11 42.93 +17 03 10.8 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.77,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.90 09:28:58.91 +18:09:54.4
212.73382 42.74565 galactic Leo Second-epoch detections are separated by 2.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:28:58.91 +18:09:54.4 (user input) | T | P | (position from user input) J-Ks=0.582+/-0.028 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:28:58.91 +18:09:54.4: 13.84 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:28:58.91 +18:09:54.4: 13.67 +/- 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!
TCP 2026 06 14.1636* 09 28 58.91 +18 09 54.4 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.90,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.04 09:31:42.07 +09:38:33.7
223.46436 39.87697 galactic Leo Second-epoch detections are separated by 2.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:42.07 +09:38:33.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.360+/-0.035 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:42.07 +09:38:33.7: 12.99 +/- 0.02 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:42.07 +09:38:33.7: 13.00 +/- 0.03 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!
TCP 2026 06 14.1636* 09 31 42.07 +09 38 33.7 12.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.04,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.53 10:10:18.77 +17:39:07.8
218.64196 51.74443 galactic Leo Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:18.77 +17:39:07.8 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.365+/-0.032 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:18.77 +17:39:07.8: 13.46 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:18.77 +17:39:07.8: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 18.77 +17 39 07.8 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.53,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.64 09:29:09.18 +16:49:15.9
214.45539 42.30035 galactic Leo Second-epoch detections are separated by 1.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J142.2882+16.8212 | 09:29:09.18 +16:49:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.843+/-0.028 (M)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:29:09.18 +16:49:15.9: 13.70 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:29:09.18 +16:49:15.9: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 29 09.18 +16 49 15.9 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J142.2882+16.8212,2461205.6636,12.64,0.05,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
ATO J142.2882+16.8212 20260614.1636 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 14.1636 2461205.6636 12.68 09:34:24.70 +14:58:25.2
217.42797 42.76261 galactic Leo Second-epoch detections are separated by 1.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:34:24.70 +14:58:25.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.599+/-0.028 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:34:24.70 +14:58:25.2: 13.69 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:34:24.70 +14:58:25.2: 13.57 +/- 0.03 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!
TCP 2026 06 14.1636* 09 34 24.70 +14 58 25.2 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.68,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.23 09:30:10.15 +11:17:46.8
221.31306 40.28579 galactic Leo Second-epoch detections are separated by 0.7" and 5.1 pix
The object was found in VSX 1" Gaia DR3 592830594951060992
Type: S
# Max. Min./Amp. JD0 Period
12.980 G 13.470 G G
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:10.15 +11:17:46.8: 13.24 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:10.15 +11:17:46.8: 13.22 +/- 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!
TCP 2026 06 14.1636* 09 30 10.15 +11 17 46.8 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 592830594951060992,2461205.6636,12.23,0.05,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
Gaia DR3 592830594951060992 20260614.1636 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 14.1636 2461205.6636 12.29 09:49:32.30 +09:44:49.9
226.10475 43.80996 galactic Leo Second-epoch detections are separated by 1.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:49:32.30 +09:44:49.9 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:49:32.30 +09:44:49.9: 13.25 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:49:32.30 +09:44:49.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 49 32.30 +09 44 49.9 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.29,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.30 09:33:15.55 +09:34:04.6
223.78258 40.18308 galactic Leo Second-epoch detections are separated by 1.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:33:15.55 +09:34:04.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.568+/-0.029 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:33:15.55 +09:34:04.6: 13.24 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:33:15.55 +09:34:04.6: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 33 15.55 +09 34 04.6 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.30,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.45 10:11:33.26 +16:11:36.7
220.99427 51.45934 galactic Leo Second-epoch detections are separated by 1.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:33.26 +16:11:36.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:33.26 +16:11:36.7: 13.47 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:33.26 +16:11:36.7: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 11 33.26 +16 11 36.7 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.45,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.66 10:09:14.65 +17:26:54.1
218.79454 51.43228 galactic Leo Second-epoch detections are separated by 1.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:14.65 +17:26:54.1 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.034 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:14.65 +17:26:54.1: 13.70 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:14.65 +17:26:54.1: 13.67 +/- 0.05 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!
TCP 2026 06 14.1636* 10 09 14.65 +17 26 54.1 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.66,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.77 09:35:13.80 +14:56:21.2
217.57786 42.93047 galactic Leo Second-epoch detections are separated by 0.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:35:13.80 +14:56:21.2 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.629+/-0.029 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:35:13.80 +14:56:21.2: 13.72 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:35:13.80 +14:56:21.2: 13.75 +/- 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!
TCP 2026 06 14.1636* 09 35 13.80 +14 56 21.2 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.77,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.74 10:07:13.34 +16:52:07.8
219.35906 50.76636 galactic Leo Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:13.34 +16:52:07.8 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.031 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:07:13.34 +16:52:07.8: 13.70 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:07:13.34 +16:52:07.8: 13.72 +/- 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!
TCP 2026 06 14.1636* 10 07 13.34 +16 52 07.8 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.74,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.06 10:12:53.82 +17:25:01.6
219.36862 52.22866 galactic Leo Second-epoch detections are separated by 0.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:53.82 +17:25:01.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.347+/-0.029 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:53.82 +17:25:01.6: 12.96 +/- 0.02 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:53.82 +17:25:01.6: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 12 53.82 +17 25 01.6 12.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.06,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.62 10:10:29.84 +16:05:00.4
220.99416 51.18266 galactic Leo Second-epoch detections are separated by 1.4" and 5.2 pix
The object was found in VSX 0" ASASSN-V J101029.83+160500.5
Type: ROT
# Max. Min./Amp. JD0 Period
14.050 g Y 0.240 g 2458117.76000 8.337300000000
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:29.84 +16:05:00.4: 13.67 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:29.84 +16:05:00.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 29.84 +16 05 00.4 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101029.83+160500.5,2461205.6636,12.62,0.05,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
ASASSN-V J101029.83+160500.5 20260614.1636 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 14.1636 2461205.6636 12.06 09:29:51.66 +10:38:16.1
222.04061 39.92561 galactic Leo Second-epoch detections are separated by 1.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:29:51.66 +10:38:16.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.356+/-0.031 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:29:51.66 +10:38:16.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:29:51.66 +10:38:16.1: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 29 51.66 +10 38 16.1 12.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.06,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.86 10:10:37.73 +18:19:06.0
217.68012 52.05621 galactic Leo Second-epoch detections are separated by 1.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:37.73 +18:19:06.0 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.574+/-0.030 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:37.73 +18:19:06.0: 13.84 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:37.73 +18:19:06.0: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 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!
TCP 2026 06 14.1636* 10 10 37.73 +18 19 06.0 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.86,0.05,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 20260614.1636 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.62 10:10:24.87 +17:46:32.2
218.47086 51.81238 galactic Leo Second-epoch detections are separated by 1.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:24.87 +17:46:32.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.515+/-0.033 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:24.87 +17:46:32.2: 13.68 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:24.87 +17:46:32.2: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 24.87 +17 46 32.2 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.62,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.70 10:12:42.81 +16:58:34.6
220.00584 52.02079 galactic Leo Second-epoch detections are separated by 2.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:42.81 +16:58:34.6 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.144+/-0.030 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:42.81 +16:58:34.6: 13.65 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:42.81 +16:58:34.6: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 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!
TCP 2026 06 14.1636* 10 12 42.81 +16 58 34.6 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.70,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.68 09:29:42.76 +16:12:40.2
215.28745 42.19719 galactic Leo Second-epoch detections are separated by 1.0" and 5.4 pix
The object was found in VSX 1" Gaia DR3 631105900385277568
Type: ROT
# Max. Min./Amp. JD0 Period
13.280 G 13.300 G G
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:29:42.76 +16:12:40.2: 13.65 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:29:42.76 +16:12:40.2: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 29 42.76 +16 12 40.2 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 631105900385277568,2461205.6636,12.68,0.05,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
Gaia DR3 631105900385277568 20260614.1636 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 14.1636 2461205.6636 12.85 10:12:07.51 +16:57:04.3
219.95583 51.88126 galactic Leo Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:07.51 +16:57:04.3 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.377+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:07.51 +16:57:04.3: 13.85 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:07.51 +16:57:04.3: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 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!
TCP 2026 06 14.1636* 10 12 07.51 +16 57 04.3 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.74 10:10:00.78 +18:03:47.9
217.98112 51.82817 galactic Leo Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:00.78 +18:03:47.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.337+/-0.030 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:00.78 +18:03:47.9: 13.84 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:00.78 +18:03:47.9: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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!
TCP 2026 06 14.1636* 10 10 00.78 +18 03 47.9 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.74,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.56 10:12:52.06 +16:52:05.9
220.19082 52.01328 galactic Leo Second-epoch detections are separated by 1.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:52.06 +16:52:05.9 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.466+/-0.034 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:52.06 +16:52:05.9: 13.63 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:52.06 +16:52:05.9: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 12 52.06 +16 52 05.9 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.56,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.70 10:10:25.64 +15:53:48.8
221.25588 51.09256 galactic Leo Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:25.64 +15:53:48.8 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.040 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:25.64 +15:53:48.8: 13.63 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:25.64 +15:53:48.8: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 25.64 +15 53 48.8 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.70,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.52 10:11:17.93 +16:25:16.0
220.61973 51.49300 galactic Leo Second-epoch detections are separated by 1.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:17.93 +16:25:16.0 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.409+/-0.035 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:17.93 +16:25:16.0: 13.63 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:17.93 +16:25:16.0: 13.53 +/- 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!
TCP 2026 06 14.1636* 10 11 17.93 +16 25 16.0 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.52,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.82 10:11:39.23 +18:10:23.2
218.04312 52.23140 galactic Leo Second-epoch detections are separated by 1.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:39.23 +18:10:23.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.418+/-0.030 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:39.23 +18:10:23.2: 13.82 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:39.23 +18:10:23.2: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 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!
TCP 2026 06 14.1636* 10 11 39.23 +18 10 23.2 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.82,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.64 10:10:52.67 +17:02:59.1
219.62444 51.64340 galactic Leo Second-epoch detections are separated by 1.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:52.67 +17:02:59.1 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.504+/-0.031 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:52.67 +17:02:59.1: 13.82 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:52.67 +17:02:59.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 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!
TCP 2026 06 14.1636* 10 10 52.67 +17 02 59.1 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.64,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.91 09:30:17.48 +16:29:37.2
215.00387 42.43193 galactic Leo Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:30:17.48 +16:29:37.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.409+/-0.030 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:17.48 +16:29:37.2: 13.99 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:17.48 +16:29:37.2: 13.90 +/- 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!
TCP 2026 06 14.1636* 09 30 17.48 +16 29 37.2 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.72 10:11:24.37 +17:04:19.7
219.66867 51.76868 galactic Leo Second-epoch detections are separated by 1.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:24.37 +17:04:19.7 (user input) | T | P | (position from user input) J-Ks=0.563+/-0.033 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:24.37 +17:04:19.7: 13.81 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:24.37 +17:04:19.7: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 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!
TCP 2026 06 14.1636* 10 11 24.37 +17 04 19.7 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.72,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.68 10:07:57.99 +16:51:13.6
219.48891 50.92512 galactic Leo Second-epoch detections are separated by 1.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:57.99 +16:51:13.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.590+/-0.032 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:07:57.99 +16:51:13.6: 13.81 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:07:57.99 +16:51:13.6: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 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!
TCP 2026 06 14.1636* 10 07 57.99 +16 51 13.6 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.68,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.76 09:33:21.24 +14:45:51.7
217.55123 42.44498 galactic Leo Second-epoch detections are separated by 4.1" and 5.3 pix
The object was found in VSX 1" Gaia DR3 618702271055666816
Type: ROT
# Max. Min./Amp. JD0 Period
13.450 G 13.490 G K
The object was found in astcheck.1062 Ljuba -280 -57 286 15.7 0 -0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:33:21.24 +14:45:51.7: 13.82 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:33:21.24 +14:45:51.7: 13.72 +/- 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!
TCP 2026 06 14.1636* 09 33 21.24 +14 45 51.7 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 618702271055666816,2461205.6636,12.76,0.05,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
Gaia DR3 618702271055666816 20260614.1636 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 14.1636 2461205.6636 12.51 10:12:08.38 +16:44:42.2
220.26583 51.80494 galactic Leo Second-epoch detections are separated by 1.0" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:08.38 +16:44:42.2 (user input) | T | P | (position from user input) J-Ks=0.755+/-0.028 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:08.38 +16:44:42.2: 13.48 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:08.38 +16:44:42.2: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 12 08.38 +16 44 42.2 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.51,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.48 09:35:33.71 +15:27:17.3
216.97190 43.20665 galactic Leo Second-epoch detections are separated by 0.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:35:33.71 +15:27:17.3 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.533+/-0.029 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:35:33.71 +15:27:17.3: 13.48 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:35:33.71 +15:27:17.3: 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!
TCP 2026 06 14.1636* 09 35 33.71 +15 27 17.3 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.48,0.05,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 20260614.1636 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 14.1636 2461205.6636 13.01 09:29:31.01 +18:50:09.5
211.93393 43.09642 galactic Leo Second-epoch detections are separated by 3.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:29:31.01 +18:50:09.5 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.034 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:29:31.01 +18:50:09.5: 13.97 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:29:31.01 +18:50:09.5: 13.92 +/- 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!
TCP 2026 06 14.1636* 09 29 31.01 +18 50 09.5 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.45 10:14:18.13 +17:01:09.4
220.17896 52.38802 galactic Leo Second-epoch detections are separated by 1.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:14:18.13 +17:01:09.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.426+/-0.031 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:14:18.13 +17:01:09.4: 13.45 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:14:18.13 +17:01:09.4: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 14 18.13 +17 01 09.4 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.45,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.34 09:33:46.12 +09:17:39.0
224.17627 40.16712 galactic Leo Second-epoch detections are separated by 0.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:33:46.12 +09:17:39.0 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.447+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:33:46.12 +09:17:39.0: 13.47 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:33:46.12 +09:17:39.0: 13.54 +/- 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!
TCP 2026 06 14.1636* 09 33 46.12 +09 17 39.0 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.34,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.47 10:07:21.04 +17:12:47.6
218.87270 50.92524 galactic Leo Second-epoch detections are separated by 1.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:21.04 +17:12:47.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.505+/-0.033 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:07:21.04 +17:12:47.6: 13.46 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:07:21.04 +17:12:47.6: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 07 21.04 +17 12 47.6 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.47,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.66 10:07:56.10 +15:40:49.4
221.18716 50.45658 galactic Leo Second-epoch detections are separated by 1.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:56.10 +15:40:49.4 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.030 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:07:56.10 +15:40:49.4: 13.45 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:07:56.10 +15:40:49.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 07 56.10 +15 40 49.4 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.66,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.36 09:48:42.64 +10:05:06.2
225.55871 43.79050 galactic Leo Second-epoch detections are separated by 0.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:48:42.64 +10:05:06.2 (user input) | T | P | (position from user input) J-Ks=0.537+/-0.035 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:48:42.64 +10:05:06.2: 13.46 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:48:42.64 +10:05:06.2: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 48 42.64 +10 05 06.2 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.36,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.44 10:08:49.99 +16:08:45.2
220.65058 50.84072 galactic Leo Second-epoch detections are separated by 1.3" and 5.2 pix
The object was found in VSX 0" Gaia DR3 621956176934474496
Type: ROT
# Max. Min./Amp. JD0 Period
13.150 G 13.180 G K
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:49.99 +16:08:45.2: 13.43 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:49.99 +16:08:45.2: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 08 49.99 +16 08 45.2 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 621956176934474496,2461205.6636,12.44,0.05,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
Gaia DR3 621956176934474496 20260614.1636 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 14.1636 2461205.6636 12.55 10:10:25.27 +15:55:01.4
221.22553 51.09931 galactic Leo Second-epoch detections are separated by 0.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:25.27 +15:55:01.4 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.032 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:25.27 +15:55:01.4: 13.43 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:25.27 +15:55:01.4: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 25.27 +15 55 01.4 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.55,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.24 09:48:40.64 +08:58:47.0
226.89214 43.25475 galactic Leo Second-epoch detections are separated by 3.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:48:40.64 +08:58:47.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:48:40.64 +08:58:47.0: 13.19 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:48:40.64 +08:58:47.0: 13.24 +/- 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!
TCP 2026 06 14.1636* 09 48 40.64 +08 58 47.0 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.24,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.15 09:48:14.61 +09:01:01.4
226.77609 43.17914 galactic Leo Second-epoch detections are separated by 1.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:48:14.61 +09:01:01.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:48:14.61 +09:01:01.4: 13.23 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:48:14.61 +09:01:01.4: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 48 14.61 +09 01 01.4 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.15,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.25 09:31:09.14 +10:38:31.8
222.22135 40.21118 galactic Leo Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:09.14 +10:38:31.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.454+/-0.040 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:09.14 +10:38:31.8: 13.20 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:09.14 +10:38:31.8: 13.22 +/- 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!
TCP 2026 06 14.1636* 09 31 09.14 +10 38 31.8 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.47 10:10:31.89 +17:04:55.3
219.52565 51.57915 galactic Leo Second-epoch detections are separated by 1.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:31.89 +17:04:55.3 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.295+/-0.033 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:31.89 +17:04:55.3: 13.42 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:31.89 +17:04:55.3: 13.56 +/- 0.04 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!
TCP 2026 06 14.1636* 10 10 31.89 +17 04 55.3 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.47,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.44 10:07:57.58 +17:33:49.5
218.44134 51.19070 galactic Leo Second-epoch detections are separated by 0.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:57.58 +17:33:49.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.347+/-0.035 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:07:57.58 +17:33:49.5: 13.43 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:07:57.58 +17:33:49.5: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 07 57.58 +17 33 49.5 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.44,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.43 10:12:42.47 +17:03:58.2
219.87000 52.05396 galactic Leo Second-epoch detections are separated by 2.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:42.47 +17:03:58.2 (user input) | T | P | (position from user input) J-Ks=0.579+/-0.033 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:42.47 +17:03:58.2: 13.40 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:42.47 +17:03:58.2: 13.47 +/- 0.04 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!
TCP 2026 06 14.1636* 10 12 42.47 +17 03 58.2 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.43,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.45 10:09:43.05 +17:27:08.1
218.85629 51.53848 galactic Leo Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 623229716344025984 | 10:09:43.05 +17:27:08.1 (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=0.439+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:43.05 +17:27:08.1: 13.41 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:43.05 +17:27:08.1: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 43.05 +17 27 08.1 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 623229716344025984,2461205.6636,12.45,0.05,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
Large-amplitude variable Gaia DR2 623229716344025984 20260614.1636 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 14.1636 2461205.6636 12.46 10:09:10.51 +17:06:33.7
219.28778 51.28966 galactic Leo Second-epoch detections are separated by 0.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:10.51 +17:06:33.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.334+/-0.035 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:10.51 +17:06:33.7: 13.39 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:10.51 +17:06:33.7: 13.43 +/- 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!
TCP 2026 06 14.1636* 10 09 10.51 +17 06 33.7 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.46,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.29 10:09:35.76 +17:29:59.4
218.76796 51.52930 galactic Leo Second-epoch detections are separated by 0.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:35.76 +17:29:59.4 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.031 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:35.76 +17:29:59.4: 13.19 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:35.76 +17:29:59.4: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 35.76 +17 29 59.4 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.29,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.71 10:08:51.14 +16:58:16.7
219.44488 51.16583 galactic Leo Second-epoch detections are separated by 1.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:51.14 +16:58:16.7 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.522+/-0.032 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:51.14 +16:58:16.7: 13.79 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:51.14 +16:58:16.7: 13.80 +/- 0.05 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!
TCP 2026 06 14.1636* 10 08 51.14 +16 58 16.7 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.71,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.28 10:08:46.96 +16:53:45.2
219.54584 51.12163 galactic Leo Second-epoch detections are separated by 0.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:46.96 +16:53:45.2 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:46.96 +16:53:45.2: 13.19 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:46.96 +16:53:45.2: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 08 46.96 +16 53 45.2 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.28,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.57 10:07:31.48 +17:23:18.4
218.63931 51.02932 galactic Leo Second-epoch detections are separated by 0.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:31.48 +17:23:18.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.279+/-0.035 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:07:31.48 +17:23:18.4: 13.62 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:07:31.48 +17:23:18.4: 13.70 +/- 0.05 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!
TCP 2026 06 14.1636* 10 07 31.48 +17 23 18.4 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.57,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.79 10:10:37.45 +17:19:13.2
219.18366 51.68971 galactic Leo Second-epoch detections are separated by 1.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:37.45 +17:19:13.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.357+/-0.032 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:37.45 +17:19:13.2: 13.79 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:37.45 +17:19:13.2: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 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!
TCP 2026 06 14.1636* 10 10 37.45 +17 19 13.2 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.79,0.05,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
target 20260614.1636 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 14.1636 2461205.6636 12.73 10:11:21.87 +18:21:38.7
217.71690 52.23444 galactic Leo Second-epoch detections are separated by 2.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:21.87 +18:21:38.7 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.751+/-0.028 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:21.87 +18:21:38.7: 13.80 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:21.87 +18:21:38.7: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 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!
TCP 2026 06 14.1636* 10 11 21.87 +18 21 38.7 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.79 10:10:35.29 +17:26:05.4
219.00715 51.72465 galactic Leo Second-epoch detections are separated by 1.5" and 5.7 pix
The object was found in VSX 0" Gaia DR3 622476658251236608
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.750 G K
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:35.29 +17:26:05.4: 13.79 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:35.29 +17:26:05.4: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 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!
TCP 2026 06 14.1636* 10 10 35.29 +17 26 05.4 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 622476658251236608,2461205.6636,12.79,0.05,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 622476658251236608 20260614.1636 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 14.1636 2461205.6636 12.80 10:08:34.97 +16:41:25.2
219.81853 50.99847 galactic Leo Second-epoch detections are separated by 0.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:34.97 +16:41:25.2 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.375+/-0.035 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:34.97 +16:41:25.2: 13.79 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:34.97 +16:41:25.2: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 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!
TCP 2026 06 14.1636* 10 08 34.97 +16 41 25.2 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.63 10:07:05.61 +15:56:35.5
220.68193 50.37661 galactic Leo Second-epoch detections are separated by 1.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:05.61 +15:56:35.5 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.035 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:07:05.61 +15:56:35.5: 13.38 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:07:05.61 +15:56:35.5: 13.58 +/- 0.04 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!
TCP 2026 06 14.1636* 10 07 05.61 +15 56 35.5 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.63,0.05,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
target 20260614.1636 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 14.1636 2461205.6636 12.39 09:32:43.71 +10:24:01.9
222.73336 40.44811 galactic Leo Second-epoch detections are separated by 0.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:32:43.71 +10:24:01.9 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.234+/-0.035 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:32:43.71 +10:24:01.9: 13.40 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:32:43.71 +10:24:01.9: 13.42 +/- 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!
TCP 2026 06 14.1636* 09 32 43.71 +10 24 01.9 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 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 14.1636 2461205.6636 12.65 10:07:42.15 +17:21:22.3
218.71207 51.05666 galactic Leo Second-epoch detections are separated by 2.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J151.9254+17.3560 | 10:07:42.15 +17:21:22.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.316+/-0.033 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:07:42.15 +17:21:22.3: 13.59 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:07:42.15 +17:21:22.3: 13.66 +/- 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!
TCP 2026 06 14.1636* 10 07 42.15 +17 21 22.3 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J151.9254+17.3560,2461205.6636,12.65,0.05,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
ATO J151.9254+17.3560 20260614.1636 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 14.1636 2461205.6636 12.63 10:11:43.59 +16:43:01.3
220.24559 51.70290 galactic Leo Second-epoch detections are separated by 2.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:43.59 +16:43:01.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.410+/-0.029 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:43.59 +16:43:01.3: 13.94 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:43.59 +16:43:01.3: 13.93 +/- 0.06 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!
TCP 2026 06 14.1636* 10 11 43.59 +16 43 01.3 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.63,0.05,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
target 20260614.1636 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 14.1636 2461205.6636 12.84 10:09:41.83 +18:20:46.2
217.51017 51.85951 galactic Leo Second-epoch detections are separated by 2.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:41.83 +18:20:46.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.418+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:41.83 +18:20:46.2: 13.91 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:41.83 +18:20:46.2: 14.05 +/- 0.07 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!
TCP 2026 06 14.1636* 10 09 41.83 +18 20 46.2 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.80 10:08:38.77 +15:50:31.2
221.06276 50.67828 galactic Leo Second-epoch detections are separated by 2.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:38.77 +15:50:31.2 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.034 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:38.77 +15:50:31.2: 13.94 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:38.77 +15:50:31.2: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 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!
TCP 2026 06 14.1636* 10 08 38.77 +15 50 31.2 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.61 10:10:00.35 +16:00:15.9
221.03449 51.04284 galactic Leo Second-epoch detections are separated by 1.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:00.35 +16:00:15.9 (user input) | T | P | (position from user input) J-Ks=0.585+/-0.033 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:00.35 +16:00:15.9: 13.59 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:00.35 +16:00:15.9: 13.58 +/- 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!
TCP 2026 06 14.1636* 10 10 00.35 +16 00 15.9 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.61,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.59 09:29:05.97 +12:15:26.3
220.02750 40.46715 galactic Leo Second-epoch detections are separated by 2.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:29:05.97 +12:15:26.3 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=0.594+/-0.039 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:29:05.97 +12:15:26.3: 13.59 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:29:05.97 +12:15:26.3: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 29 05.97 +12 15 26.3 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.59,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.52 10:07:46.14 +16:28:19.3
220.01750 50.73406 galactic Leo Second-epoch detections are separated by 1.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:46.14 +16:28:19.3 (user input) | T | P | (position from user input) SpType: Carbon (LAMOST DR5) J-Ks=0.564+/-0.035 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:07:46.14 +16:28:19.3: 13.38 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:07:46.14 +16:28:19.3: 13.44 +/- 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!
TCP 2026 06 14.1636* 10 07 46.14 +16 28 19.3 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.52,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.55 10:09:09.07 +16:58:40.2
219.47872 51.23437 galactic Leo Second-epoch detections are separated by 0.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:09.07 +16:58:40.2 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.407+/-0.032 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:09.07 +16:58:40.2: 13.57 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:09.07 +16:58:40.2: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 09.07 +16 58 40.2 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.55,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.53 10:09:13.82 +17:30:56.4
218.69233 51.45424 galactic Leo Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:13.82 +17:30:56.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.466+/-0.033 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:13.82 +17:30:56.4: 13.59 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:13.82 +17:30:56.4: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 13.82 +17 30 56.4 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.53,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.41 10:12:59.74 +17:07:24.3
219.82658 52.13938 galactic Leo Second-epoch detections are separated by 1.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:59.74 +17:07:24.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.542+/-0.031 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:59.74 +17:07:24.3: 13.38 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:59.74 +17:07:24.3: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 12 59.74 +17 07 24.3 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.41,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.26 10:10:19.61 +18:00:14.8
218.11416 51.87630 galactic Leo Second-epoch detections are separated by 1.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:19.61 +18:00:14.8 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.527+/-0.028 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:19.61 +18:00:14.8: 13.16 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:19.61 +18:00:14.8: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 19.61 +18 00 14.8 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.26,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.79 10:13:30.26 +16:43:04.6
220.51228 52.09548 galactic Leo Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:13:30.26 +16:43:04.6 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.429+/-0.030 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:13:30.26 +16:43:04.6: 13.79 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:13:30.26 +16:43:04.6: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 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!
TCP 2026 06 14.1636* 10 13 30.26 +16 43 04.6 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.79,0.05,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
target 20260614.1636 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 14.1636 2461205.6636 12.59 09:30:03.58 +16:22:58.2
215.11485 42.33893 galactic Leo Second-epoch detections are separated by 2.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:30:03.58 +16:22:58.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.375+/-0.029 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:03.58 +16:22:58.2: 13.58 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:03.58 +16:22:58.2: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 30 03.58 +16 22 58.2 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.59,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.78 09:35:08.76 +14:36:03.8
217.98987 42.77704 galactic Leo Second-epoch detections are separated by 1.6" and 5.3 pix
The object was found in VSX 1" Gaia DR3 617936392487607424
Type: ROT
# Max. Min./Amp. JD0 Period
13.630 G 13.650 G K
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:35:08.76 +14:36:03.8: 13.98 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:35:08.76 +14:36:03.8: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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!
TCP 2026 06 14.1636* 09 35 08.76 +14 36 03.8 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 617936392487607424,2461205.6636,12.78,0.05,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
Gaia DR3 617936392487607424 20260614.1636 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 14.1636 2461205.6636 12.81 10:10:33.94 +16:16:03.3
220.73470 51.27083 galactic Leo Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:33.94 +16:16:03.3 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.323+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:33.94 +16:16:03.3: 13.77 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:33.94 +16:16:03.3: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 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!
TCP 2026 06 14.1636* 10 10 33.94 +16 16 03.3 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.81,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.69 10:11:01.97 +16:14:39.9
220.83973 51.36463 galactic Leo Second-epoch detections are separated by 1.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 622148179152381184 | 10:11:01.97 +16:14:39.9 (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: F7 (LAMOST DR5) J-Ks=0.264+/-0.036 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:01.97 +16:14:39.9: 13.77 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:01.97 +16:14:39.9: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 11 01.97 +16 14 39.9 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 622148179152381184,2461205.6636,12.69,0.05,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
Large-amplitude variable Gaia DR2 622148179152381184 20260614.1636 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 14.1636 2461205.6636 12.73 10:10:03.92 +16:54:20.6
219.71905 51.40884 galactic Leo Second-epoch detections are separated by 2.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:03.92 +16:54:20.6 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.297+/-0.038 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:03.92 +16:54:20.6: 13.75 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:03.92 +16:54:20.6: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 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!
TCP 2026 06 14.1636* 10 10 03.92 +16 54 20.6 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.88 09:28:42.96 +18:35:22.1
212.16169 42.83385 galactic Leo Second-epoch detections are separated by 2.3" and 5.0 pix
The object was found in VSX 2" Gaia DR3 633898281961244928
Type: ROT
# Max. Min./Amp. JD0 Period
13.600 G 13.630 G F
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:28:42.96 +18:35:22.1: 14.07 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:28:42.96 +18:35:22.1: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 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!
TCP 2026 06 14.1636* 09 28 42.96 +18 35 22.1 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 633898281961244928,2461205.6636,12.88,0.05,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
Gaia DR3 633898281961244928 20260614.1636 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 14.1636 2461205.6636 12.49 10:09:15.52 +16:02:10.0
220.87455 50.89088 galactic Leo Second-epoch detections are separated by 0.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:15.52 +16:02:10.0 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:15.52 +16:02:10.0: 13.37 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:15.52 +16:02:10.0: 13.47 +/- 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!
TCP 2026 06 14.1636* 10 09 15.52 +16 02 10.0 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.49,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.76 09:32:12.65 +16:39:56.5
215.01983 42.92283 galactic Leo Second-epoch detections are separated by 1.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:32:12.65 +16:39:56.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.503+/-0.028 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:32:12.65 +16:39:56.5: 13.78 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:32:12.65 +16:39:56.5: 13.65 +/- 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!
TCP 2026 06 14.1636* 09 32 12.65 +16 39 56.5 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.76,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.27 09:30:28.33 +10:19:40.6
222.48958 39.92040 galactic Leo Second-epoch detections are separated by 3.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:30:28.33 +10:19:40.6 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.312+/-0.031 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:28.33 +10:19:40.6: 13.17 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:28.33 +10:19:40.6: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 30 28.33 +10 19 40.6 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.27,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.24 10:13:46.76 +16:47:06.6
220.45305 52.18226 galactic Leo Second-epoch detections are separated by 1.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:13:46.76 +16:47:06.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.376+/-0.030 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:13:46.76 +16:47:06.6: 13.13 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:13:46.76 +16:47:06.6: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 13 46.76 +16 47 06.6 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.24,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.19 09:32:44.55 +10:29:47.3
222.62291 40.49456 galactic Leo Second-epoch detections are separated by 0.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:32:44.55 +10:29:47.3 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.035 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:32:44.55 +10:29:47.3: 13.15 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:32:44.55 +10:29:47.3: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 32 44.55 +10 29 47.3 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.19,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.54 10:08:41.58 +17:06:14.2
219.22610 51.18098 galactic Leo Second-epoch detections are separated by 1.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J152.1757+17.1016 | 10:08:41.58 +17:06:14.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.468+/-0.033 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:41.58 +17:06:14.2: 13.36 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:41.58 +17:06:14.2: 13.46 +/- 0.04 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!
TCP 2026 06 14.1636* 10 08 41.58 +17 06 14.2 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J152.1757+17.1016,2461205.6636,12.54,0.05,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
ATO J152.1757+17.1016 20260614.1636 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 14.1636 2461205.6636 12.79 10:09:25.01 +16:30:57.3
220.19763 51.11494 galactic Leo Second-epoch detections are separated by 1.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J152.3594+16.5071 | 10:09:25.01 +16:30:57.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.361+/-0.036 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:25.01 +16:30:57.3: 13.75 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:25.01 +16:30:57.3: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 25.01 +16 30 57.3 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J152.3594+16.5071,2461205.6636,12.79,0.05,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
ATO J152.3594+16.5071 20260614.1636 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 14.1636 2461205.6636 12.22 10:08:23.11 +16:07:47.4
220.60647 50.73558 galactic Leo Second-epoch detections are separated by 0.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:23.11 +16:07:47.4 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.331+/-0.031 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:23.11 +16:07:47.4: 13.13 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:23.11 +16:07:47.4: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 08 23.11 +16 07 47.4 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.22,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.74 10:10:43.04 +16:37:11.4
220.23864 51.44243 galactic Leo Second-epoch detections are separated by 2.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:43.04 +16:37:11.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.434+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:43.04 +16:37:11.4: 13.93 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:43.04 +16:37:11.4: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 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!
TCP 2026 06 14.1636* 10 10 43.04 +16 37 11.4 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.74,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.56 10:10:10.89 +16:33:40.8
220.24490 51.30140 galactic Leo Second-epoch detections are separated by 1.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:10.89 +16:33:40.8 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.324+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:10.89 +16:33:40.8: 13.56 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:10.89 +16:33:40.8: 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!
TCP 2026 06 14.1636* 10 10 10.89 +16 33 40.8 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.56,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.91 09:30:57.82 +15:54:50.3
215.81326 42.36245 galactic Leo Second-epoch detections are separated by 1.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 619076040585434752 | 09:30:57.82 +15:54:50.3 (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: K3 (LAMOST DR5) J-Ks=0.591+/-0.032 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:57.82 +15:54:50.3: 13.99 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:57.82 +15:54:50.3: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 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!
TCP 2026 06 14.1636* 09 30 57.82 +15 54 50.3 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 619076040585434752,2461205.6636,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 619076040585434752 20260614.1636 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.80 09:31:17.58 +16:11:51.7
215.49826 42.54340 galactic Leo Second-epoch detections are separated by 0.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:17.58 +16:11:51.7 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.450+/-0.026 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:17.58 +16:11:51.7: 13.75 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:17.58 +16:11:51.7: 13.69 +/- 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!
TCP 2026 06 14.1636* 09 31 17.58 +16 11 51.7 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.64 09:31:31.92 +15:40:20.7
216.18623 42.39611 galactic Leo Second-epoch detections are separated by 0.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:31.92 +15:40:20.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.357+/-0.028 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:31.92 +15:40:20.7: 13.74 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:31.92 +15:40:20.7: 13.59 +/- 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!
TCP 2026 06 14.1636* 09 31 31.92 +15 40 20.7 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.64,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.69 10:09:12.68 +18:02:07.5
217.91196 51.64041 galactic Leo Second-epoch detections are separated by 2.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:12.68 +18:02:07.5 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.461+/-0.028 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:12.68 +18:02:07.5: 13.71 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:12.68 +18:02:07.5: 13.87 +/- 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!
TCP 2026 06 14.1636* 10 09 12.68 +18 02 07.5 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.69,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.82 09:29:30.01 +16:17:37.4
215.15831 42.18106 galactic Leo Second-epoch detections are separated by 0.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:29:30.01 +16:17:37.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.386+/-0.029 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:29:30.01 +16:17:37.4: 13.74 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:29:30.01 +16:17:37.4: 13.73 +/- 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!
TCP 2026 06 14.1636* 09 29 30.01 +16 17 37.4 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.82,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.36 09:32:51.16 +10:05:09.8
223.11934 40.33235 galactic Leo Second-epoch detections are separated by 0.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:32:51.16 +10:05:09.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.547+/-0.030 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:32:51.16 +10:05:09.8: 13.37 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:32:51.16 +10:05:09.8: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 32 51.16 +10 05 09.8 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.36,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.32 10:09:14.38 +17:46:55.8
218.29567 51.55457 galactic Leo Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:14.38 +17:46:55.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.404+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:14.38 +17:46:55.8: 13.37 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:14.38 +17:46:55.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 14.38 +17 46 55.8 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.32,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.41 10:10:51.08 +16:30:39.8
220.41941 51.42957 galactic Leo Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:51.08 +16:30:39.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.318+/-0.035 (F)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:51.08 +16:30:39.8: 13.35 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:51.08 +16:30:39.8: 13.38 +/- 0.04 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!
TCP 2026 06 14.1636* 10 10 51.08 +16 30 39.8 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.41,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.96 10:08:39.09 +18:12:16.5
217.58076 51.57711 galactic Leo Second-epoch detections are separated by 1.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J152.1642+18.2110 | 10:08:39.09 +18:12:16.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.560+/-0.027 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:39.09 +18:12:16.5: 14.14 +/- 0.07 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:39.09 +18:12:16.5: 14.25 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 08 39.09 +18 12 16.5 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J152.1642+18.2110,2461205.6636,12.96,0.05,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
ATO J152.1642+18.2110 20260614.1636 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.88 09:32:40.39 +17:44:38.0
213.69798 43.41814 galactic Leo Second-epoch detections are separated by 2.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:32:40.39 +17:44:38.0 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.030 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:32:40.39 +17:44:38.0: 13.93 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:32:40.39 +17:44:38.0: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 32 40.39 +17 44 38.0 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.88,0.05,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 20260614.1636 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 14.1636 2461205.6636 13.09 10:10:50.87 +16:15:08.1
220.80007 51.32696 galactic Leo Second-epoch detections are separated by 2.6" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:50.87 +16:15:08.1 (user input) | T | P | (position from user input) J-Ks=0.476+/-0.036 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:50.87 +16:15:08.1: 14.48 +/- 0.09 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:50.87 +16:15:08.1: 14.62 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 50.87 +16 15 08.1 13.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,13.09,0.05,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 20260614.1636 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.64 10:10:39.35 +17:06:38.0
219.50134 51.61747 galactic Leo Second-epoch detections are separated by 0.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:39.35 +17:06:38.0 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.334+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:39.35 +17:06:38.0: 13.56 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:39.35 +17:06:38.0: 13.63 +/- 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!
TCP 2026 06 14.1636* 10 10 39.35 +17 06 38.0 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.64,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.46 09:31:42.89 +10:00:26.2
223.04369 40.04718 galactic Leo Second-epoch detections are separated by 2.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:42.89 +10:00:26.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.523+/-0.049 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:42.89 +10:00:26.2: 13.54 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:42.89 +10:00:26.2: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 31 42.89 +10 00 26.2 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.46,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.55 10:09:05.56 +17:31:22.0
218.66220 51.42641 galactic Leo Second-epoch detections are separated by 1.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:05.56 +17:31:22.0 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.426+/-0.030 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:05.56 +17:31:22.0: 13.56 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:05.56 +17:31:22.0: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 05.56 +17 31 22.0 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.55,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.64 10:09:43.06 +17:58:14.6
218.07953 51.72920 galactic Leo Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:43.06 +17:58:14.6 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.667+/-0.027 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:43.06 +17:58:14.6: 13.54 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:43.06 +17:58:14.6: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 43.06 +17 58 14.6 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.64,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.43 10:11:10.07 +17:21:23.4
219.20823 51.82354 galactic Leo Second-epoch detections are separated by 1.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:10.07 +17:21:23.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.359+/-0.034 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:10.07 +17:21:23.4: 13.34 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:10.07 +17:21:23.4: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 11 10.07 +17 21 23.4 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.43,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.99 09:31:49.58 +16:06:54.1
215.66803 42.63065 galactic Leo Second-epoch detections are separated by 3.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J142.9542+16.1122 | 09:31:49.58 +16:06:54.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.335+/-0.035 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:49.58 +16:06:54.1: 14.23 +/- 0.07 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:49.58 +16:06:54.1: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 31 49.58 +16 06 54.1 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J142.9542+16.1122,2461205.6636,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J142.9542+16.1122 20260614.1636 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.60 10:09:24.22 +17:15:06.0
219.10982 51.39393 galactic Leo Second-epoch detections are separated by 1.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:24.22 +17:15:06.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.407+/-0.032 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:24.22 +17:15:06.0: 13.54 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:24.22 +17:15:06.0: 13.66 +/- 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!
TCP 2026 06 14.1636* 10 09 24.22 +17 15 06.0 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.60,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.23 09:31:13.40 +10:13:09.9
222.72504 40.03602 galactic Leo Second-epoch detections are separated by 2.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:13.40 +10:13:09.9 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.402+/-0.039 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:31:13.40 +10:13:09.9: 13.11 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:31:13.40 +10:13:09.9: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 31 13.40 +10 13 09.9 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 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 14.1636 2461205.6636 12.12 09:47:41.35 +09:18:14.3
226.34086 43.19760 galactic Leo Second-epoch detections are separated by 1.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:47:41.35 +09:18:14.3 (user input) | T | P | (position from user input) J-Ks=0.573+/-0.035 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:47:41.35 +09:18:14.3: 13.10 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:47:41.35 +09:18:14.3: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 47 41.35 +09 18 14.3 12.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1636 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.04 09:32:20.14 +10:03:48.9
223.06941 40.20887 galactic Leo Second-epoch detections are separated by 1.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:32:20.14 +10:03:48.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.693+/-0.034 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:32:20.14 +10:03:48.9: 13.09 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:32:20.14 +10:03:48.9: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 32 20.14 +10 03 48.9 12.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.04,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.38 10:12:18.53 +17:29:42.2
219.16511 52.12778 galactic Leo Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:18.53 +17:29:42.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.506+/-0.034 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:18.53 +17:29:42.2: 13.32 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:18.53 +17:29:42.2: 13.42 +/- 0.04 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!
TCP 2026 06 14.1636* 10 12 18.53 +17 29 42.2 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.38,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.35 09:32:19.94 +09:53:48.4
223.26305 40.13185 galactic Leo Second-epoch detections are separated by 1.4" and 5.5 pix
The object was found in VSX 1" Gaia DR3 589103662849532160
Type: ROT
# Max. Min./Amp. JD0 Period
13.050 G 13.070 G K
The object was not found in astcheck.
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:32:19.94 +09:53:48.4: 13.32 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:32:19.94 +09:53:48.4: 13.41 +/- 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!
TCP 2026 06 14.1636* 09 32 19.94 +09 53 48.4 12.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 589103662849532160,2461205.6636,12.35,0.05,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
Gaia DR3 589103662849532160 20260614.1636 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 14.1636 2461205.6636 12.70 10:11:15.98 +16:30:21.8
220.48929 51.51915 galactic Leo Second-epoch detections are separated by 2.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:15.98 +16:30:21.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.350+/-0.033 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:11:15.98 +16:30:21.8: 13.90 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:11:15.98 +16:30:21.8: 13.92 +/- 0.06 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!
TCP 2026 06 14.1636* 10 11 15.98 +16 30 21.8 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.70,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.40 10:10:26.63 +18:28:22.3
217.41980 52.07004 galactic Leo Second-epoch detections are separated by 1.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:26.63 +18:28:22.3 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.379+/-0.030 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:26.63 +18:28:22.3: 13.31 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:26.63 +18:28:22.3: 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!
TCP 2026 06 14.1636* 10 10 26.63 +18 28 22.3 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.40,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.41 10:12:57.74 +17:36:06.1
219.09833 52.31207 galactic Leo Second-epoch detections are separated by 1.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:57.74 +17:36:06.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.367+/-0.030 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:12:57.74 +17:36:06.1: 13.31 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:12:57.74 +17:36:06.1: 13.27 +/- 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!
TCP 2026 06 14.1636* 10 12 57.74 +17 36 06.1 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.41,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.74 09:32:49.20 +15:25:18.6
216.66239 42.58517 galactic Leo Second-epoch detections are separated by 2.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:32:49.20 +15:25:18.6 (user input) | T | P | (position from user input) J-Ks=0.642+/-0.027 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:32:49.20 +15:25:18.6: 13.71 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:32:49.20 +15:25:18.6: 13.69 +/- 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!
TCP 2026 06 14.1636* 09 32 49.20 +15 25 18.6 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.74,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.10 09:30:24.00 +10:29:40.8
222.28502 39.97973 galactic Leo Second-epoch detections are separated by 0.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:30:24.00 +10:29:40.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.368+/-0.031 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:30:24.00 +10:29:40.8: 13.09 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:30:24.00 +10:29:40.8: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 09 30 24.00 +10 29 40.8 12.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.10,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.81 10:10:24.93 +16:53:23.4
219.79413 51.48010 galactic Leo Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:24.93 +16:53:23.4 (user input) | T | P | (position from user input) J-Ks=0.545+/-0.033 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:24.93 +16:53:23.4: 14.06 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:24.93 +16:53:23.4: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 10 24.93 +16 53 23.4 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.81,0.05,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 20260614.1636 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 14.1636 2461205.6636 12.96 09:29:35.58 +17:06:54.5
214.13724 42.50613 galactic Leo Second-epoch detections are separated by 2.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:29:35.58 +17:06:54.5 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.536+/-0.030 (K)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:29:35.58 +17:06:54.5: 14.06 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:29:35.58 +17:06:54.5: 13.94 +/- 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!
TCP 2026 06 14.1636* 09 29 35.58 +17 06 54.5 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.96,0.05,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 20260614.1636 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.96 10:09:43.59 +17:50:30.7
218.27444 51.68425 galactic Leo Second-epoch detections are separated by 1.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:43.59 +17:50:30.7 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.349+/-0.040 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:09:43.59 +17:50:30.7: 14.06 +/- 0.07 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:09:43.59 +17:50:30.7: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 09 43.59 +17 50 30.7 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.96,0.05,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 20260614.1636 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.63 10:08:46.21 +18:05:18.4
217.77144 51.56174 galactic Leo Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:46.21 +18:05:18.4 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.377+/-0.029 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:46.21 +18:05:18.4: 13.54 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:46.21 +18:05:18.4: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1636* 10 08 46.21 +18 05 18.4 12.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.63,0.05,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
target 20260614.1636 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 14.1636 2461205.6636 12.89 10:10:41.90 +18:28:48.4
217.44348 52.12905 galactic Leo Second-epoch detections are separated by 1.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:41.90 +18:28:48.4 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.396+/-0.031 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:10:41.90 +18:28:48.4: 13.91 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:10:41.90 +18:28:48.4: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 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!
TCP 2026 06 14.1636* 10 10 41.90 +18 28 48.4 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.89,0.05,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 20260614.1636 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1636 2461205.6636 12.89 10:08:30.48 +16:31:16.1
220.05509 50.91635 galactic Leo Second-epoch detections are separated by 1.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:30.48 +16:31:16.1 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.395+/-0.037 (G)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:30.48 +16:31:16.1: 14.04 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:30.48 +16:31:16.1: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 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!
TCP 2026 06 14.1636* 10 08 30.48 +16 31 16.1 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461205.6636,12.89,0.05,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 20260614.1636 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
First image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Last image: 2461205.66384612 14.06.2026 03:55:46.305 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
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: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6885
Objects passed selection criteria: 6868
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 4735.75
Average stars matched: 4640.75 (97.994 %)
Memory usage VmPeak: 113100 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jun 13 23:02:38 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
First image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Last image: 2461205.66384612 14.06.2026 03:55:46.305 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 306
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 14 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): 37501
Objects passed selection criteria: 37405
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 27039.2
Average stars matched: 25721 (95.1247 %)
Memory usage VmPeak: 141068 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jun 13 23:04:21 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461205.66330119
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits exists and is non-empty
Saving wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits to local_wcs_cache/
'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits'
wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits exists and is non-empty
Saving wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits to local_wcs_cache/
'wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits'
wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits exists and is non-empty
Saving wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits'
wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits exists and is non-empty
Saving wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (1st reference image)
verification OK: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:46:31.742 +14:00:33.63 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits (1st new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:37.548 +13:59:45.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:46:31.742 +14:00:33.63
Second-epoch image center 09:46:37.548 +13:59:45.34
Angular distance between the image centers 0.0270 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits (2nd new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:37.920 +14:00:16.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:31.742 +14:00:33.63
Second-epoch image center 09:46:37.920 +14:00:16.24
Angular distance between the image centers 0.0254 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:46:37.548 +13:59:45.34
Second-epoch second image center 09:46:37.920 +14:00:16.24
Angular distance between the image centers 0.00871 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits &> /tmp/tmp.dftf1qYDMh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits &> /tmp/tmp.8EdAuP1xJ4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits &> /tmp/tmp.A40l1xpa7Z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits &> /tmp/tmp.fZ7A26CDgt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Found non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
The reference image (wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits) and catalog (wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat) found
'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat' -> 'wcsmag.cat'
Read 7795 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4789 to 154.9675 deg, Dec +8.5563 to +19.3047 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 138.4789 to 154.9675 deg, Dec 8.5563 to 19.3047 deg
Loaded 4793 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3886 out of 4074 total matches.
Matched with Tycho-2 4074 out of 7795 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.915650
a=0.000000 b=1.000000 c=22.915650
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7795 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4789 to 154.9675 deg, Dec +8.5563 to +19.3047 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 138.4789 to 154.9675 deg, Dec 8.5563 to 19.3047 deg
Loaded 4793 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3886 out of 4074 total matches.
Matched with Tycho-2 4074 out of 7795 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits:
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (aperture=6.6)
Read 7228 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4295 to 155.2660 deg, Dec +8.1771 to +19.5842 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 138.4295 to 155.2660 deg, Dec 8.1771 to 19.5842 deg
Loaded 5215 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3899 out of 4084 total matches.
Matched with Tycho-2 4084 out of 7228 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits:
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
2.1 pix Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
2.6 pix fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
2.6 pix fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
2.4 pix wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
2.1 pix wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Limiting magnitude estimates:
15.3 mag. Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
15.3 mag. Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
13.2 mag. fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
13.0 mag. fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dftf1qYDMh (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=485, passed=7795
Got 7795 stars (including 7304 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
util/solve_plate_with_UCAC5 got 7795 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 906 matched stars entering correct_measured_positions(), 883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 906 matched stars entering correct_measured_positions(), 7515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 906 matched stars entering correct_measured_positions(), 7517 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 906 matched stars entering correct_measured_positions(), 7517 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 906 stars left (next iteration limit 996)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits N_match=906 sigma_overall_arcsec=0.455 sigma_q1_arcsec=0.362 sigma_q2_arcsec=0.579 sigma_q3_arcsec=0.419 sigma_q4_arcsec=0.483 n_q1=277 n_q2=221 n_q3=218 n_q4=190 worst_quadrant_to_overall_ratio=1.272
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -region wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8EdAuP1xJ4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=490, passed=7228
Got 7228 stars (including 6724 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 7228 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 6991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 6991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 6991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits N_match=912 sigma_overall_arcsec=0.309 sigma_q1_arcsec=0.368 sigma_q2_arcsec=0.322 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.291 n_q1=202 n_q2=221 n_q3=206 n_q4=283 worst_quadrant_to_overall_ratio=1.190
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -region wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.A40l1xpa7Z (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=85, passed=2036
Got 2036 stars (including 1949 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat
util/solve_plate_with_UCAC5 got 2036 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 1954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 1955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 1955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 903 stars left (next iteration limit 993)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits N_match=903 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.312 sigma_q2_arcsec=0.425 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.359 n_q1=244 n_q2=259 n_q3=110 n_q4=290 worst_quadrant_to_overall_ratio=1.171
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits -region wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fZ7A26CDgt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=80, passed=2001
Got 2001 stars (including 1918 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat
util/solve_plate_with_UCAC5 got 2001 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 549 (Dec 8.7 to 19.5)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 1931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 549 (Dec 8.7 to 19.5)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 1930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 1929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits N_match=911 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.336 sigma_q2_arcsec=0.359 sigma_q3_arcsec=0.336 sigma_q4_arcsec=0.299 n_q1=205 n_q2=290 n_q3=134 n_q4=282 worst_quadrant_to_overall_ratio=1.092
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits -region wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits sigma_overall=0.455 worst_q_ratio=1.272
ref2=Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits sigma_overall=0.309 worst_q_ratio=1.190
new1=fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits sigma_overall=0.362 worst_q_ratio=1.171
new2=fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits sigma_overall=0.329 worst_q_ratio=1.092
reference average sigma_overall=0.382 worst_q_ratio=1.231
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155_astrometric_residuals.png (906 matched stars from wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138_astrometric_residuals.png (912 matched stars from wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042_astrometric_residuals.png (903 matched stars from wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043_astrometric_residuals.png (911 matched stars from wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-54-59_20.00sec_-0.00C_LIGHTs_0042.fits'
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-04-Q1b1x1_225924_TTUQ1b1x1_3190518_N9NSImpf/wcs_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043.fits'
Preparing the HTML report for the field Leo-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:14:43.83 +10:12:53.5: 9.55 +/- 0.00 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:15:13.38 +09:45:35.3: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:15:16.73 +09:52:19.2: 9.91 +/- 0.00 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:15:09.10 +10:22:56.6: 9.72 +/- 0.00 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:15:16.73 +09:52:19.2: 9.96 +/- 0.00 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:14:43.83 +10:12:53.5: 9.62 +/- 0.00 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:15:13.38 +09:45:35.3: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 09:15:13.38 +09:45:35.3: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:15:09.10 +10:22:56.6: 9.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.58 +/- 0.00
Forced photometry reference-image weighted average: 9.93 +/- 0.00
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter REJECTED candidate at 09:14:43.83 +10:12:53.5: ref_mag=9.58 +/- 0.00 new_mean_mag=10.7422 delta=-1.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:15:16.73 +09:52:19.2: ref_mag=9.93 +/- 0.00 new_mean_mag=10.7414 delta=-0.81 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:15:09.10 +10:22:56.6: ref_mag=9.75 +/- 0.00 new_mean_mag=10.8702 delta=-1.12 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20363_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 20363_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:15:01.45 +12:52:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20364_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 20364_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:35:55.54 +14:22:53.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20366_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 20366_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:15:49.45 +10:22:25.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20368_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 20368_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 20370_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 20370_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 20371_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 20371_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 20372_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 20372_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 07429_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 07429_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:15:01.46 +12:52:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54808_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54808_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:15:49.46 +10:22:25.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 54813_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54813_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54815_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54815_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54816_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54816_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54817_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54817_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54821_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54821_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:15:49.85 +10:13:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54823_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54823_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:16:35.57 +09:29:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54833_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54833_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:18:58.26 +09:25:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54834_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54834_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54836_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54836_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:16:40.21 +09:45:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54838_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54838_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:17:23.43 +09:32:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54841_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54841_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54842_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54842_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:16:16.14 +09:17:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54843_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54843_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54844_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54844_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:15:49.84 +09:18:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54846_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54846_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54851_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54851_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54858_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54858_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54860_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54860_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:15:54.41 +10:05:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54863_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54863_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54865_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54865_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:16:22.30 +09:22:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54867_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54867_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:17:22.92 +09:56:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54869_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54869_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54870_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54870_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54872_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 54872_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 54873_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54873_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54875_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54875_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:16:39.74 +09:31:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54878_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54878_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:18:20.27 +09:32:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54879_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54879_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:18:20.80 +09:45:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54881_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54881_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:16:20.34 +09:34:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54887_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54887_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:17:33.26 +09:23:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54889_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 54889_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 54892_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54892_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:15:35.77 +10:04:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54893_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54893_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54897_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54897_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:17:05.28 +10:07:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54898_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54898_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:15:48.65 +10:05:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54902_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54902_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:18:42.64 +09:28:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54906_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54906_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:17:01.28 +09:59:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54910_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54910_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:16:40.30 +10:04:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54916_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54916_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:40:58.89 +09:52:39.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 54920_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54920_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:16:22.05 +10:19:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54922_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54922_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:16:50.00 +09:46:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54930_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54930_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 54938_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 54938_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54967_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 54967_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 55017_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 55017_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30132_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30132_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29121_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 29121_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28787_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28787_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:12:30.42 +18:09:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29477_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 29477_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34254_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34254_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31696_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 31696_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:12:36.90 +17:35:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09041_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 09041_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34015_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34015_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30799_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30799_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30407_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 30407_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 34592_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 34592_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39463_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 39463_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30527_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30527_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29530_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 29530_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38413_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38413_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32087_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 32087_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:15:11.54 +17:27:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33174_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 33174_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:53.69 +17:13:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28540_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28540_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 35425_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 35425_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32778_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32778_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28204_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28204_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 33331_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 33331_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:52.44 +17:08:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33244_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 33244_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 38010_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38010_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32653_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 32653_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:36.30 +17:22:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28017_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28017_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:16:50.24 +18:20:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31787_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 31787_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32677_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32677_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 27733_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 27733_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:12:19.78 +18:28:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36197_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36197_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 05462_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 05462_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 27487_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 27487_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:25:35.46 +18:49:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31482_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 31482_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28360_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28360_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:02.38 +18:17:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29704_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 29704_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:10.78 +18:01:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03685_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 03685_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32823_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32823_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 00807_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 00807_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31755_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 31755_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38161_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38161_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30386_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30386_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31827_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 31827_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 36439_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36439_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32070_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32070_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 08376_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 08376_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 37853_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 37853_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 33786_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33786_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31095_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 31095_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:53.82 +17:39:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06505_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 06505_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 33106_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33106_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31961_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 31961_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:00.81 +17:31:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30338_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30338_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 02056_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 02056_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 36707_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36707_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 27937_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 27937_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:11:48.22 +18:25:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30016_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30016_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32485_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32485_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31045_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 31045_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:59.36 +17:43:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32522_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 32522_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 31823_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 31823_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30413_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30413_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 03181_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 03181_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31597_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 31597_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 36032_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36032_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 25592_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 25592_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 10027_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 10027_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29526_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 29526_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:39.24 +18:03:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03914_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 03914_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 02935_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 02935_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 37380_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 37380_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32572_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32572_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 25445_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 25445_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34891_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34891_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32519_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32519_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 37975_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 37975_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 07215_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 07215_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28361_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 28361_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34166_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 34166_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:16:37.28 +16:56:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28418_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28418_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:11:40.76 +18:16:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30937_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 30937_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:14.05 +17:44:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30954_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30954_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34169_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34169_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38521_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38521_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34299_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34299_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29631_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 29631_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30508_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 30508_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:50.31 +17:48:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34581_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34581_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38724_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38724_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 36003_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36003_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28796_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 28796_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 27995_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 27995_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:25.04 +18:22:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37661_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 37661_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 32409_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 32409_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:46.34 +17:23:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34118_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34118_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 37359_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 37359_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 33575_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33575_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 35076_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 35076_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 24776_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 24776_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 35079_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 35079_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 36515_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36515_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 05429_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 05429_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:49:58.85 +10:06:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27484_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 27484_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 33653_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33653_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 01902_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 01902_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 33296_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33296_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30492_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 30492_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:05.23 +17:49:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34655_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 34655_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 39454_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 39454_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 27779_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 27779_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:12:04.01 +18:28:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05318_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 05318_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 50425_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 50425_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 37832_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 37832_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29160_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 29160_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 00949_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 00949_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28002_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28002_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:14.54 +18:23:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01071_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 01071_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 07246_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 07246_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29332_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 29332_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:57.33 +18:03:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30381_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 30381_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:39.82 +17:49:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33974_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33974_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31883_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 31883_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 33984_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33984_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32381_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32381_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 33976_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33976_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32185_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32185_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31285_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 31285_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34641_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34641_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32564_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 32564_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 32611_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32611_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32888_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32888_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28203_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 28203_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32495_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32495_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 35416_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 35416_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38620_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38620_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28438_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28438_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 06313_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 06313_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 33066_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33066_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30660_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30660_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28311_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 28311_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38883_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38883_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38398_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38398_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 14178_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 14178_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 36530_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36530_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34445_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34445_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32302_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32302_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38912_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 38912_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 33395_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33395_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29802_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 29802_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 35267_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 35267_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32129_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 32129_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:33.76 +17:26:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37609_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 37609_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 24108_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 24108_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32516_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 32516_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:18.16 +17:24:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27016_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 27016_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 37211_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 37211_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 37101_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 37101_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29949_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 29949_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:15:21.96 +17:53:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34722_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34722_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28288_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 28288_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38180_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38180_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 36741_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36741_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32032_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 32032_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:20.40 +17:30:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05971_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 05971_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34749_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34749_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 06696_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 06696_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 27660_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 27660_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:00.20 +18:29:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33596_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33596_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 36270_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36270_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 27519_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 27519_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:04.35 +18:31:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29239_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 29239_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:17.02 +18:05:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37910_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 37910_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32384_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 32384_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:15:21.45 +17:21:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35841_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 35841_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 36107_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36107_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 39499_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 39499_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38700_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38700_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 40430_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 40430_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 27724_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 27724_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:24:38.12 +18:44:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29632_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 29632_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 38189_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 38189_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30548_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 30548_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 05028_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 05028_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30877_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30877_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 01373_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 01373_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:48:15.60 +09:05:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27853_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 27853_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:57.57 +18:24:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36398_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36398_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28817_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 28817_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32296_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32296_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29284_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 29284_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:53.75 +18:03:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37357_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 37357_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 33593_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33593_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34878_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 34878_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:42.49 +16:49:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04696_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 04696_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32162_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32162_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28494_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28494_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:12:22.82 +18:15:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30003_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30003_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32718_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 32718_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29501_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 29501_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28627_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28627_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:12:52.76 +18:12:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28330_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28330_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:40.12 +18:17:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28785_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28785_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:33.37 +18:09:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28562_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28562_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:04.03 +18:13:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28506_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28506_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:11:35.34 +18:15:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31836_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 31836_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:45.85 +17:31:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33457_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 33457_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 05571_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 05571_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 02171_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 02171_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 04902_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 04902_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31811_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 31811_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 04221_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 04221_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 06560_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 06560_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:50:03.19 +10:23:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36355_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36355_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 29342_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 29342_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 27855_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 27855_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 31458_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 31458_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 35723_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 35723_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 06685_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 06685_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34754_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34754_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 34873_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 34873_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 30787_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 30787_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 32963_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 32963_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:13:03.63 +17:17:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29683_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 29683_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 27821_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 27821_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 28505_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
The candidate 28505_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 10:14:12.57 +18:13:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36380_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 36380_fd_Leo-04-Q1b1x1_2026-06-13_22-55-46_20.00sec_-0.00C_LIGHTs_0043
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 331s
Prepared the HTML report for the field Leo-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:48:37.65 +08:56:43.2
09:48:40.64 +08:58:47.0
09:48:14.61 +09:01:01.4
09:33:46.12 +09:17:39.0
09:34:00.01 +09:20:00.1
09:47:41.35 +09:18:14.3
09:33:15.55 +09:34:04.6
09:31:42.07 +09:38:33.7
09:48:40.57 +09:41:57.1
09:49:32.30 +09:44:49.9
09:32:19.94 +09:53:48.4
09:31:42.89 +10:00:26.2
09:32:20.14 +10:03:48.9
09:32:51.16 +10:05:09.8
09:48:42.64 +10:05:06.2
09:31:40.40 +10:11:05.2
09:31:13.40 +10:13:09.9
09:30:28.33 +10:19:40.6
09:32:43.71 +10:24:01.9
09:31:38.57 +10:27:13.4
09:30:24.00 +10:29:40.8
09:32:44.55 +10:29:47.3
09:29:51.66 +10:38:16.1
09:31:09.14 +10:38:31.8
09:31:13.35 +10:54:31.8
09:48:43.33 +11:00:10.0
09:30:10.15 +11:17:46.8
09:29:05.97 +12:15:26.3
09:35:08.76 +14:36:03.8
09:33:21.24 +14:45:51.7
09:35:13.80 +14:56:21.2
09:34:24.70 +14:58:25.2
09:29:31.01 +18:50:09.5
10:10:41.90 +18:28:48.4
10:10:26.63 +18:28:22.3
10:11:21.87 +18:21:38.7
09:28:42.96 +18:35:22.1
10:09:41.83 +18:20:46.2
10:10:37.73 +18:19:06.0
10:11:39.23 +18:10:23.2
10:08:39.09 +18:12:16.5
10:08:11.07 +18:11:00.1
10:10:25.27 +15:55:01.4
10:09:44.00 +18:06:01.7
09:31:49.58 +16:06:54.1
10:09:14.66 +18:05:49.9
10:10:00.78 +18:03:47.9
10:09:12.68 +18:02:07.5
10:08:46.21 +18:05:18.4
10:10:19.61 +18:00:14.8
10:09:43.06 +17:58:14.6
10:10:49.80 +17:59:38.3
10:05:49.23 +16:23:10.4
10:12:59.58 +16:38:04.5
09:29:58.07 +18:10:51.0
09:28:58.91 +18:09:54.4
10:12:07.19 +17:51:42.3
10:11:43.59 +16:43:01.3
10:09:43.59 +17:50:30.7
10:11:25.30 +17:45:26.5
10:09:14.38 +17:46:55.8
10:10:24.87 +17:46:32.2
10:08:51.14 +16:58:16.7
10:12:57.74 +17:36:06.1
10:10:52.56 +17:37:45.2
10:10:18.77 +17:39:07.8
09:29:25.02 +17:51:57.2
10:10:33.44 +17:35:44.7
10:12:18.53 +17:29:42.2
10:11:42.93 +17:03:10.8
09:26:20.01 +17:50:56.8
10:07:57.58 +17:33:49.5
10:11:22.40 +17:30:48.7
10:09:05.56 +17:31:22.0
10:09:35.76 +17:29:59.4
09:32:40.39 +17:44:38.0
10:09:13.82 +17:30:56.4
10:09:43.05 +17:27:08.1
10:10:03.37 +17:26:02.0
10:10:35.29 +17:26:05.4
10:12:53.82 +17:25:01.6
10:09:14.65 +17:26:54.1
10:07:31.48 +17:23:18.4
10:10:20.06 +17:21:07.8
10:11:10.07 +17:21:23.4
10:12:39.69 +17:21:26.2
10:13:06.84 +17:18:37.6
10:10:37.45 +17:19:13.2
10:07:42.15 +17:21:22.3
10:10:11.60 +17:16:57.6
10:07:21.04 +17:12:47.6
10:12:59.74 +17:07:24.3
10:09:24.22 +17:15:06.0
10:11:24.37 +17:04:19.7
10:10:39.35 +17:06:38.0
10:08:41.58 +17:06:14.2
10:14:18.13 +17:01:09.4
10:09:21.09 +17:09:53.5
10:10:31.89 +17:04:55.3
10:09:10.51 +17:06:33.7
10:12:42.47 +17:03:58.2
10:12:32.91 +17:01:37.5
10:10:52.67 +17:02:59.1
10:12:42.81 +16:58:34.6
10:09:00.33 +17:01:14.6
10:12:07.51 +16:57:04.3
10:09:09.07 +16:58:40.2
10:12:52.06 +16:52:05.9
10:08:46.96 +16:53:45.2
10:10:03.92 +16:54:20.6
10:13:46.76 +16:47:06.6
10:10:24.93 +16:53:23.4
09:29:35.58 +17:06:54.5
10:07:13.34 +16:52:07.8
10:07:57.99 +16:51:13.6
10:12:08.38 +16:44:42.2
10:13:30.26 +16:43:04.6
10:08:34.97 +16:41:25.2
09:36:12.89 +15:24:11.5
09:32:49.20 +15:25:18.6
10:10:43.04 +16:37:11.4
10:11:17.93 +16:25:16.0
09:29:09.18 +16:49:15.9
10:10:10.89 +16:33:40.8
10:12:27.87 +16:27:45.6
10:09:25.01 +16:30:57.3
10:11:15.98 +16:30:21.8
10:08:30.48 +16:31:16.1
10:10:51.08 +16:30:39.8
09:28:03.79 +16:44:23.6
09:35:33.71 +15:27:17.3
10:07:46.14 +16:28:19.3
09:31:48.57 +15:27:27.0
09:32:12.65 +16:39:56.5
10:11:01.97 +16:14:39.9
10:10:33.94 +16:16:03.3
10:10:50.87 +16:15:08.1
09:30:17.48 +16:29:37.2
10:11:33.26 +16:11:36.7
09:30:03.58 +16:22:58.2
10:08:49.99 +16:08:45.2
09:32:22.82 +16:20:24.4
10:08:23.11 +16:07:47.4
10:10:29.84 +16:05:00.4
09:24:22.65 +16:19:53.7
09:30:32.98 +16:15:39.2
10:09:15.52 +16:02:10.0
09:29:30.01 +16:17:37.4
10:10:00.35 +16:00:15.9
10:07:32.34 +16:01:55.1
09:29:42.76 +16:12:40.2
10:07:05.61 +15:56:35.5
09:31:17.58 +16:11:51.7
10:10:25.64 +15:53:48.8
10:08:38.77 +15:50:31.2
10:07:56.10 +15:40:49.4
10:09:16.57 +15:42:59.3
09:30:57.82 +15:54:50.3
09:31:31.92 +15:40:20.7
09:59:01.05 +14:36:16.5
09:24:05.66 +17:00:58.8
09:34:19.79 +15:54:01.5
09:42:33.04 +10:07:03.6
########### Completed Leo-04-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 ####
09:59:01.05 +14:36:16.5
09:24:05.66 +17:00:58.8
09:34:19.79 +15:54:01.5
09:42:33.04 +10:07:03.6
10:05:49.23 +16:23:10.4
10:08:11.07 +18:11:00.1
10:09:44.00 +18:06:01.7
10:09:00.33 +17:01:14.6
09:48:43.33 +11:00:10.0
10:12:32.91 +17:01:37.5
10:11:25.30 +17:45:26.5
10:09:16.57 +15:42:59.3
10:12:07.19 +17:51:42.3
10:09:14.66 +18:05:49.9
10:07:32.34 +16:01:55.1
09:36:12.89 +15:24:11.5
10:12:39.69 +17:21:26.2
09:24:22.65 +16:19:53.7
10:10:33.44 +17:35:44.7
10:10:20.06 +17:21:07.8
10:12:27.87 +16:27:45.6
09:31:40.40 +10:11:05.2
10:10:52.56 +17:37:45.2
09:48:40.57 +09:41:57.1
10:13:06.84 +17:18:37.6
09:48:37.65 +08:56:43.2
09:29:25.02 +17:51:57.2
09:30:32.98 +16:15:39.2
09:29:58.07 +18:10:51.0
09:26:20.01 +17:50:56.8
09:28:03.79 +16:44:23.6
10:11:22.40 +17:30:48.7
09:31:13.35 +10:54:31.8
09:32:22.82 +16:20:24.4
10:09:21.09 +17:09:53.5
09:31:38.57 +10:27:13.4
10:10:11.60 +17:16:57.6
10:12:59.58 +16:38:04.5
09:34:00.01 +09:20:00.1
09:31:48.57 +15:27:27.0
10:10:49.80 +17:59:38.3
10:10:03.37 +17:26:02.0
10:11:42.93 +17:03:10.8
09:28:58.91 +18:09:54.4
09:31:42.07 +09:38:33.7
10:10:18.77 +17:39:07.8
09:29:09.18 +16:49:15.9
09:34:24.70 +14:58:25.2
09:30:10.15 +11:17:46.8
09:49:32.30 +09:44:49.9
09:33:15.55 +09:34:04.6
10:11:33.26 +16:11:36.7
10:09:14.65 +17:26:54.1
09:35:13.80 +14:56:21.2
10:07:13.34 +16:52:07.8
10:12:53.82 +17:25:01.6
10:10:29.84 +16:05:00.4
09:29:51.66 +10:38:16.1
10:10:37.73 +18:19:06.0
10:10:24.87 +17:46:32.2
10:12:42.81 +16:58:34.6
09:29:42.76 +16:12:40.2
10:12:07.51 +16:57:04.3
10:10:00.78 +18:03:47.9
10:12:52.06 +16:52:05.9
10:10:25.64 +15:53:48.8
10:11:17.93 +16:25:16.0
10:11:39.23 +18:10:23.2
10:10:52.67 +17:02:59.1
09:30:17.48 +16:29:37.2
10:11:24.37 +17:04:19.7
10:07:57.99 +16:51:13.6
09:33:21.24 +14:45:51.7
10:12:08.38 +16:44:42.2
09:35:33.71 +15:27:17.3
09:29:31.01 +18:50:09.5
10:14:18.13 +17:01:09.4
09:33:46.12 +09:17:39.0
10:07:21.04 +17:12:47.6
10:07:56.10 +15:40:49.4
09:48:42.64 +10:05:06.2
10:08:49.99 +16:08:45.2
10:10:25.27 +15:55:01.4
09:48:40.64 +08:58:47.0
09:48:14.61 +09:01:01.4
09:31:09.14 +10:38:31.8
10:10:31.89 +17:04:55.3
10:07:57.58 +17:33:49.5
10:12:42.47 +17:03:58.2
10:09:43.05 +17:27:08.1
10:09:10.51 +17:06:33.7
10:09:35.76 +17:29:59.4
10:08:51.14 +16:58:16.7
10:08:46.96 +16:53:45.2
10:07:31.48 +17:23:18.4
10:10:37.45 +17:19:13.2
10:11:21.87 +18:21:38.7
10:10:35.29 +17:26:05.4
10:08:34.97 +16:41:25.2
10:07:05.61 +15:56:35.5
09:32:43.71 +10:24:01.9
10:07:42.15 +17:21:22.3
10:11:43.59 +16:43:01.3
10:09:41.83 +18:20:46.2
10:08:38.77 +15:50:31.2
10:10:00.35 +16:00:15.9
09:29:05.97 +12:15:26.3
10:07:46.14 +16:28:19.3
10:09:09.07 +16:58:40.2
10:09:13.82 +17:30:56.4
10:12:59.74 +17:07:24.3
10:10:19.61 +18:00:14.8
10:13:30.26 +16:43:04.6
09:30:03.58 +16:22:58.2
09:35:08.76 +14:36:03.8
10:10:33.94 +16:16:03.3
10:11:01.97 +16:14:39.9
10:10:03.92 +16:54:20.6
09:28:42.96 +18:35:22.1
10:09:15.52 +16:02:10.0
09:32:12.65 +16:39:56.5
09:30:28.33 +10:19:40.6
10:13:46.76 +16:47:06.6
09:32:44.55 +10:29:47.3
10:08:41.58 +17:06:14.2
10:09:25.01 +16:30:57.3
10:08:23.11 +16:07:47.4
10:10:43.04 +16:37:11.4
10:10:10.89 +16:33:40.8
09:30:57.82 +15:54:50.3
09:31:17.58 +16:11:51.7
09:31:31.92 +15:40:20.7
10:09:12.68 +18:02:07.5
09:29:30.01 +16:17:37.4
09:32:51.16 +10:05:09.8
10:09:14.38 +17:46:55.8
10:10:51.08 +16:30:39.8
10:08:39.09 +18:12:16.5
09:32:40.39 +17:44:38.0
10:10:50.87 +16:15:08.1
10:10:39.35 +17:06:38.0
09:31:42.89 +10:00:26.2
10:09:05.56 +17:31:22.0
10:09:43.06 +17:58:14.6
10:11:10.07 +17:21:23.4
09:31:49.58 +16:06:54.1
10:09:24.22 +17:15:06.0
09:31:13.40 +10:13:09.9
09:47:41.35 +09:18:14.3
09:32:20.14 +10:03:48.9
10:12:18.53 +17:29:42.2
09:32:19.94 +09:53:48.4
10:11:15.98 +16:30:21.8
10:10:26.63 +18:28:22.3
10:12:57.74 +17:36:06.1
09:32:49.20 +15:25:18.6
09:30:24.00 +10:29:40.8
10:10:24.93 +16:53:23.4
09:29:35.58 +17:06:54.5
10:09:43.59 +17:50:30.7
10:08:46.21 +18:05:18.4
10:10:41.90 +18:28:48.4
10:08:30.48 +16:31:16.1
###################################################################################
09:59:01.05 +14:36:16.5 -- asteroid (will NOT add it to exclusion list)
09:24:05.66 +17:00:58.8 -- asteroid (will NOT add it to exclusion list)
09:34:19.79 +15:54:01.5 -- asteroid (will NOT add it to exclusion list)
09:42:33.04 +10:07:03.6 -- not an asteroid (will add it to exclusion list)
10:05:49.23 +16:23:10.4 -- not an asteroid (will add it to exclusion list)
10:08:11.07 +18:11:00.1 -- not an asteroid (will add it to exclusion list)
10:09:44.00 +18:06:01.7 -- not an asteroid (will add it to exclusion list)
10:09:00.33 +17:01:14.6 -- not an asteroid (will add it to exclusion list)
09:48:43.33 +11:00:10.0 -- not an asteroid (will add it to exclusion list)
10:12:32.91 +17:01:37.5 -- not an asteroid (will add it to exclusion list)
10:11:25.30 +17:45:26.5 -- not an asteroid (will add it to exclusion list)
10:09:16.57 +15:42:59.3 -- not an asteroid (will add it to exclusion list)
10:12:07.19 +17:51:42.3 -- not an asteroid (will add it to exclusion list)
10:09:14.66 +18:05:49.9 -- not an asteroid (will add it to exclusion list)
10:07:32.34 +16:01:55.1 -- not an asteroid (will add it to exclusion list)
09:36:12.89 +15:24:11.5 -- not an asteroid (will add it to exclusion list)
10:12:39.69 +17:21:26.2 -- not an asteroid (will add it to exclusion list)
09:24:22.65 +16:19:53.7 -- not an asteroid (will add it to exclusion list)
10:10:33.44 +17:35:44.7 -- not an asteroid (will add it to exclusion list)
10:10:20.06 +17:21:07.8 -- not an asteroid (will add it to exclusion list)
10:12:27.87 +16:27:45.6 -- not an asteroid (will add it to exclusion list)
09:31:40.40 +10:11:05.2 -- not an asteroid (will add it to exclusion list)
10:10:52.56 +17:37:45.2 -- not an asteroid (will add it to exclusion list)
09:48:40.57 +09:41:57.1 -- not an asteroid (will add it to exclusion list)
10:13:06.84 +17:18:37.6 -- not an asteroid (will add it to exclusion list)
09:48:37.65 +08:56:43.2 -- not an asteroid (will add it to exclusion list)
09:29:25.02 +17:51:57.2 -- not an asteroid (will add it to exclusion list)
09:30:32.98 +16:15:39.2 -- not an asteroid (will add it to exclusion list)
09:29:58.07 +18:10:51.0 -- not an asteroid (will add it to exclusion list)
09:26:20.01 +17:50:56.8 -- not an asteroid (will add it to exclusion list)
09:28:03.79 +16:44:23.6 -- not an asteroid (will add it to exclusion list)
10:11:22.40 +17:30:48.7 -- not an asteroid (will add it to exclusion list)
09:31:13.35 +10:54:31.8 -- not an asteroid (will add it to exclusion list)
09:32:22.82 +16:20:24.4 -- not an asteroid (will add it to exclusion list)
10:09:21.09 +17:09:53.5 -- not an asteroid (will add it to exclusion list)
09:31:38.57 +10:27:13.4 -- not an asteroid (will add it to exclusion list)
10:10:11.60 +17:16:57.6 -- not an asteroid (will add it to exclusion list)
10:12:59.58 +16:38:04.5 -- not an asteroid (will add it to exclusion list)
09:34:00.01 +09:20:00.1 -- not an asteroid (will add it to exclusion list)
09:31:48.57 +15:27:27.0 -- not an asteroid (will add it to exclusion list)
10:10:49.80 +17:59:38.3 -- not an asteroid (will add it to exclusion list)
10:10:03.37 +17:26:02.0 -- not an asteroid (will add it to exclusion list)
10:11:42.93 +17:03:10.8 -- not an asteroid (will add it to exclusion list)
09:28:58.91 +18:09:54.4 -- not an asteroid (will add it to exclusion list)
09:31:42.07 +09:38:33.7 -- not an asteroid (will add it to exclusion list)
10:10:18.77 +17:39:07.8 -- not an asteroid (will add it to exclusion list)
09:29:09.18 +16:49:15.9 -- not an asteroid (will add it to exclusion list)
09:34:24.70 +14:58:25.2 -- not an asteroid (will add it to exclusion list)
09:30:10.15 +11:17:46.8 -- not an asteroid (will add it to exclusion list)
09:49:32.30 +09:44:49.9 -- not an asteroid (will add it to exclusion list)
09:33:15.55 +09:34:04.6 -- not an asteroid (will add it to exclusion list)
10:11:33.26 +16:11:36.7 -- not an asteroid (will add it to exclusion list)
10:09:14.65 +17:26:54.1 -- not an asteroid (will add it to exclusion list)
09:35:13.80 +14:56:21.2 -- not an asteroid (will add it to exclusion list)
10:07:13.34 +16:52:07.8 -- not an asteroid (will add it to exclusion list)
10:12:53.82 +17:25:01.6 -- not an asteroid (will add it to exclusion list)
10:10:29.84 +16:05:00.4 -- not an asteroid (will add it to exclusion list)
09:29:51.66 +10:38:16.1 -- not an asteroid (will add it to exclusion list)
10:10:37.73 +18:19:06.0 -- not an asteroid (will add it to exclusion list)
10:10:24.87 +17:46:32.2 -- not an asteroid (will add it to exclusion list)
10:12:42.81 +16:58:34.6 -- not an asteroid (will add it to exclusion list)
09:29:42.76 +16:12:40.2 -- not an asteroid (will add it to exclusion list)
10:12:07.51 +16:57:04.3 -- not an asteroid (will add it to exclusion list)
10:10:00.78 +18:03:47.9 -- not an asteroid (will add it to exclusion list)
10:12:52.06 +16:52:05.9 -- not an asteroid (will add it to exclusion list)
10:10:25.64 +15:53:48.8 -- not an asteroid (will add it to exclusion list)
10:11:17.93 +16:25:16.0 -- not an asteroid (will add it to exclusion list)
10:11:39.23 +18:10:23.2 -- not an asteroid (will add it to exclusion list)
10:10:52.67 +17:02:59.1 -- not an asteroid (will add it to exclusion list)
09:30:17.48 +16:29:37.2 -- not an asteroid (will add it to exclusion list)
10:11:24.37 +17:04:19.7 -- not an asteroid (will add it to exclusion list)
10:07:57.99 +16:51:13.6 -- not an asteroid (will add it to exclusion list)
09:33:21.24 +14:45:51.7 -- asteroid (will NOT add it to exclusion list)
10:12:08.38 +16:44:42.2 -- not an asteroid (will add it to exclusion list)
09:35:33.71 +15:27:17.3 -- not an asteroid (will add it to exclusion list)
09:29:31.01 +18:50:09.5 -- not an asteroid (will add it to exclusion list)
10:14:18.13 +17:01:09.4 -- not an asteroid (will add it to exclusion list)
09:33:46.12 +09:17:39.0 -- not an asteroid (will add it to exclusion list)
10:07:21.04 +17:12:47.6 -- not an asteroid (will add it to exclusion list)
10:07:56.10 +15:40:49.4 -- not an asteroid (will add it to exclusion list)
09:48:42.64 +10:05:06.2 -- not an asteroid (will add it to exclusion list)
10:08:49.99 +16:08:45.2 -- not an asteroid (will add it to exclusion list)
10:10:25.27 +15:55:01.4 -- not an asteroid (will add it to exclusion list)
09:48:40.64 +08:58:47.0 -- not an asteroid (will add it to exclusion list)
09:48:14.61 +09:01:01.4 -- not an asteroid (will add it to exclusion list)
09:31:09.14 +10:38:31.8 -- not an asteroid (will add it to exclusion list)
10:10:31.89 +17:04:55.3 -- not an asteroid (will add it to exclusion list)
10:07:57.58 +17:33:49.5 -- not an asteroid (will add it to exclusion list)
10:12:42.47 +17:03:58.2 -- not an asteroid (will add it to exclusion list)
10:09:43.05 +17:27:08.1 -- not an asteroid (will add it to exclusion list)
10:09:10.51 +17:06:33.7 -- not an asteroid (will add it to exclusion list)
10:09:35.76 +17:29:59.4 -- not an asteroid (will add it to exclusion list)
10:08:51.14 +16:58:16.7 -- not an asteroid (will add it to exclusion list)
10:08:46.96 +16:53:45.2 -- not an asteroid (will add it to exclusion list)
10:07:31.48 +17:23:18.4 -- not an asteroid (will add it to exclusion list)
10:10:37.45 +17:19:13.2 -- not an asteroid (will add it to exclusion list)
10:11:21.87 +18:21:38.7 -- not an asteroid (will add it to exclusion list)
10:10:35.29 +17:26:05.4 -- not an asteroid (will add it to exclusion list)
10:08:34.97 +16:41:25.2 -- not an asteroid (will add it to exclusion list)
10:07:05.61 +15:56:35.5 -- not an asteroid (will add it to exclusion list)
09:32:43.71 +10:24:01.9 -- not an asteroid (will add it to exclusion list)
10:07:42.15 +17:21:22.3 -- not an asteroid (will add it to exclusion list)
10:11:43.59 +16:43:01.3 -- not an asteroid (will add it to exclusion list)
10:09:41.83 +18:20:46.2 -- not an asteroid (will add it to exclusion list)
10:08:38.77 +15:50:31.2 -- not an asteroid (will add it to exclusion list)
10:10:00.35 +16:00:15.9 -- not an asteroid (will add it to exclusion list)
09:29:05.97 +12:15:26.3 -- not an asteroid (will add it to exclusion list)
10:07:46.14 +16:28:19.3 -- not an asteroid (will add it to exclusion list)
10:09:09.07 +16:58:40.2 -- not an asteroid (will add it to exclusion list)
10:09:13.82 +17:30:56.4 -- not an asteroid (will add it to exclusion list)
10:12:59.74 +17:07:24.3 -- not an asteroid (will add it to exclusion list)
10:10:19.61 +18:00:14.8 -- not an asteroid (will add it to exclusion list)
10:13:30.26 +16:43:04.6 -- not an asteroid (will add it to exclusion list)
09:30:03.58 +16:22:58.2 -- not an asteroid (will add it to exclusion list)
09:35:08.76 +14:36:03.8 -- not an asteroid (will add it to exclusion list)
10:10:33.94 +16:16:03.3 -- not an asteroid (will add it to exclusion list)
10:11:01.97 +16:14:39.9 -- not an asteroid (will add it to exclusion list)
10:10:03.92 +16:54:20.6 -- not an asteroid (will add it to exclusion list)
09:28:42.96 +18:35:22.1 -- not an asteroid (will add it to exclusion list)
10:09:15.52 +16:02:10.0 -- not an asteroid (will add it to exclusion list)
09:32:12.65 +16:39:56.5 -- not an asteroid (will add it to exclusion list)
09:30:28.33 +10:19:40.6 -- not an asteroid (will add it to exclusion list)
10:13:46.76 +16:47:06.6 -- not an asteroid (will add it to exclusion list)
09:32:44.55 +10:29:47.3 -- not an asteroid (will add it to exclusion list)
10:08:41.58 +17:06:14.2 -- not an asteroid (will add it to exclusion list)
10:09:25.01 +16:30:57.3 -- not an asteroid (will add it to exclusion list)
10:08:23.11 +16:07:47.4 -- not an asteroid (will add it to exclusion list)
10:10:43.04 +16:37:11.4 -- not an asteroid (will add it to exclusion list)
10:10:10.89 +16:33:40.8 -- not an asteroid (will add it to exclusion list)
09:30:57.82 +15:54:50.3 -- not an asteroid (will add it to exclusion list)
09:31:17.58 +16:11:51.7 -- not an asteroid (will add it to exclusion list)
09:31:31.92 +15:40:20.7 -- not an asteroid (will add it to exclusion list)
10:09:12.68 +18:02:07.5 -- not an asteroid (will add it to exclusion list)
09:29:30.01 +16:17:37.4 -- not an asteroid (will add it to exclusion list)
09:32:51.16 +10:05:09.8 -- not an asteroid (will add it to exclusion list)
10:09:14.38 +17:46:55.8 -- not an asteroid (will add it to exclusion list)
10:10:51.08 +16:30:39.8 -- not an asteroid (will add it to exclusion list)
10:08:39.09 +18:12:16.5 -- not an asteroid (will add it to exclusion list)
09:32:40.39 +17:44:38.0 -- not an asteroid (will add it to exclusion list)
10:10:50.87 +16:15:08.1 -- not an asteroid (will add it to exclusion list)
10:10:39.35 +17:06:38.0 -- not an asteroid (will add it to exclusion list)
09:31:42.89 +10:00:26.2 -- not an asteroid (will add it to exclusion list)
10:09:05.56 +17:31:22.0 -- not an asteroid (will add it to exclusion list)
10:09:43.06 +17:58:14.6 -- not an asteroid (will add it to exclusion list)
10:11:10.07 +17:21:23.4 -- not an asteroid (will add it to exclusion list)
09:31:49.58 +16:06:54.1 -- not an asteroid (will add it to exclusion list)
10:09:24.22 +17:15:06.0 -- not an asteroid (will add it to exclusion list)
09:31:13.40 +10:13:09.9 -- not an asteroid (will add it to exclusion list)
09:47:41.35 +09:18:14.3 -- not an asteroid (will add it to exclusion list)
09:32:20.14 +10:03:48.9 -- not an asteroid (will add it to exclusion list)
10:12:18.53 +17:29:42.2 -- not an asteroid (will add it to exclusion list)
09:32:19.94 +09:53:48.4 -- not an asteroid (will add it to exclusion list)
10:11:15.98 +16:30:21.8 -- not an asteroid (will add it to exclusion list)
10:10:26.63 +18:28:22.3 -- not an asteroid (will add it to exclusion list)
10:12:57.74 +17:36:06.1 -- not an asteroid (will add it to exclusion list)
09:32:49.20 +15:25:18.6 -- not an asteroid (will add it to exclusion list)
09:30:24.00 +10:29:40.8 -- not an asteroid (will add it to exclusion list)
10:10:24.93 +16:53:23.4 -- not an asteroid (will add it to exclusion list)
09:29:35.58 +17:06:54.5 -- not an asteroid (will add it to exclusion list)
10:09:43.59 +17:50:30.7 -- not an asteroid (will add it to exclusion list)
10:08:46.21 +18:05:18.4 -- not an asteroid (will add it to exclusion list)
10:10:41.90 +18:28:48.4 -- not an asteroid (will add it to exclusion list)
10:08:30.48 +16:31:16.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
09:24:22.65 +16:19:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:26:20.01 +17:50:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:28:03.79 +16:44:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:28:42.96 +18:35:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:28:58.91 +18:09:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:05.97 +12:15:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:09.18 +16:49:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:25.02 +17:51:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:30.01 +16:17:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:31.01 +18:50:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:35.58 +17:06:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:42.76 +16:12:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:51.66 +10:38:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:58.07 +18:10:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:30:03.58 +16:22:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:30:10.15 +11:17:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:30:17.48 +16:29:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:30:24.00 +10:29:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:30:28.33 +10:19:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:30:32.98 +16:15:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:30:57.82 +15:54:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:09.14 +10:38:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:13.35 +10:54:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:13.40 +10:13:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:17.58 +16:11:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:31.92 +15:40:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:38.57 +10:27:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:40.40 +10:11:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:42.07 +09:38:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:42.89 +10:00:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:48.57 +15:27:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:49.58 +16:06:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:32:12.65 +16:39:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:32:19.94 +09:53:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:32:20.14 +10:03:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:32:22.82 +16:20:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:32:40.39 +17:44:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:32:43.71 +10:24:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:32:44.55 +10:29:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:32:49.20 +15:25:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:32:51.16 +10:05:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:33:15.55 +09:34:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:33:46.12 +09:17:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:34:00.01 +09:20:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:34:24.70 +14:58:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:35:08.76 +14:36:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:35:13.80 +14:56:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:35:33.71 +15:27:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:36:12.89 +15:24:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:42:33.04 +10:07:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:47:41.35 +09:18:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:14.61 +09:01:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:37.65 +08:56:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:40.57 +09:41:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:40.64 +08:58:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:42.64 +10:05:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:43.33 +11:00:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:49:32.30 +09:44:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:05:49.23 +16:23:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:05.61 +15:56:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:13.34 +16:52:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:21.04 +17:12:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:31.48 +17:23:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:32.34 +16:01:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:42.15 +17:21:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:46.14 +16:28:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:56.10 +15:40:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:57.58 +17:33:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:57.99 +16:51:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:11.07 +18:11:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:23.11 +16:07:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:30.48 +16:31:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:34.97 +16:41:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:38.77 +15:50:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:39.09 +18:12:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:41.58 +17:06:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:46.21 +18:05:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:46.96 +16:53:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:49.99 +16:08:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:51.14 +16:58:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:00.33 +17:01:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:05.56 +17:31:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:09.07 +16:58:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:10.51 +17:06:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:12.68 +18:02:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:13.82 +17:30:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:14.38 +17:46:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:14.65 +17:26:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:14.66 +18:05:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:15.52 +16:02:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:16.57 +15:42:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:21.09 +17:09:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:24.22 +17:15:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:25.01 +16:30:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:35.76 +17:29:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:41.83 +18:20:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:43.05 +17:27:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:43.06 +17:58:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:43.59 +17:50:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:44.00 +18:06:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:00.35 +16:00:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:00.78 +18:03:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:03.37 +17:26:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:03.92 +16:54:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:10.89 +16:33:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:11.60 +17:16:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:18.77 +17:39:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:19.61 +18:00:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:20.06 +17:21:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:24.87 +17:46:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:24.93 +16:53:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:25.27 +15:55:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:25.64 +15:53:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:26.63 +18:28:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:29.84 +16:05:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:31.89 +17:04:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:33.44 +17:35:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:33.94 +16:16:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:35.29 +17:26:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:37.45 +17:19:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:37.73 +18:19:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:39.35 +17:06:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:41.90 +18:28:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:43.04 +16:37:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:49.80 +17:59:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:50.87 +16:15:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:51.08 +16:30:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:52.56 +17:37:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:52.67 +17:02:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:01.97 +16:14:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:10.07 +17:21:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:15.98 +16:30:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:17.93 +16:25:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:21.87 +18:21:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:22.40 +17:30:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:24.37 +17:04:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:25.30 +17:45:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:33.26 +16:11:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:39.23 +18:10:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:42.93 +17:03:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:43.59 +16:43:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:07.19 +17:51:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:07.51 +16:57:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:08.38 +16:44:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:18.53 +17:29:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:27.87 +16:27:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:32.91 +17:01:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:39.69 +17:21:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:42.47 +17:03:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:42.81 +16:58:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:52.06 +16:52:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:53.82 +17:25:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:57.74 +17:36:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:59.58 +16:38:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:59.74 +17:07:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:13:06.84 +17:18:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:13:30.26 +16:43:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:13:46.76 +16:47:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:14:18.13 +17:01:09.4 -- 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)
09:24:22.65 +16:19:53.7 -- not a known variable star
09:26:20.01 +17:50:56.8 -- not a known variable star
09:28:03.79 +16:44:23.6 -- not a known variable star
09:28:42.96 +18:35:22.1 -- a known variable star
09:28:58.91 +18:09:54.4 -- not a known variable star
09:29:05.97 +12:15:26.3 -- not a known variable star
09:29:09.18 +16:49:15.9 -- not a known variable star
09:29:25.02 +17:51:57.2 -- not a known variable star
09:29:30.01 +16:17:37.4 -- not a known variable star
09:29:31.01 +18:50:09.5 -- not a known variable star
09:29:35.58 +17:06:54.5 -- not a known variable star
09:29:42.76 +16:12:40.2 -- a known variable star
09:29:51.66 +10:38:16.1 -- not a known variable star
09:29:58.07 +18:10:51.0 -- not a known variable star
09:30:03.58 +16:22:58.2 -- not a known variable star
09:30:10.15 +11:17:46.8 -- a known variable star
09:30:17.48 +16:29:37.2 -- not a known variable star
09:30:24.00 +10:29:40.8 -- not a known variable star
09:30:28.33 +10:19:40.6 -- not a known variable star
09:30:32.98 +16:15:39.2 -- a known variable star
09:30:57.82 +15:54:50.3 -- not a known variable star
09:31:09.14 +10:38:31.8 -- not a known variable star
09:31:13.35 +10:54:31.8 -- not a known variable star
09:31:13.40 +10:13:09.9 -- not a known variable star
09:31:17.58 +16:11:51.7 -- not a known variable star
09:31:31.92 +15:40:20.7 -- not a known variable star
09:31:38.57 +10:27:13.4 -- not a known variable star
09:31:40.40 +10:11:05.2 -- not a known variable star
09:31:42.07 +09:38:33.7 -- not a known variable star
09:31:42.89 +10:00:26.2 -- not a known variable star
09:31:48.57 +15:27:27.0 -- not a known variable star
09:31:49.58 +16:06:54.1 -- not a known variable star
09:32:12.65 +16:39:56.5 -- not a known variable star
09:32:19.94 +09:53:48.4 -- a known variable star
09:32:20.14 +10:03:48.9 -- not a known variable star
09:32:22.82 +16:20:24.4 -- not a known variable star
09:32:40.39 +17:44:38.0 -- not a known variable star
09:32:43.71 +10:24:01.9 -- not a known variable star
09:32:44.55 +10:29:47.3 -- not a known variable star
09:32:49.20 +15:25:18.6 -- not a known variable star
09:32:51.16 +10:05:09.8 -- not a known variable star
09:33:15.55 +09:34:04.6 -- not a known variable star
09:33:46.12 +09:17:39.0 -- not a known variable star
09:34:00.01 +09:20:00.1 -- not a known variable star
09:34:24.70 +14:58:25.2 -- not a known variable star
09:35:08.76 +14:36:03.8 -- a known variable star
09:35:13.80 +14:56:21.2 -- not a known variable star
09:35:33.71 +15:27:17.3 -- not a known variable star
09:36:12.89 +15:24:11.5 -- not a known variable star
09:42:33.04 +10:07:03.6 -- not a known variable star
09:47:41.35 +09:18:14.3 -- not a known variable star
09:48:14.61 +09:01:01.4 -- not a known variable star
09:48:37.65 +08:56:43.2 -- not a known variable star
09:48:40.57 +09:41:57.1 -- a known variable star
09:48:40.64 +08:58:47.0 -- not a known variable star
09:48:42.64 +10:05:06.2 -- not a known variable star
09:48:43.33 +11:00:10.0 -- not a known variable star
09:49:32.30 +09:44:49.9 -- not a known variable star
10:05:49.23 +16:23:10.4 -- not a known variable star
10:07:05.61 +15:56:35.5 -- not a known variable star
10:07:13.34 +16:52:07.8 -- not a known variable star
10:07:21.04 +17:12:47.6 -- not a known variable star
10:07:31.48 +17:23:18.4 -- not a known variable star
10:07:32.34 +16:01:55.1 -- not a known variable star
10:07:42.15 +17:21:22.3 -- not a known variable star
10:07:46.14 +16:28:19.3 -- not a known variable star
10:07:56.10 +15:40:49.4 -- not a known variable star
10:07:57.58 +17:33:49.5 -- not a known variable star
10:07:57.99 +16:51:13.6 -- not a known variable star
10:08:11.07 +18:11:00.1 -- not a known variable star
10:08:23.11 +16:07:47.4 -- not a known variable star
10:08:30.48 +16:31:16.1 -- not a known variable star
10:08:34.97 +16:41:25.2 -- not a known variable star
10:08:38.77 +15:50:31.2 -- not a known variable star
10:08:39.09 +18:12:16.5 -- not a known variable star
10:08:41.58 +17:06:14.2 -- not a known variable star
10:08:46.21 +18:05:18.4 -- not a known variable star
10:08:46.96 +16:53:45.2 -- not a known variable star
10:08:49.99 +16:08:45.2 -- a known variable star
10:08:51.14 +16:58:16.7 -- not a known variable star
10:09:00.33 +17:01:14.6 -- a known variable star
10:09:05.56 +17:31:22.0 -- not a known variable star
10:09:09.07 +16:58:40.2 -- not a known variable star
10:09:10.51 +17:06:33.7 -- not a known variable star
10:09:12.68 +18:02:07.5 -- not a known variable star
10:09:13.82 +17:30:56.4 -- not a known variable star
10:09:14.38 +17:46:55.8 -- not a known variable star
10:09:14.65 +17:26:54.1 -- not a known variable star
10:09:14.66 +18:05:49.9 -- not a known variable star
10:09:15.52 +16:02:10.0 -- not a known variable star
10:09:16.57 +15:42:59.3 -- not a known variable star
10:09:21.09 +17:09:53.5 -- not a known variable star
10:09:24.22 +17:15:06.0 -- not a known variable star
10:09:25.01 +16:30:57.3 -- not a known variable star
10:09:35.76 +17:29:59.4 -- not a known variable star
10:09:41.83 +18:20:46.2 -- not a known variable star
10:09:43.05 +17:27:08.1 -- not a known variable star
10:09:43.06 +17:58:14.6 -- not a known variable star
10:09:43.59 +17:50:30.7 -- not a known variable star
10:09:44.00 +18:06:01.7 -- not a known variable star
10:10:00.35 +16:00:15.9 -- not a known variable star
10:10:00.78 +18:03:47.9 -- not a known variable star
10:10:03.37 +17:26:02.0 -- a known variable star
10:10:03.92 +16:54:20.6 -- not a known variable star
10:10:10.89 +16:33:40.8 -- not a known variable star
10:10:11.60 +17:16:57.6 -- not a known variable star
10:10:18.77 +17:39:07.8 -- not a known variable star
10:10:19.61 +18:00:14.8 -- not a known variable star
10:10:20.06 +17:21:07.8 -- not a known variable star
10:10:24.87 +17:46:32.2 -- not a known variable star
10:10:24.93 +16:53:23.4 -- not a known variable star
10:10:25.27 +15:55:01.4 -- not a known variable star
10:10:25.64 +15:53:48.8 -- not a known variable star
10:10:26.63 +18:28:22.3 -- not a known variable star
10:10:29.84 +16:05:00.4 -- a known variable star
10:10:31.89 +17:04:55.3 -- not a known variable star
10:10:33.44 +17:35:44.7 -- a known variable star
10:10:33.94 +16:16:03.3 -- not a known variable star
10:10:35.29 +17:26:05.4 -- a known variable star
10:10:37.45 +17:19:13.2 -- not a known variable star
10:10:37.73 +18:19:06.0 -- not a known variable star
10:10:39.35 +17:06:38.0 -- not a known variable star
10:10:41.90 +18:28:48.4 -- not a known variable star
10:10:43.04 +16:37:11.4 -- not a known variable star
10:10:49.80 +17:59:38.3 -- not a known variable star
10:10:50.87 +16:15:08.1 -- not a known variable star
10:10:51.08 +16:30:39.8 -- not a known variable star
10:10:52.56 +17:37:45.2 -- not a known variable star
10:10:52.67 +17:02:59.1 -- not a known variable star
10:11:01.97 +16:14:39.9 -- not a known variable star
10:11:10.07 +17:21:23.4 -- not a known variable star
10:11:15.98 +16:30:21.8 -- not a known variable star
10:11:17.93 +16:25:16.0 -- not a known variable star
10:11:21.87 +18:21:38.7 -- not a known variable star
10:11:22.40 +17:30:48.7 -- not a known variable star
10:11:24.37 +17:04:19.7 -- not a known variable star
10:11:25.30 +17:45:26.5 -- not a known variable star
10:11:33.26 +16:11:36.7 -- not a known variable star
10:11:39.23 +18:10:23.2 -- not a known variable star
10:11:42.93 +17:03:10.8 -- not a known variable star
10:11:43.59 +16:43:01.3 -- not a known variable star
10:12:07.19 +17:51:42.3 -- not a known variable star
10:12:07.51 +16:57:04.3 -- not a known variable star
10:12:08.38 +16:44:42.2 -- not a known variable star
10:12:18.53 +17:29:42.2 -- not a known variable star
10:12:27.87 +16:27:45.6 -- not a known variable star
10:12:32.91 +17:01:37.5 -- not a known variable star
10:12:39.69 +17:21:26.2 -- not a known variable star
10:12:42.47 +17:03:58.2 -- not a known variable star
10:12:42.81 +16:58:34.6 -- not a known variable star
10:12:52.06 +16:52:05.9 -- not a known variable star
10:12:53.82 +17:25:01.6 -- not a known variable star
10:12:57.74 +17:36:06.1 -- not a known variable star
10:12:59.58 +16:38:04.5 -- not a known variable star
10:12:59.74 +17:07:24.3 -- not a known variable star
10:13:06.84 +17:18:37.6 -- not a known variable star
10:13:30.26 +16:43:04.6 -- not a known variable star
10:13:46.76 +16:47:06.6 -- not a known variable star
10:14:18.13 +17:01:09.4 -- not a known variable star
Found 146 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
159 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 159 (excluding asteroids and hot pixels, 146 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)2461205.66330119 -observatory V36
07:15:08.54 +23:35:32.4 Mercury (0.5mag)
08:12:30.91 +22:02:10.8 Venus (-4.0mag)
03:07:00.19 +17:00:43.6 Mars (1.3mag)
07:53:28.36 +21:18:31.2 Jupiter (-1.8mag)
00:50:59.42 +02:57:22.1 Saturn (0.8mag)
04:01:36.78 +20:29:29.0 Uranus (5.8mag)
00:16:27.54 +00:18:31.7 Neptune (7.8mag)
20:32:59.98 -23:06:51.0 Pluto (14.5mag)
04:23:57.77 +25:54:53.9 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Jun 13 23:02 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461205.66330119:
07:53:34.39 +21:18:11.5 Io (6.0mag)
07:53:20.28 +21:18:56.3 Europa (6.2mag)
07:53:22.77 +21:18:44.4 Ganymede (5.6mag)
07:52:59.99 +21:19:58.7 Callisto (6.8mag)
07:53:24.30 +20:55:25.3 Himalia (15.6mag)
07:53:31.44 +21:18:22.0 Thebe (16.5mag)
07:53:13.80 +21:08:18.3 Elara (17.6mag)
07:55:57.04 +21:26:57.3 Pasiphae (17.7mag)
07:59:47.31 +21:20:42.1 Carme (18.9mag)
00:51:11.08 +02:57:10.1 Titan (8.6mag)
00:50:58.53 +02:57:14.6 Rhea (9.9mag)
00:51:25.51 +02:59:53.9 Iapetus (11.3mag)
00:51:13.95 +02:57:03.9 Hyperion (14.6mag)
00:51:34.29 +02:58:26.7 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 13 23:02 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461205.66330119:
17:28:16.57 -35:34:47.5 JWST
17:15:18.46 +43:45:20.7 Chandra
18:38:42.16 -22:15:02.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 13 23:02 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461205.66330119 -observatory V36
18:39:11.34 -33:04:24.9 13.6mag P/2010 H2 (Vales)
05:59:22.76 -68:00:54.7 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:51:15.96 +32:02:51.9 17.5mag C/2017 K2 (PANSTARRS)
17:12:20.81 +15:37:09.9 17.8mag C/2021 G2 (ATLAS)
22:10:17.66 -44:57:13.5 16.4mag P/2021 N1 (ZTF)
23:11:07.10 +31:48:23.5 17.2mag C/2022 E2 (ATLAS)
05:41:20.46 +27:00:08.5 16.5mag C/2022 N2 (PANSTARRS)
09:34:07.38 +30:52:01.5 16.7mag C/2022 QE78 (ATLAS)
08:53:49.36 +04:12:04.9 17.7mag C/2022 R6 (PANSTARRS)
18:24:17.61 +21:41:07.8 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:17:20.07 -11:01:40.6 17.6mag P/2023 B1 (PANSTARRS)
22:11:58.05 +66:52:27.4 17.8mag C/2023 H5 (Lemmon)
17:31:32.49 -07:17:17.9 13.7mag C/2023 R1 (PANSTARRS)
13:16:35.62 +81:36:46.3 18.0mag C/2023 X2 (Lemmon)
07:18:53.94 +64:31:13.2 17.7mag C/2024 A1 (ATLAS)
06:56:13.53 +28:20:24.7 13.8mag C/2024 E1 (Wierzchos)
15:32:43.06 +14:00:48.8 17.4mag C/2024 G6 (ATLAS)
20:08:43.65 +32:53:05.9 13.9mag C/2024 J3 (ATLAS)
04:24:00.37 -15:26:57.1 16.0mag C/2024 T5 (ATLAS)
06:11:27.22 +33:27:42.8 17.9mag C/2025 J1 (Borisov)
11:32:47.29 +52:23:36.0 17.6mag C/2025 L1 (ATLAS)
06:51:45.93 -11:08:58.6 14.7mag C/2025 R3 (PANSTARRS)
09:29:14.76 +23:14:42.1 17.9mag C/2025 V2 (Rankin)
12:39:44.76 +04:38:54.8 17.2mag C/2025 Y1 (ATLAS)
18:02:11.60 +76:20:22.5 17.8mag C/2026 A2 (Bok)
02:10:43.41 +43:49:25.2 16.2mag C/2026 B2 (Sun-Gao)
11:12:50.01 -01:44:48.1 16.6mag A/2026 E1
20:34:25.72 -09:06:38.0 8.4mag 10P/Tempel
11:03:32.70 -01:04:07.9 16.0mag 29P/Schwassmann-Wachmann
03:20:56.07 +26:25:54.2 17.7mag 47P/Ashbrook-Jackson
09:12:42.65 +22:02:35.3 16.9mag 63P/Wild
00:31:52.46 -06:00:27.9 15.6mag 65P/Gunn
07:02:49.99 +33:56:44.3 17.1mag 76P/West-Kohoutek-Ikemura
03:23:38.74 +17:56:36.6 13.8mag 78P/Gehrels
01:33:28.04 +06:06:28.4 15.7mag 88P/Howell
05:13:50.54 +30:40:35.4 15.3mag 93P/Lovas
03:00:05.33 +28:32:16.4 17.5mag 114P/Wiseman-Skiff
07:04:51.46 +32:47:01.3 15.5mag 123P/West-Hartley
10:00:38.01 +12:05:27.6 16.6mag 124P/Mrkos
04:08:53.33 +19:37:50.6 16.3mag 128P/Shoemaker-Holt
04:45:24.81 +19:19:48.3 17.8mag 131P/Mueller
06:23:12.14 +17:53:41.8 15.4mag 141P/Machholz
06:26:13.06 +17:52:47.0 15.4mag 141P-A/Machholz
05:23:37.46 +16:51:35.1 12.2mag 141P-D/Machholz
03:01:48.64 -23:53:59.8 16.6mag 161P/Hartley-IRAS
04:01:23.23 +26:07:17.0 15.0mag 162P/SidingSpring
19:35:29.10 +03:34:40.9 16.5mag 169P/NEAT
00:34:19.47 +03:36:16.7 17.8mag 220P/McNaught
16:47:47.11 -08:14:07.9 16.5mag 235P/LINEAR
07:48:06.28 +35:12:43.3 17.6mag 240P/NEAT
00:48:05.23 +00:06:20.2 16.2mag 260P/McNaught
04:20:39.17 +33:31:21.9 17.5mag 295P/LINEAR
00:26:38.47 -02:39:57.0 17.7mag 320P/McNaught
15:12:43.06 +07:51:36.9 17.5mag 391P/Kowalski
08:11:57.92 +20:35:06.2 17.9mag 450P/LONEOS
07:09:42.24 +41:15:56.7 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 13 23:02 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -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
15:03:05.18 +22:02:03.40 AT2026lxf 2026-05-8.07 13.94
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
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
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
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:26:28.11 -72:31:19.50 2026-06-11 17.05
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
21:26:28.11 -72:31:19.50 2026-06-11 17.05
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 2026-04-9.14 13.64
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 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
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
19:32:43.68 -22:39:32.70 ASASSN-26cm 2026-04-4.27 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
-rw-r--r-- 1 apache apache 5.6K Jun 13 23:02 asassn_transients_list.txt
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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 13 23:02 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:00:35.665 +40:33:28.48 AT 2026okd 2026-06-06.92 19.53
14:23:47.456 +75:46:01.44 AT 2026okc 2026-06-06.35 19.202
09:06:15.590 -05:53:46.80 AT 2026okb 2026-06-05.71 19.229
00:23:52.320 +36:21:31.09 AT 2026oka 2026-06-06.19 19.004
11:27:24.917 -04:39:24.73 AT 2026ojz 2026-06-05.80 19.208
08:40:07.303 -16:41:42.39 AT 2026ojy 2026-06-05.73 18.788
09:41:38.510 -12:30:07.46 AT 2026ojx 2026-06-04.26 19.393
14:21:14.441 +56:50:47.63 AT 2026ojw 2026-06-06.37 19.475
09:10:24.455 -13:57:44.58 AT 2026ojv 2026-06-05.73 19.004
10:12:37.525 +13:13:10.28 AT 2026oju 2026-06-05.26 19.164
13:19:00.470 +43:14:24.76 AT 2026ojt 2026-06-06.33 18.85
18:43:15.260 -08:47:37.40 AT 2026ojs 2026-06-06.73 17.82
00:35:11.496 -00:49:17.94 AT 2026ojr 2026-06-01.47 19.0273
13:27:16.739 -38:01:33.63 AT 2026ojq 2026-06-06.42 19.89
02:13:54.662 +31:51:42.05 AT 2026ojp 2026-05-31.48 18.5771
12:22:54.475 -14:25:27.09 AT 2026ojo 2026-06-06.37 20.1
12:12:13.424 -28:02:18.53 AT 2026ojn 2026-06-06.36 19.27
12:01:26.980 -21:29:06.86 AT 2026ojm 2026-06-06.37 19.41
10:54:17.334 -30:22:38.44 AT 2026ojl 2026-06-06.35 18.98
17:55:33.072 +06:11:38.39 AT 2026ojk 2026-06-05.77 18.68
-rw-r--r-- 1 apache apache 30K Jun 13 23:02 tns_transients_list.txt
