This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc
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 14.1813 2461205.6813 10.96 20:27:25.00 +23:26:56.7
64.95872 -8.66024 galactic Vul Second-epoch detections are separated by 0.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.8553+23.4505 | 20:27:25.27 +23:27:01.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:27:25.00 +23:26:56.7: 12.33 +/- 0.02 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:27:25.00 +23:26:56.7: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J306.8553+23.4505,2461205.6813,10.96,0.05,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 J306.8553+23.4505 20260614.1813 10.96CV 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 14.1813 2461205.6813 12.03 20:22:26.00 +23:52:46.0
64.66628 -7.47558 galactic Vul Second-epoch detections are separated by 1.5" and 6.3 pix
The object was found in VSX 3" ASAS J202226+2352.8
Type: MISC
# Max. Min./Amp. JD0 Period
9.998 Ic Y 0.384 Ic 2452956.40000 137.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:22:26.00 +23:52:46.0: 13.77 +/- 0.07 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:22:26.00 +23:52:46.0: 15.09 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J202226+2352.8,2461205.6813,12.03,0.05,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
ASAS J202226+2352.8 20260614.1813 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 14.1813 2461205.6813 12.79 20:28:42.22 +24:18:09.9
65.83736 -8.41465 galactic Vul Second-epoch detections are separated by 2.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:28:42.22 +24:18:09.9 (user input) | T | P | (position from user input) J-Ks=0.713+/-0.028 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:28:42.22 +24:18:09.9: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:28:42.22 +24:18:09.9: 15.82 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.79,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.68 20:19:31.65 +23:09:14.8
63.68449 -7.32756 galactic Vul Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:31.65 +23:09:14.8 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.041 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:31.65 +23:09:14.8: 13.75 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:31.65 +23:09:14.8: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.68,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.80 20:15:28.35 +23:54:07.5
63.79563 -6.13963 galactic Vul Second-epoch detections are separated by 1.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:28.35 +23:54:07.5 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.036 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:28.35 +23:54:07.5: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:28.35 +23:54:07.5: 15.49 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.49 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.80,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.57 20:18:23.54 +23:31:23.8
63.84857 -6.90605 galactic Vul Second-epoch detections are separated by 2.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.5974+23.5239 | 20:18:23.54 +23:31:23.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:23.54 +23:31:23.8: 15.01 +/- 0.18 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:23.54 +23:31:23.8: 15.08 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.5974+23.5239,2461205.6813,12.57,0.05,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
ATO J304.5974+23.5239 20260614.1813 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 14.1813 2461205.6813 12.44 20:19:56.50 +24:09:40.9
64.58122 -6.84623 galactic Vul Second-epoch detections are separated by 2.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:56.50 +24:09:40.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:56.50 +24:09:40.9: 15.69 +/- 0.33 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:56.50 +24:09:40.9: 15.70 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.69 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.44,0.05,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 20260614.1813 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 14.1813 2461205.6813 11.84 20:16:37.88 +23:06:36.9
63.27693 -6.79685 galactic Vul Second-epoch detections are separated by 0.3" and 6.3 pix
The object was found in VSX 2" ASASSN-V J201638.01+230637.4
Type: SR
# Max. Min./Amp. JD0 Period
13.070 V 13.330 V 2458347.94000 34.900000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:16:37.88 +23:06:36.9: 12.82 +/- 0.02 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:16:37.88 +23:06:36.9: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201638.01+230637.4,2461205.6813,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201638.01+230637.4 20260614.1813 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.46 20:15:15.95 +23:31:59.5
63.45934 -6.30257 galactic Vul Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.8143+23.5430 | 20:15:15.95 +23:31:59.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:15.95 +23:31:59.5: 15.05 +/- 0.19 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:15.95 +23:31:59.5: 14.47 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J303.8143+23.5430,2461205.6813,12.46,0.05,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
ATO J303.8143+23.5430 20260614.1813 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 14.1813 2461205.6813 12.53 20:23:45.75 +23:18:06.7
64.35663 -8.05195 galactic Vul Second-epoch detections are separated by 1.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1831052344789841280 | 20:23:48.26 +23:17:56.9 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.774+/-0.029 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:45.75 +23:18:06.7: 13.55 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:45.75 +23:18:06.7: 13.73 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1831052344789841280,2461205.6813,12.53,0.05,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
Gaia DR3 1831052344789841280 20260614.1813 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 14.1813 2461205.6813 12.49 20:27:50.30 +23:55:49.5
65.41439 -8.46540 galactic Vul Second-epoch detections are separated by 2.3" and 6.1 pix
The object was found in VSX19" Gaia DR3 1831179067809233024
Type: RS
# Max. Min./Amp. JD0 Period
17.640 G 17.760 G
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:27:50.30 +23:55:49.5: 15.35 +/- 0.27 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:27:50.30 +23:55:49.5: 15.03 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1831179067809233024,2461205.6813,12.49,0.05,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
Gaia DR3 1831179067809233024 20260614.1813 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 14.1813 2461205.6813 12.71 20:16:26.22 +24:21:00.1
64.29357 -6.07681 galactic Vul Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:26.22 +24:21:00.1 (user input) | T | P | (position from user input) J-Ks=0.671+/-0.028 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:16:26.22 +24:21:00.1: 15.06 +/- 0.20 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:16:26.22 +24:21:00.1: 15.66 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.71,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.29 20:13:26.81 +22:59:53.1
62.77881 -6.24523 galactic Vul Second-epoch detections are separated by 0.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:13:26.81 +22:59:53.1 (user input) | T | P | (position from user input) J-Ks=1.111+/-0.032 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:13:26.81 +22:59:53.1: 13.23 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:13:26.81 +22:59:53.1: 13.23 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.29,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.79 20:19:25.08 +23:28:38.5
63.94144 -7.12719 galactic Vul Second-epoch detections are separated by 1.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:25.08 +23:28:38.5 (user input) | T | P | (position from user input) J-Ks=0.461+/-0.034 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:25.08 +23:28:38.5: 14.91 +/- 0.16 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:25.08 +23:28:38.5: 15.80 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.91 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.79,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.55 20:32:06.83 +20:39:08.3
63.25571 -11.14867 galactic Del Second-epoch detections are separated by 2.7" and 6.8 pix
The object was found in VSX 1" NSVS J2032074+203906
Type: SR
# Max. Min./Amp. JD0 Period
12.945 r Y 0.793 r 2458373.53400 95.359256300000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:32:06.83 +20:39:08.3: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:32:06.83 +20:39:08.3: 15.75 +/- 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 14.1813* 20 32 06.83 +20 39 08.3 12.6 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2032074+203906,2461205.6813,12.55,0.05,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
NSVS J2032074+203906 20260614.1813 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 14.1813 2461205.6813 12.57 20:21:41.24 +23:04:49.3
63.90160 -7.78114 galactic Vul Second-epoch detections are separated by 2.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:21:41.24 +23:04:49.3 (user input) | T | P | (position from user input) J-Ks=1.165+/-0.031 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:21:41.24 +23:04:49.3: 13.65 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:21:41.24 +23:04:49.3: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.57,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.09 20:30:19.38 +21:06:49.9
63.39907 -10.54189 galactic Vul Second-epoch detections are separated by 0.8" and 6.6 pix
The object was found in VSX 2" ASASSN-V J203019.50+210650.2
Type: SR
# Max. Min./Amp. JD0 Period
13.690 V 14.100 V 2458432.67220 67.346746500000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:30:19.38 +21:06:49.9: 15.72 +/- 0.35 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:30:19.38 +21:06:49.9: 15.77 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.72 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J203019.50+210650.2,2461205.6813,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203019.50+210650.2 20260614.1813 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.52 20:17:35.60 +22:59:09.7
63.29529 -7.04998 galactic Vul Second-epoch detections are separated by 2.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:17:35.60 +22:59:09.7 (user input) | T | P | (position from user input) J-Ks=0.749+/-0.028 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:35.60 +22:59:09.7: 13.41 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:35.60 +22:59:09.7: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.52,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.12 20:20:45.40 +23:37:30.3
64.23725 -7.29986 galactic Vul Second-epoch detections are separated by 1.1" and 6.4 pix
The object was found in VSX 1" ASASSN-V J202045.48+233729.9
Type: SRS
# Max. Min./Amp. JD0 Period
13.390 V 13.630 V 2457133.09700 28.694000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:20:45.40 +23:37:30.3: 14.33 +/- 0.11 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:20:45.40 +23:37:30.3: 15.03 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J202045.48+233729.9,2461205.6813,12.12,0.05,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
ASASSN-V J202045.48+233729.9 20260614.1813 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 14.1813 2461205.6813 12.40 20:19:08.58 +23:06:10.5
63.59211 -7.28240 galactic Vul Second-epoch detections are separated by 2.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:08.58 +23:06:10.5 (user input) | T | P | (position from user input) J-Ks=1.166+/-0.031 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:08.58 +23:06:10.5: 13.34 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:08.58 +23:06:10.5: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.40,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.09 20:26:30.94 +23:29:03.1
64.86923 -8.47025 galactic Vul Second-epoch detections are separated by 1.5" and 6.3 pix
The object was found in VSX 2" ASASSN-V J202631.07+232903.1
Type: SR
# Max. Min./Amp. JD0 Period
14.320 g Y 0.780 g 2459154.76500 416.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:26:30.94 +23:29:03.1: 14.58 +/- 0.14 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:26:30.94 +23:29:03.1: 15.62 +/- 0.34 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J202631.07+232903.1,2461205.6813,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202631.07+232903.1 20260614.1813 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.81 20:18:36.22 +23:25:39.9
63.79547 -6.99930 galactic Vul Second-epoch detections are separated by 2.3" and 6.0 pix
The object was found in VSX 2" Gaia DR3 1830352200707825152
Type: VAR
# Max. Min./Amp. JD0 Period
13.260 G 13.280 G 0.022827500000 K
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:36.22 +23:25:39.9: 14.82 +/- 0.16 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:36.22 +23:25:39.9: 15.07 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830352200707825152,2461205.6813,12.81,0.05,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
Gaia DR3 1830352200707825152 20260614.1813 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 14.1813 2461205.6813 11.95 20:23:34.94 +22:27:35.4
63.62899 -8.49039 galactic Vul Second-epoch detections are separated by 0.2" and 6.5 pix
The object was found in VSX 1" NSVS 11430687
Type: SR|L
# Max. Min./Amp. JD0 Period
11.397 R1 11.865 R1 2451325.24000 64.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:34.94 +22:27:35.4: 13.27 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:34.94 +22:27:35.4: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11430687,2461205.6813,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11430687 20260614.1813 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.41 20:14:42.77 +23:36:31.4
63.45303 -6.15519 galactic Vul Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:14:42.77 +23:36:31.4 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.031 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:42.77 +23:36:31.4: 15.40 +/- 0.26 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:42.77 +23:36:31.4: 15.21 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.29 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.41,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.62 20:24:07.18 +23:16:29.3
64.38065 -8.13498 galactic Vul Second-epoch detections are separated by 2.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.0318+23.2687 | 20:24:07.18 +23:16:29.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:24:07.18 +23:16:29.3: 13.94 +/- 0.07 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:24:07.18 +23:16:29.3: 14.19 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.04 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J306.0318+23.2687,2461205.6813,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J306.0318+23.2687 20260614.1813 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 14.1813 2461205.6813 12.29 20:19:40.58 +23:06:45.1
63.66877 -7.37910 galactic Vul Second-epoch detections are separated by 1.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J201937.93+230632.1 | 20:19:37.93 +23:06:32.1 (Gaia DR3) | SR (local) | 2458798.50500 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:40.58 +23:06:45.1: 13.46 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:40.58 +23:06:45.1: 13.36 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201937.93+230632.1,2461205.6813,12.29,0.05,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
ASASSN-V J201937.93+230632.1 20260614.1813 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 14.1813 2461205.6813 12.62 20:20:13.86 +23:11:39.9
63.80887 -7.43959 galactic Vul Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1829584982109884672 | 20:20:12.59 +23:12:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:20:13.86 +23:11:39.9: 13.72 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:20:13.86 +23:11:39.9: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1829584982109884672,2461205.6813,12.62,0.05,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
Gaia DR3 1829584982109884672 20260614.1813 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 14.1813 2461205.6813 12.04 20:18:37.75 +23:28:46.6
63.84223 -6.97544 galactic Vul Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.6578+23.4797 | 20:18:37.88 +23:28:46.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.240+/-0.030 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:37.75 +23:28:46.6: 14.40 +/- 0.10 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:37.75 +23:28:46.6: 14.60 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.49 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.6578+23.4797,2461205.6813,12.04,0.05,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
ATO J304.6578+23.4797 20260614.1813 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 14.1813 2461205.6813 12.59 20:24:40.42 +23:23:01.0
64.54385 -8.17873 galactic Vul Second-epoch detections are separated by 1.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.1716+23.3872 | 20:24:38.96 +23:22:42.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:24:40.42 +23:23:01.0: 14.43 +/- 0.11 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:24:40.42 +23:23:01.0: 15.74 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.43 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J306.1716+23.3872,2461205.6813,12.59,0.05,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
ATO J306.1716+23.3872 20260614.1813 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 14.1813 2461205.6813 12.16 20:18:54.67 +23:11:49.1
63.64127 -7.18592 galactic Vul Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.7294+23.1962 | 20:18:54.67 +23:11:49.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:54.67 +23:11:49.1: 13.35 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:54.67 +23:11:49.1: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.7294+23.1962,2461205.6813,12.16,0.05,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
ATO J304.7294+23.1962 20260614.1813 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 14.1813 2461205.6813 12.52 20:19:07.28 +22:57:03.6
63.46183 -7.36243 galactic Vul Second-epoch detections are separated by 2.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:07.28 +22:57:03.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:07.28 +22:57:03.6: 13.41 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:07.28 +22:57:03.6: 13.51 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.52,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.70 20:22:39.53 +22:24:00.1
63.45813 -8.34703 galactic Vul Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:22:39.53 +22:24:00.1 (user input) | T | P | (position from user input) J-Ks=1.094+/-0.029 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:22:39.53 +22:24:00.1: 13.87 +/- 0.07 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:22:39.53 +22:24:00.1: 15.06 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.01 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.70,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.63 20:17:50.89 +23:21:37.3
63.64231 -6.89217 galactic Vul Second-epoch detections are separated by 2.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:17:50.89 +23:21:37.3 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.035 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:50.89 +23:21:37.3: 14.01 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:50.89 +23:21:37.3: 14.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.13 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.63,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.64 20:21:51.27 +22:31:05.7
63.45238 -8.12685 galactic Vul Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:21:51.27 +22:31:05.7 (user input) | T | P | (position from user input) J-Ks=0.883+/-0.031 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:21:51.27 +22:31:05.7: 13.74 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:21:51.27 +22:31:05.7: 14.34 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.64,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.46 20:27:03.70 +22:40:42.4
64.26980 -9.03061 galactic Vul Second-epoch detections are separated by 2.2" and 6.6 pix
The object was found in VSX 2" ASASSN-V J202703.83+224042.9
Type: SR
# Max. Min./Amp. JD0 Period
13.530 V 13.910 V 2458369.45190 178.714092400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:27:03.70 +22:40:42.4: 13.59 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:27:03.70 +22:40:42.4: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202703.83+224042.9,2461205.6813,12.46,0.05,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
ASASSN-V J202703.83+224042.9 20260614.1813 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 14.1813 2461205.6813 12.55 20:19:13.10 +23:48:41.8
64.19590 -6.90353 galactic Vul Second-epoch detections are separated by 1.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:13.10 +23:48:41.8 (user input) | T | P | (position from user input) J-Ks=0.456+/-0.032 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:13.10 +23:48:41.8: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:13.10 +23:48:41.8: 15.80 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.55,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.66 20:18:45.82 +23:41:06.2
64.03170 -6.88722 galactic Vul Second-epoch detections are separated by 1.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.6909+23.6776 | 20:18:45.82 +23:41:06.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:45.82 +23:41:06.2: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:45.82 +23:41:06.2: 15.77 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.6909+23.6776,2461205.6813,12.66,0.05,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
ATO J304.6909+23.6776 20260614.1813 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 14.1813 2461205.6813 12.50 20:23:52.00 +22:11:29.8
63.44163 -8.69521 galactic Vul Second-epoch detections are separated by 1.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.9658+22.1993 | 20:23:52.00 +22:11:29.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.462+/-0.028 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:52.00 +22:11:29.8: 13.68 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:52.00 +22:11:29.8: 15.02 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.77 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J305.9658+22.1993,2461205.6813,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J305.9658+22.1993 20260614.1813 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.45 20:18:41.39 +22:57:37.7
63.41434 -7.27447 galactic Vul Second-epoch detections are separated by 1.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:41.39 +22:57:37.7 (user input) | T | P | (position from user input) J-Ks=0.300+/-0.034 (F)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:41.39 +22:57:37.7: 13.45 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:41.39 +22:57:37.7: 13.31 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.45,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.19 20:25:23.34 +23:12:25.1
64.49020 -8.41403 galactic Vul Second-epoch detections are separated by 0.8" and 6.4 pix
The object was found in VSX 1" NSVS J2025235+231223
Type: SR
# Max. Min./Amp. JD0 Period
14.850 g Y 0.744 g 2458383.48320 70.676307000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:25:23.34 +23:12:25.1: 13.66 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:25:23.34 +23:12:25.1: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2025235+231223,2461205.6813,12.19,0.05,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
NSVS J2025235+231223 20260614.1813 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 14.1813 2461205.6813 12.71 20:19:15.78 +23:33:07.6
63.98421 -7.05614 galactic Vul Second-epoch detections are separated by 2.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:15.78 +23:33:07.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:15.78 +23:33:07.6: 15.54 +/- 0.30 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:15.78 +23:33:07.6: 15.71 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.54 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.71,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.29 20:18:01.86 +22:56:24.8
63.31282 -7.15927 galactic Vul Second-epoch detections are separated by 0.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:01.86 +22:56:24.8 (user input) | T | P | (position from user input) J-Ks=0.981+/-0.027 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:01.86 +22:56:24.8: 13.28 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:01.86 +22:56:24.8: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.29,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.79 20:19:58.50 +23:59:34.2
64.44452 -6.94644 galactic Vul Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.9971+23.9843 | 20:19:58.50 +23:59:34.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:58.50 +23:59:34.2: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:58.50 +23:59:34.2: 15.66 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.9971+23.9843,2461205.6813,12.79,0.05,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 J304.9971+23.9843 20260614.1813 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 14.1813 2461205.6813 12.38 20:19:05.11 +24:23:29.0
64.66423 -6.55603 galactic Vul Second-epoch detections are separated by 8.0" 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 | ATO J304.7769+24.3848 | 20:19:05.11 +24:23:29.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:05.11 +24:23:29.0: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:05.11 +24:23:29.0: 14.68 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.7769+24.3848,2461205.6813,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.7769+24.3848 20260614.1813 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 14.1813 2461205.6813 12.79 20:19:32.91 +23:49:30.8
64.24958 -6.95874 galactic Vul Second-epoch detections are separated by 1.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:32.91 +23:49:30.8 (user input) | T | P | (position from user input) J-Ks=0.868+/-0.030 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:32.91 +23:49:30.8: 15.67 +/- 0.32 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:32.91 +23:49:30.8: 15.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.67 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.79,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.79 20:23:31.80 +24:12:35.5
65.08386 -7.49687 galactic Vul Second-epoch detections are separated by 1.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:23:31.80 +24:12:35.5 (user input) | T | P | (position from user input) J-Ks=0.866+/-0.027 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:31.80 +24:12:35.5: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:31.80 +24:12:35.5: 15.84 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.79,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.39 20:18:39.74 +23:25:31.1
63.80093 -7.01186 galactic Vul Second-epoch detections are separated by 1.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:39.74 +23:25:31.1 (user input) | T | P | (position from user input) J-Ks=0.901+/-0.036 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:39.74 +23:25:31.1: 14.02 +/- 0.08 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:39.74 +23:25:31.1: 14.56 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.15 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.39,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.69 20:14:48.97 +24:10:43.3
63.94541 -5.86253 galactic Vul Second-epoch detections are separated by 3.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.7013+24.1798 | 20:14:48.97 +24:10:43.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.330+/-0.032 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:48.97 +24:10:43.3: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:48.97 +24:10:43.3: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J303.7013+24.1798,2461205.6813,12.69,0.05,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
ATO J303.7013+24.1798 20260614.1813 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 14.1813 2461205.6813 12.61 20:18:55.93 +23:03:42.1
63.53044 -7.26487 galactic Vul Second-epoch detections are separated by 2.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:55.93 +23:03:42.1 (user input) | T | P | (position from user input) J-Ks=0.772+/-0.030 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:55.93 +23:03:42.1: 13.72 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:55.93 +23:03:42.1: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.61,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.61 20:17:59.47 +23:33:41.6
63.82943 -6.80828 galactic Vul Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1830403942162271232 | 20:17:59.63 +23:33:41.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.377+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:59.47 +23:33:41.6: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:59.47 +23:33:41.6: 15.77 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830403942162271232,2461205.6813,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1830403942162271232 20260614.1813 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 14.1813 2461205.6813 12.53 20:20:25.79 +22:50:29.7
63.53873 -7.67384 galactic Vul Second-epoch detections are separated by 1.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.1097+22.8409 | 20:20:25.79 +22:50:29.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.878+/-0.033 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:20:25.79 +22:50:29.7: 13.50 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:20:25.79 +22:50:29.7: 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J305.1097+22.8409,2461205.6813,12.53,0.05,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
ATO J305.1097+22.8409 20260614.1813 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 14.1813 2461205.6813 12.55 20:11:23.36 +22:41:21.9
62.25927 -6.01471 galactic Vul Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:11:23.36 +22:41:21.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:11:23.36 +22:41:21.9: 13.46 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:11:23.36 +22:41:21.9: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.55,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.66 20:14:31.75 +23:09:11.9
63.04635 -6.36912 galactic Vul Second-epoch detections are separated by 2.0" and 6.2 pix
The object was found in VSX 1" ASASSN-V J201431.84+230912.4
Type: SR
# Max. Min./Amp. JD0 Period
14.130 V 14.540 V 2457470.10000 84.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:31.75 +23:09:11.9: 13.99 +/- 0.08 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:31.75 +23:09:11.9: 13.88 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201431.84+230912.4,2461205.6813,12.66,0.05,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
ASASSN-V J201431.84+230912.4 20260614.1813 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 14.1813 2461205.6813 12.46 20:26:47.98 +21:11:16.6
62.98850 -9.82283 galactic Vul Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.7010+21.1877 | 20:26:47.98 +21:11:16.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:26:47.98 +21:11:16.6: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:26:47.98 +21:11:16.6: 15.75 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J306.7010+21.1877,2461205.6813,12.46,0.05,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
ATO J306.7010+21.1877 20260614.1813 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 14.1813 2461205.6813 12.06 20:15:40.67 +23:47:48.2
63.73303 -6.23675 galactic Vul Second-epoch detections are separated by 1.0" and 6.3 pix
The object was found in VSX 3" ASASSN-V J201540.83+234746.9
Type: SR
# Max. Min./Amp. JD0 Period
13.660 V 14.230 V 2458288.98240 90.125521000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:40.67 +23:47:48.2: 13.71 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:40.67 +23:47:48.2: 14.48 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.86 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201540.83+234746.9,2461205.6813,12.06,0.05,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
ASASSN-V J201540.83+234746.9 20260614.1813 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 14.1813 2461205.6813 12.88 20:23:49.18 +24:45:14.6
65.57443 -7.24430 galactic Vul Second-epoch detections are separated by 2.2" and 6.2 pix
The object was found in VSX17" Gaia DR3 1832088050380126976
Type: ROT
# Max. Min./Amp. JD0 Period
18.260 G 18.320 G 0.781920000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:49.18 +24:45:14.6: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:49.18 +24:45:14.6: 15.76 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1832088050380126976,2461205.6813,12.88,0.05,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 1832088050380126976 20260614.1813 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 14.1813 2461205.6813 12.71 20:15:26.19 +23:37:25.0
63.55697 -6.28565 galactic Vul Second-epoch detections are separated by 3.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1830586529817588224 | 20:15:28.43 +23:37:57.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.314+/-0.038 (F)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:26.19 +23:37:25.0: 14.84 +/- 0.16 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:26.19 +23:37:25.0: 15.58 +/- 0.33 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830586529817588224,2461205.6813,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1830586529817588224 20260614.1813 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 14.1813 2461205.6813 12.40 20:20:26.10 +24:16:27.2
64.73875 -6.87665 galactic Vul Second-epoch detections are separated by 1.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:20:26.10 +24:16:27.2 (user input) | T | P | (position from user input) J-Ks=1.220+/-0.029 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:20:26.10 +24:16:27.2: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:20:26.10 +24:16:27.2: 15.73 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.40,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.52 20:18:36.33 +23:11:17.1
63.59460 -7.13235 galactic Vul Second-epoch detections are separated by 0.9" and 6.4 pix
The object was found in VSX 2" Gaia DR3 1830343954370813824
Type: ROT
# Max. Min./Amp. JD0 Period
13.340 G 13.360 G F
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:36.33 +23:11:17.1: 13.58 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:36.33 +23:11:17.1: 13.55 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830343954370813824,2461205.6813,12.52,0.05,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
Gaia DR3 1830343954370813824 20260614.1813 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 14.1813 2461205.6813 12.41 20:19:54.65 +23:42:39.3
64.20034 -7.09121 galactic Vul Second-epoch detections are separated by 1.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.9787+23.7040 | 20:19:54.65 +23:42:39.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.769+/-0.033 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:54.65 +23:42:39.3: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:54.65 +23:42:39.3: 14.08 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.9787+23.7040,2461205.6813,12.41,0.05,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
ATO J304.9787+23.7040 20260614.1813 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 14.1813 2461205.6813 12.88 20:19:07.33 +23:50:31.1
64.20903 -6.86837 galactic Vul Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:07.33 +23:50:31.1 (user input) | T | P | (position from user input) J-Ks=1.030+/-0.032 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:07.33 +23:50:31.1: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:07.33 +23:50:31.1: 15.80 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.88,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.46 20:14:24.38 +23:07:33.9
63.00788 -6.36035 galactic Vul Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:14:24.38 +23:07:33.9 (user input) | T | P | (position from user input) J-Ks=1.139+/-0.034 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:24.38 +23:07:33.9: 13.56 +/- 0.07 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:24.38 +23:07:33.9: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.46,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.35 20:14:18.66 +23:16:57.2
63.12767 -6.25649 galactic Vul Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:14:18.66 +23:16:57.2 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.040 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:18.66 +23:16:57.2: 14.52 +/- 0.13 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:18.66 +23:16:57.2: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1813 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 14.1813 2461205.6813 12.47 20:19:26.11 +24:07:44.6
64.48940 -6.76824 galactic Vul Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.8621+24.1326 | 20:19:26.11 +24:07:44.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.377+/-0.028 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:26.11 +24:07:44.6: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:26.11 +24:07:44.6: 13.70 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.8621+24.1326,2461205.6813,12.47,0.05,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
ATO J304.8621+24.1326 20260614.1813 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 14.1813 2461205.6813 12.39 20:22:12.40 +22:35:35.5
63.56104 -8.15248 galactic Vul Second-epoch detections are separated by 2.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:22:12.40 +22:35:35.5 (user input) | T | P | (position from user input) J-Ks=0.674+/-0.030 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:22:12.40 +22:35:35.5: 13.37 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:22:12.40 +22:35:35.5: 13.82 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.39,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.65 20:14:28.85 +23:20:02.8
63.19255 -6.26095 galactic Vul Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:14:28.85 +23:20:02.8 (user input) | T | P | (position from user input) J-Ks=0.871+/-0.034 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:28.85 +23:20:02.8: 14.65 +/- 0.14 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:28.85 +23:20:02.8: 14.05 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.21 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1813 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 14.1813 2461205.6813 12.38 20:17:45.56 +23:03:50.7
63.38211 -7.03877 galactic Vul Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.4294+23.0658 | 20:17:45.56 +23:03:50.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.649+/- (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:45.56 +23:03:50.7: 13.31 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:45.56 +23:03:50.7: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.4294+23.0658,2461205.6813,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.4294+23.0658 20260614.1813 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 14.1813 2461205.6813 12.54 20:17:05.18 +24:10:42.5
64.23184 -6.29490 galactic Vul Second-epoch detections are separated by 1.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.2666+24.1724 | 20:17:05.18 +24:10:42.5 (user input) | MPULSE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.994+/-0.026 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:05.18 +24:10:42.5: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:05.18 +24:10:42.5: 15.77 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.2666+24.1724,2461205.6813,12.54,0.05,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 J304.2666+24.1724 20260614.1813 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 14.1813 2461205.6813 12.57 20:21:00.10 +23:15:20.0
63.95955 -7.55260 galactic Vul Second-epoch detections are separated by 1.2" and 6.3 pix
The object was found in VSX 3" ASASSN-V J202100.29+231520.9
Type: SR
# Max. Min./Amp. JD0 Period
13.920 V 14.440 V 2457303.80000 60.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:21:00.10 +23:15:20.0: 14.04 +/- 0.08 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:21:00.10 +23:15:20.0: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J202100.29+231520.9,2461205.6813,12.57,0.05,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
ASASSN-V J202100.29+231520.9 20260614.1813 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 14.1813 2461205.6813 12.30 20:21:59.75 +22:43:25.2
63.64292 -8.03927 galactic Vul Second-epoch detections are separated by 1.7" and 6.3 pix
The object was found in VSX 2" ASASSN-V J202159.88+224326.0
Type: SR
# Max. Min./Amp. JD0 Period
14.570 g Y 0.480 g 2458681.88200 79.260000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:21:59.75 +22:43:25.2: 13.57 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:21:59.75 +22:43:25.2: 13.59 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202159.88+224326.0,2461205.6813,12.30,0.05,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
ASASSN-V J202159.88+224326.0 20260614.1813 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 14.1813 2461205.6813 12.52 20:27:47.52 +24:08:40.9
65.58618 -8.33446 galactic Vul Second-epoch detections are separated by 0.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J306.9494+24.1564 | 20:27:47.52 +24:08:40.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:27:47.52 +24:08:40.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:27:47.52 +24:08:40.9: 15.77 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J306.9494+24.1564,2461205.6813,12.52,0.05,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
ATO J306.9494+24.1564 20260614.1813 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 14.1813 2461205.6813 12.22 20:17:43.06 +24:59:39.7
64.99517 -5.96288 galactic Vul Second-epoch detections are separated by 1.5" and 6.2 pix
The object was found in VSX 2" ASASSN-V J201743.20+245940.1
Type: SR
# Max. Min./Amp. JD0 Period
13.570 V 13.960 V 2458328.79430 193.798899300000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:43.06 +24:59:39.7: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:43.06 +24:59:39.7: 15.66 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201743.20+245940.1,2461205.6813,12.22,0.05,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
ASASSN-V J201743.20+245940.1 20260614.1813 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 14.1813 2461205.6813 12.38 20:13:46.81 +23:13:04.3
63.00618 -6.18967 galactic Vul Second-epoch detections are separated by 3.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:13:46.81 +23:13:04.3 (user input) | T | P | (position from user input) J-Ks=0.318+/-0.038 (F)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:13:46.81 +23:13:04.3: 13.74 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:13:46.81 +23:13:04.3: 13.42 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.38,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.14 20:16:37.13 +24:06:43.1
64.11683 -6.24268 galactic Vul Second-epoch detections are separated by 2.7" and 6.0 pix
The object was found in VSX10" ASASSN-V J201637.05+240653.0
Type: SR
# Max. Min./Amp. JD0 Period
13.690 V 13.910 V 2458266.82990 121.420540800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:16:37.13 +24:06:43.1: 15.29 +/- 0.27 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:16:37.13 +24:06:43.1: 15.13 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.20 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201637.05+240653.0,2461205.6813,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201637.05+240653.0 20260614.1813 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.00 20:23:12.59 +22:21:31.5
63.49557 -8.47570 galactic Vul Second-epoch detections are separated by 1.5" and 6.3 pix
The object was found in VSX 1" ASASSN-V J202312.69+222131.7
Type: SRS
# Max. Min./Amp. JD0 Period
13.120 V 13.290 V 2458307.06000 26.551000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:12.59 +22:21:31.5: 12.97 +/- 0.03 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:12.59 +22:21:31.5: 14.48 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202312.69+222131.7,2461205.6813,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J202312.69+222131.7 20260614.1813 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.67 20:17:28.92 +22:57:52.5
63.26302 -7.04043 galactic Vul Second-epoch detections are separated by 1.8" and 6.2 pix
The object was found in VSX 2" ASASSN-V J201729.07+225753.3
Type: SRS
# Max. Min./Amp. JD0 Period
14.170 V 14.340 V 2458019.88000 26.579000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:28.92 +22:57:52.5: 13.73 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:28.92 +22:57:52.5: 13.69 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201729.07+225753.3,2461205.6813,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201729.07+225753.3 20260614.1813 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.32 20:19:02.45 +23:32:09.7
63.94225 -7.02271 galactic Vul Second-epoch detections are separated by 1.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1830360305294172288 | 20:19:01.22 +23:31:43.9 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE J-Ks=1.103+/-0.030 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:02.45 +23:32:09.7: 14.57 +/- 0.13 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:02.45 +23:32:09.7: 15.13 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830360305294172288,2461205.6813,12.32,0.05,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
Gaia DR3 1830360305294172288 20260614.1813 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 14.1813 2461205.6813 12.54 20:19:02.12 +23:01:14.4
63.50925 -7.30736 galactic Vul Second-epoch detections are separated by 1.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:02.12 +23:01:14.4 (user input) | T | P | (position from user input) J-Ks=0.483+/-0.033 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:02.12 +23:01:14.4: 13.44 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:02.12 +23:01:14.4: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1813 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 14.1813 2461205.6813 12.70 20:23:04.80 +22:54:38.6
63.94070 -8.14169 galactic Vul Second-epoch detections are separated by 5.2" and 5.7 pix
The object was found in VSX 2" ASASSN-V J202304.84+225440.6
Type: SRS
# Max. Min./Amp. JD0 Period
14.150 V 14.310 V 2457106.13000 23.402000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:04.80 +22:54:38.6: 13.87 +/- 0.07 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:04.80 +22:54:38.6: 13.87 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.87 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J202304.84+225440.6,2461205.6813,12.70,0.05,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
ASASSN-V J202304.84+225440.6 20260614.1813 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 14.1813 2461205.6813 12.54 20:16:05.07 +24:17:55.9
64.20613 -6.03801 galactic Vul Second-epoch detections are separated by 1.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.0183+24.3023 | 20:16:05.07 +24:17:55.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.301+/-0.034 (F)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:16:05.07 +24:17:55.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:16:05.07 +24:17:55.9: 15.68 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.0183+24.3023,2461205.6813,12.54,0.05,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 J304.0183+24.3023 20260614.1813 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 14.1813 2461205.6813 12.52 20:12:57.05 +23:39:07.6
63.26793 -5.79345 galactic Vul Second-epoch detections are separated by 1.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:12:57.05 +23:39:07.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:12:57.05 +23:39:07.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:12:57.05 +23:39:07.6: 15.53 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.52,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.84 20:18:46.17 +23:28:12.9
63.85235 -7.00741 galactic Vul Second-epoch detections are separated by 4.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:46.17 +23:28:12.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:46.17 +23:28:12.9: 14.75 +/- 0.14 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:46.17 +23:28:12.9: 15.87 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.75 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.84,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.52 20:12:57.35 +23:18:54.0
62.98432 -5.97799 galactic Vul Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:12:57.35 +23:18:54.0 (user input) | T | P | (position from user input) J-Ks=0.731+/-0.033 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:12:57.35 +23:18:54.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:12:57.35 +23:18:54.0: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.52,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.62 20:19:20.82 +23:47:36.0
64.19707 -6.93815 galactic Vul Second-epoch detections are separated by 2.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.8431+23.7858 | 20:19:20.82 +23:47:36.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.607+/-0.032 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:20.82 +23:47:36.0: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:20.82 +23:47:36.0: 15.78 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.8431+23.7858,2461205.6813,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.8431+23.7858 20260614.1813 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 14.1813 2461205.6813 12.04 20:14:40.28 +23:44:03.1
63.55337 -6.07852 galactic Vul Second-epoch detections are separated by 1.1" and 6.3 pix
The object was found in VSX 2" ASASSN-V J201440.27+234404.9
Type: L
# Max. Min./Amp. JD0 Period
13.490 V 13.780 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:40.28 +23:44:03.1: 15.36 +/- 0.23 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:40.28 +23:44:03.1: 14.20 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.32 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201440.27+234404.9,2461205.6813,12.04,0.05,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
ASASSN-V J201440.27+234404.9 20260614.1813 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 14.1813 2461205.6813 12.65 20:23:40.99 +23:27:45.3
64.48049 -7.94651 galactic Vul Second-epoch detections are separated by 3.3" and 5.9 pix
The object was found in VSX 4" Gaia DR3 1831103613826707328
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.720 G 13.750 G A
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:40.99 +23:27:45.3: 14.30 +/- 0.09 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:40.99 +23:27:45.3: 15.74 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.30 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1831103613826707328,2461205.6813,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1831103613826707328 20260614.1813 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 14.1813 2461205.6813 12.45 20:22:46.53 +23:06:20.7
64.06417 -7.97435 galactic Vul Second-epoch detections are separated by 1.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.7032+23.1139 | 20:22:46.53 +23:06:20.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:22:46.53 +23:06:20.7: 13.51 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:22:46.53 +23:06:20.7: 13.47 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J305.7032+23.1139,2461205.6813,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J305.7032+23.1139 20260614.1813 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 14.1813 2461205.6813 12.31 20:21:04.73 +23:59:58.4
64.59188 -7.15190 galactic Vul Second-epoch detections are separated by 1.8" and 6.5 pix
The object was found in VSX 1" ASASSN-V J202104.82+235957.9
Type: SRS
# Max. Min./Amp. JD0 Period
13.570 V 13.660 V 2457596.04500 18.424000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:21:04.73 +23:59:58.4: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:21:04.73 +23:59:58.4: 14.28 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J202104.82+235957.9,2461205.6813,12.31,0.05,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
ASASSN-V J202104.82+235957.9 20260614.1813 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 14.1813 2461205.6813 12.66 20:18:10.49 +23:09:22.8
63.51277 -7.06746 galactic Vul Second-epoch detections are separated by 2.2" and 6.2 pix
The object was found in VSX14" ZTF J201811.20+230912.4
Type: EW
# Max. Min./Amp. JD0 Period
16.888 r Y 0.252 r 2458346.81650 0.340596400000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:10.49 +23:09:22.8: 13.69 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:10.49 +23:09:22.8: 13.71 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201811.20+230912.4,2461205.6813,12.66,0.05,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
ZTF J201811.20+230912.4 20260614.1813 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 14.1813 2461205.6813 12.64 20:14:02.44 +23:12:03.1
63.02471 -6.24910 galactic Vul Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.5091+23.2119 | 20:14:02.44 +23:12:03.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:02.44 +23:12:03.1: 14.33 +/- 0.11 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:02.44 +23:12:03.1: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J303.5091+23.2119,2461205.6813,12.64,0.05,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 J303.5091+23.2119 20260614.1813 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 14.1813 2461205.6813 12.66 20:14:50.01 +22:26:23.0
62.48336 -6.81782 galactic Vul Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1830178099918889472 | 20:14:48.67 +22:25:52.1 (Gaia DR3) | S (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.986+/-0.037 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:50.01 +22:26:23.0: 13.65 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:50.01 +22:26:23.0: 13.90 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830178099918889472,2461205.6813,12.66,0.05,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
Gaia DR3 1830178099918889472 20260614.1813 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 14.1813 2461205.6813 11.73 20:19:37.76 +23:06:32.2
63.65971 -7.37210 galactic Vul Second-epoch detections are separated by 1.3" and 6.3 pix
The object was found in VSX 3" ASASSN-V J201937.93+230632.1
Type: SR
# Max. Min./Amp. JD0 Period
14.090 g Y 0.220 g 2458798.50500 34.410000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:37.76 +23:06:32.2: 12.68 +/- 0.02 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:37.76 +23:06:32.2: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201937.93+230632.1,2461205.6813,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201937.93+230632.1 20260614.1813 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.56 20:13:56.23 +23:29:05.4
63.25093 -6.07412 galactic Vul Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:13:56.23 +23:29:05.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:13:56.23 +23:29:05.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:13:56.23 +23:29:05.4: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.07 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.56,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.65 20:19:37.91 +23:05:43.5
63.64869 -7.38009 galactic Vul Second-epoch detections are separated by 7.8" and 5.8 pix
The object was found in VSX 3" Gaia DR3 1830328458128671488
Type: ROT
# Max. Min./Amp. JD0 Period
14.490 G 14.520 G G
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:37.91 +23:05:43.5: 13.77 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:37.91 +23:05:43.5: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1830328458128671488,2461205.6813,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1830328458128671488 20260614.1813 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 14.1813 2461205.6813 12.53 20:18:28.04 +23:11:01.8
63.57333 -7.10826 galactic Vul Second-epoch detections are separated by 0.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:28.04 +23:11:01.8 (user input) | T | P | (position from user input) J-Ks=0.796+/-0.028 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:28.04 +23:11:01.8: 13.73 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:28.04 +23:11:01.8: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.53,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.86 20:18:16.35 +23:25:22.4
63.74902 -6.93872 galactic Vul Second-epoch detections are separated by 1.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.5689+23.4228 | 20:18:16.35 +23:25:22.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:16.35 +23:25:22.4: 14.96 +/- 0.16 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:16.35 +23:25:22.4: 14.89 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.5689+23.4228,2461205.6813,12.86,0.05,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
ATO J304.5689+23.4228 20260614.1813 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 14.1813 2461205.6813 12.69 20:18:13.34 +24:34:56.0
64.71418 -6.28679 galactic Vul Second-epoch detections are separated by 1.3" and 6.5 pix
The object was found in VSX 2" ASASSN-V J201813.48+243455.2
Type: SRS
# Max. Min./Amp. JD0 Period
13.910 V 14.040 V 2457203.84100 25.774000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:13.34 +24:34:56.0: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:13.34 +24:34:56.0: 14.67 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201813.48+243455.2,2461205.6813,12.69,0.05,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
ASASSN-V J201813.48+243455.2 20260614.1813 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 14.1813 2461205.6813 12.60 20:23:04.63 +23:05:54.5
64.09736 -8.03588 galactic Vul Second-epoch detections are separated by 3.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:23:04.63 +23:05:54.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:04.63 +23:05:54.5: 13.72 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:04.63 +23:05:54.5: 13.65 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.60,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.70 20:16:34.82 +23:55:41.4
63.95769 -6.33668 galactic Vul Second-epoch detections are separated by 2.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:34.82 +23:55:41.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:16:34.82 +23:55:41.4: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:16:34.82 +23:55:41.4: 15.68 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.70,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.79 20:18:40.19 +22:59:37.7
63.43976 -7.25219 galactic Vul Second-epoch detections are separated by 3.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.6702+22.9969 | 20:18:40.19 +22:59:37.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.133+/-0.030 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:40.19 +22:59:37.7: 14.02 +/- 0.08 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:40.19 +22:59:37.7: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.6702+22.9969,2461205.6813,12.79,0.05,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 J304.6702+22.9969 20260614.1813 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 14.1813 2461205.6813 12.79 20:15:49.06 +23:46:14.4
63.72882 -6.27779 galactic Vul Second-epoch detections are separated by 2.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:49.06 +23:46:14.4 (user input) | T | P | (position from user input) J-Ks=1.340+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:49.06 +23:46:14.4: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:49.06 +23:46:14.4: 15.80 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.79,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.37 20:16:46.15 +23:39:25.9
63.75412 -6.52208 galactic Vul Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.1984+23.6690 | 20:16:46.32 +23:39:26.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.323+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:16:46.15 +23:39:25.9: 15.52 +/- 0.29 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:16:46.15 +23:39:25.9: 15.20 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.1984+23.6690,2461205.6813,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.1984+23.6690 20260614.1813 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 14.1813 2461205.6813 12.31 20:08:52.27 +22:36:04.1
61.86979 -5.57288 galactic Vul Second-epoch detections are separated by 3.3" and 5.9 pix
The object was found in VSX 2" ASASSN-V J200852.42+223604.2
Type: SR
# Max. Min./Amp. JD0 Period
13.470 V 13.590 V 2458234.01000 46.220000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:08:52.27 +22:36:04.1: 13.24 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:08:52.27 +22:36:04.1: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200852.42+223604.2,2461205.6813,12.31,0.05,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
ASASSN-V J200852.42+223604.2 20260614.1813 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 14.1813 2461205.6813 12.63 20:23:46.41 +24:07:33.9
65.04562 -7.58996 galactic Vul Second-epoch detections are separated by 3.8" and 7.0 pix
The object was found in VSX12" Gaia DR3 1831983360565594112
Type: ROT
# Max. Min./Amp. JD0 Period
13.970 G 13.990 G G
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:46.41 +24:07:33.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:46.41 +24:07:33.9: 14.60 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1831983360565594112,2461205.6813,12.63,0.05,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
Gaia DR3 1831983360565594112 20260614.1813 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 14.1813 2461205.6813 12.66 20:20:02.81 +23:11:46.8
63.78675 -7.40336 galactic Vul Second-epoch detections are separated by 2.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.0122+23.1964 | 20:20:02.81 +23:11:46.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.348+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:20:02.81 +23:11:46.8: 14.10 +/- 0.08 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:20:02.81 +23:11:46.8: 13.98 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.03 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J305.0122+23.1964,2461205.6813,12.66,0.05,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
ATO J305.0122+23.1964 20260614.1813 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 14.1813 2461205.6813 12.54 20:14:26.27 +23:55:18.5
63.68180 -5.93109 galactic Vul Second-epoch detections are separated by 0.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:14:26.27 +23:55:18.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:26.27 +23:55:18.5: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:26.27 +23:55:18.5: 15.56 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1813 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 14.1813 2461205.6813 12.66 20:21:39.38 +23:14:06.8
64.02721 -7.68872 galactic Vul Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:21:39.38 +23:14:06.8 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.031 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:21:39.38 +23:14:06.8: 13.78 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:21:39.38 +23:14:06.8: 13.83 +/- 0.05 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.66,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.61 20:25:28.11 +21:50:31.3
63.35987 -9.19871 galactic Vul Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:25:28.11 +21:50:31.3 (user input) | T | P | (position from user input) J-Ks=0.952+/-0.027 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:25:28.11 +21:50:31.3: 15.04 +/- 0.19 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:25:28.11 +21:50:31.3: 14.50 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.61,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.68 20:15:47.40 +24:03:53.9
63.97258 -6.11068 galactic Vul Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1830632816694245888 | 20:15:47.40 +24:03:53.9 (user input) | ROT (local) | (local) | (position from user input) J-Ks=1.153+/-0.030 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:47.40 +24:03:53.9: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:47.40 +24:03:53.9: 15.81 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830632816694245888,2461205.6813,12.68,0.05,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 1830632816694245888 20260614.1813 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 14.1813 2461205.6813 12.79 20:15:46.06 +22:57:45.7
63.04285 -6.71187 galactic Vul Second-epoch detections are separated by 1.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:46.06 +22:57:45.7 (user input) | T | P | (position from user input) J-Ks=1.256+/-0.030 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:46.06 +22:57:45.7: 13.84 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:46.06 +22:57:45.7: 13.95 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.79,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.64 20:15:44.83 +24:28:19.7
64.30903 -5.87847 galactic Vul Second-epoch detections are separated by 1.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:44.83 +24:28:19.7 (user input) | T | P | (position from user input) J-Ks=1.183+/-0.030 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:44.83 +24:28:19.7: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:44.83 +24:28:19.7: 15.80 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.64,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.63 20:17:43.69 +23:06:52.6
63.42058 -7.00490 galactic Vul Second-epoch detections are separated by 0.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:17:43.69 +23:06:52.6 (user input) | T | P | (position from user input) J-Ks=0.839+/-0.028 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:43.69 +23:06:52.6: 13.70 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:43.69 +23:06:52.6: 13.70 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.63,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.68 20:21:03.59 +24:08:50.5
64.71294 -7.06568 galactic Vul Second-epoch detections are separated by 2.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:21:03.59 +24:08:50.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:21:03.59 +24:08:50.5: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:21:03.59 +24:08:50.5: 15.80 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.68,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.67 20:20:11.91 +23:50:00.5
64.33985 -7.07764 galactic Vul Second-epoch detections are separated by 2.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.0474+23.8319 | 20:20:11.91 +23:50:00.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.938+/-0.030 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:20:11.91 +23:50:00.5: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:20:11.91 +23:50:00.5: 14.30 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J305.0474+23.8319,2461205.6813,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J305.0474+23.8319 20260614.1813 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.56 20:18:57.60 +23:16:23.1
63.71139 -7.15308 galactic Vul Second-epoch detections are separated by 2.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.7365+23.2642 | 20:18:57.60 +23:16:23.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:57.60 +23:16:23.1: 13.88 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:57.60 +23:16:23.1: 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.7365+23.2642,2461205.6813,12.56,0.05,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
ATO J304.7365+23.2642 20260614.1813 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 14.1813 2461205.6813 12.30 20:18:35.60 +22:54:41.2
63.36077 -7.28309 galactic Vul Second-epoch detections are separated by 1.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:35.60 +22:54:41.2 (user input) | T | P | (position from user input) J-Ks=0.861+/-0.033 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:35.60 +22:54:41.2: 13.28 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:35.60 +22:54:41.2: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.30,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.49 20:17:20.32 +24:20:12.9
64.39666 -6.25526 galactic Vul Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.3410+24.3374 | 20:17:20.32 +24:20:12.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.295+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:20.32 +24:20:12.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:20.32 +24:20:12.9: 15.73 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.3410+24.3374,2461205.6813,12.49,0.05,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
ATO J304.3410+24.3374 20260614.1813 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 14.1813 2461205.6813 12.66 20:23:45.85 +23:27:44.0
64.49074 -7.96207 galactic Vul Second-epoch detections are separated by 2.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:23:45.85 +23:27:44.0 (user input) | T | P | (position from user input) J-Ks=0.363+/-0.033 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:45.85 +23:27:44.0: 14.09 +/- 0.08 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:45.85 +23:27:44.0: 15.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.09 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.66,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.68 20:20:05.96 +23:59:41.3
64.46210 -6.96892 galactic Vul Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:20:05.96 +23:59:41.3 (user input) | T | P | (position from user input) J-Ks=0.831+/-0.029 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:20:05.96 +23:59:41.3: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:20:05.96 +23:59:41.3: 15.40 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.40 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.68,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.62 20:28:25.05 +24:13:43.6
65.73831 -8.40349 galactic Vul Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:28:25.05 +24:13:43.6 (user input) | T | P | (position from user input) J-Ks=0.637+/-0.028 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:28:25.05 +24:13:43.6: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:28:25.05 +24:13:43.6: 15.76 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.62,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.49 20:18:41.36 +23:32:44.5
63.90535 -6.95030 galactic Vul Second-epoch detections are separated by 0.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:41.36 +23:32:44.5 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.037 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:41.36 +23:32:44.5: 14.72 +/- 0.13 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:41.36 +23:32:44.5: 15.88 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.72 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.49,0.05,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 20260614.1813 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 14.1813 2461205.6813 11.88 20:22:52.68 +22:37:20.1
63.67291 -8.26469 galactic Vul Second-epoch detections are separated by 1.5" and 6.2 pix
The object was found in VSX 2" ASASSN-V J202252.81+223720.4
Type: SR
# Max. Min./Amp. JD0 Period
13.380 V 13.700 V 2457860.00000 533.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:22:52.68 +22:37:20.1: 13.16 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:22:52.68 +22:37:20.1: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J202252.81+223720.4,2461205.6813,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J202252.81+223720.4 20260614.1813 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.58 20:18:38.31 +23:00:33.2
63.44868 -7.23766 galactic Vul Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:38.31 +23:00:33.2 (user input) | T | P | (position from user input) J-Ks=0.691+/-0.033 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:38.31 +23:00:33.2: 13.76 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:38.31 +23:00:33.2: 13.77 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1813 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.69 20:18:16.35 +24:59:08.1
65.05799 -6.07233 galactic Vul Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:16.35 +24:59:08.1 (user input) | T | P | (position from user input) J-Ks=1.019+/-0.029 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:16.35 +24:59:08.1: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:16.35 +24:59:08.1: 15.81 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.69,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.19 20:09:36.24 +22:21:24.4
61.75409 -5.84696 galactic Vul Second-epoch detections are separated by 0.4" and 6.6 pix
The object was found in VSX 2" ASASSN-V J200936.41+222124.2
Type: SR
# Max. Min./Amp. JD0 Period
13.290 V 13.410 V 2458049.00000 519.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:09:36.24 +22:21:24.4: 13.18 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:09:36.24 +22:21:24.4: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200936.41+222124.2,2461205.6813,12.19,0.05,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
ASASSN-V J200936.41+222124.2 20260614.1813 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 14.1813 2461205.6813 12.49 20:19:07.60 +24:19:07.1
64.60865 -6.60434 galactic Vul Second-epoch detections are separated by 2.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:07.60 +24:19:07.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:07.60 +24:19:07.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:07.60 +24:19:07.1: 15.79 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.49,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.64 20:19:44.53 +24:10:49.4
64.57160 -6.79784 galactic Vul Second-epoch detections are separated by 3.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.9363+24.1802 | 20:19:44.53 +24:10:49.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:44.53 +24:10:49.4: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:44.53 +24:10:49.4: 15.74 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.9363+24.1802,2461205.6813,12.64,0.05,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 J304.9363+24.1802 20260614.1813 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 14.1813 2461205.6813 11.93 20:29:27.06 +19:53:19.8
62.25389 -11.06824 galactic Del Second-epoch detections are separated by 0.4" and 6.5 pix
The object was found in VSX 2" NSVS J2029269+195319
Type: L:
# Max. Min./Amp. JD0 Period
10.956 R1 Y 0.388 R1 127.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:29:27.06 +19:53:19.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:29:27.06 +19:53:19.8: 14.78 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 14.1813* 20 29 27.06 +19 53 19.8 11.9 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2029269+195319,2461205.6813,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2029269+195319 20260614.1813 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.71 20:15:21.93 +23:54:04.4
63.78140 -6.11967 galactic Vul Second-epoch detections are separated by 0.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.8484+23.9071 | 20:15:21.93 +23:54:04.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.970+/-0.031 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:21.93 +23:54:04.4: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:21.93 +23:54:04.4: 15.86 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J303.8484+23.9071,2461205.6813,12.71,0.05,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
ATO J303.8484+23.9071 20260614.1813 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 14.1813 2461205.6813 12.45 20:19:36.32 +23:16:27.0
63.79517 -7.27578 galactic Vul Second-epoch detections are separated by 1.1" and 6.4 pix
The object was found in VSX11" Gaia DR3 1830339625043350784
Type: E
# Max. Min./Amp. JD0 Period
14.490 G 15.410 G 2.105690000000 A
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:36.32 +23:16:27.0: 13.76 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:36.32 +23:16:27.0: 13.83 +/- 0.06 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830339625043350784,2461205.6813,12.45,0.05,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
Gaia DR3 1830339625043350784 20260614.1813 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 14.1813 2461205.6813 12.50 20:16:22.76 +23:43:05.7
63.75592 -6.41396 galactic Vul Second-epoch detections are separated by 1.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:22.76 +23:43:05.7 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.037 (F)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:16:22.76 +23:43:05.7: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:16:22.76 +23:43:05.7: 15.77 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1813 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.59 20:34:17.99 +24:48:14.1
66.99540 -9.16348 galactic Vul Second-epoch detections are separated by 1.7" and 6.2 pix
The object was found in VSX 2" ASASSN-V J203418.08+244815.5
Type: SR
# Max. Min./Amp. JD0 Period
12.950 V 13.770 V 2457255.90000 417.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:34:17.99 +24:48:14.1: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:34:17.99 +24:48:14.1: 15.40 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.40 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J203418.08+244815.5,2461205.6813,12.59,0.05,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
ASASSN-V J203418.08+244815.5 20260614.1813 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 14.1813 2461205.6813 12.64 20:26:41.34 +23:10:53.0
64.63986 -8.67478 galactic Vul Second-epoch detections are separated by 1.1" and 6.2 pix
The object was found in VSX 4" Gaia DR3 1830849179960185856
Type: ROT
# Max. Min./Amp. JD0 Period
14.860 G 14.890 G K
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:26:41.34 +23:10:53.0: 14.38 +/- 0.11 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:26:41.34 +23:10:53.0: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830849179960185856,2461205.6813,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1830849179960185856 20260614.1813 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 14.1813 2461205.6813 11.90 20:16:27.05 +23:04:10.8
63.21980 -6.78450 galactic Vul Second-epoch detections are separated by 1.2" and 6.3 pix
The object was found in VSX 2" ASAS J201628+2304.2
Type: MISC
# Max. Min./Amp. JD0 Period
11.861 V Y 1.268 V 46.967738000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:16:27.05 +23:04:10.8: 13.09 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:16:27.05 +23:04:10.8: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J201628+2304.2,2461205.6813,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J201628+2304.2 20260614.1813 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.30 20:13:33.45 +23:07:15.5
62.89641 -6.19961 galactic Vul Second-epoch detections are separated by 1.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:13:33.45 +23:07:15.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:13:33.45 +23:07:15.5: 13.49 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:13:33.45 +23:07:15.5: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.30,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.44 20:12:46.59 +23:13:21.8
62.88394 -5.99365 galactic Vul Second-epoch detections are separated by 2.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:12:46.59 +23:13:21.8 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.031 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:12:46.59 +23:13:21.8: 15.03 +/- 0.25 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:12:46.59 +23:13:21.8: 13.49 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.44,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.49 20:23:26.74 +22:38:49.1
63.76776 -8.35935 galactic Vul Second-epoch detections are separated by 1.5" and 6.5 pix
The object was found in VSX 2" ASASSN-V J202326.86+223849.7
Type: SR
# Max. Min./Amp. JD0 Period
13.990 V 15.300 V 2458432.63100 110.124260800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:26.74 +22:38:49.1: 14.07 +/- 0.07 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:26.74 +22:38:49.1: 14.26 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J202326.86+223849.7,2461205.6813,12.49,0.05,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
ASASSN-V J202326.86+223849.7 20260614.1813 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 14.1813 2461205.6813 12.25 20:19:40.21 +23:46:58.6
64.22977 -7.00538 galactic Vul Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.9151+23.7825 | 20:19:40.21 +23:46:58.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.876+/-0.033 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:40.21 +23:46:58.6: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:40.21 +23:46:58.6: 15.61 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.61 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.9151+23.7825,2461205.6813,12.25,0.05,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
ATO J304.9151+23.7825 20260614.1813 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 14.1813 2461205.6813 12.55 20:16:47.43 +23:45:57.0
63.84805 -6.46627 galactic Vul Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:16:47.43 +23:45:57.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:16:47.43 +23:45:57.0: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:16:47.43 +23:45:57.0: 15.72 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.55,0.05,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 20260614.1813 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 14.1813 2461205.6813 11.61 20:23:46.74 +23:09:26.9
64.23818 -8.13627 galactic Vul Second-epoch detections are separated by 0.6" and 6.4 pix
The object was found in VSX 2" ASAS J202347+2309.5
Type: MISC
# Max. Min./Amp. JD0 Period
12.541 V Y 0.862 V 400.344066000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:46.74 +23:09:26.9: 12.96 +/- 0.03 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:46.74 +23:09:26.9: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J202347+2309.5,2461205.6813,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J202347+2309.5 20260614.1813 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.48 20:11:33.09 +22:40:44.6
62.27087 -6.05177 galactic Vul Second-epoch detections are separated by 1.9" and 6.4 pix
The object was found in VSX 2" ZTF J201133.26+224044.7
Type: SR
# Max. Min./Amp. JD0 Period
12.861 r Y 0.062 r 2458336.90870 148.226618100000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:11:33.09 +22:40:44.6: 13.37 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:11:33.09 +22:40:44.6: 13.50 +/- 0.05 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201133.26+224044.7,2461205.6813,12.48,0.05,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
ZTF J201133.26+224044.7 20260614.1813 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 14.1813 2461205.6813 12.42 20:20:06.83 +23:36:13.4
64.13666 -7.18950 galactic Vul Second-epoch detections are separated by 1.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.0345+23.6088 | 20:20:06.83 +23:36:13.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.217+/-0.031 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:20:06.83 +23:36:13.4: 14.70 +/- 0.16 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:20:06.83 +23:36:13.4: 15.45 +/- 0.29 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J305.0345+23.6088,2461205.6813,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J305.0345+23.6088 20260614.1813 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.59 20:22:33.21 +23:34:59.6
64.43445 -7.66450 galactic Vul Second-epoch detections are separated by 3.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:22:33.21 +23:34:59.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:22:33.21 +23:34:59.6: 14.46 +/- 0.11 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:22:33.21 +23:34:59.6: 14.76 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.59,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.59 20:22:20.55 +23:36:06.2
64.42256 -7.61410 galactic Vul Second-epoch detections are separated by 3.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J305.5863+23.6029 | 20:22:20.55 +23:36:06.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:22:20.55 +23:36:06.2: 14.89 +/- 0.16 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:22:20.55 +23:36:06.2: 15.81 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.89 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J305.5863+23.6029,2461205.6813,12.59,0.05,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
ATO J305.5863+23.6029 20260614.1813 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 14.1813 2461205.6813 12.59 20:15:24.28 +23:54:20.4
63.79008 -6.12471 galactic Vul Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.8484+23.9071 | 20:15:24.28 +23:54:20.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.343+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:24.28 +23:54:20.4: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:24.28 +23:54:20.4: 15.79 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J303.8484+23.9071,2461205.6813,12.59,0.05,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
ATO J303.8484+23.9071 20260614.1813 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 14.1813 2461205.6813 11.87 20:01:57.99 +22:35:02.4
61.00518 -4.23196 galactic Vul Second-epoch detections are separated by 1.9" and 6.5 pix
The object was found in VSX 1" ASAS J200158+2235.1
Type: MISC
# Max. Min./Amp. JD0 Period
9.163 Ic Y 0.349 Ic 2452577.40000 79.696000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:01:57.99 +22:35:02.4: 13.03 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:01:57.99 +22:35:02.4: 13.09 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J200158+2235.1,2461205.6813,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J200158+2235.1 20260614.1813 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.38 20:22:40.14 +23:23:18.4
64.28668 -7.79564 galactic Vul Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:22:40.14 +23:23:18.4 (user input) | T | P | (position from user input) J-Ks=0.715+/-0.029 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:22:40.14 +23:23:18.4: 13.65 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:22:40.14 +23:23:18.4: 15.11 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.75 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.38,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.66 20:23:27.27 +23:51:53.5
64.78644 -7.67689 galactic Vul Second-epoch detections are separated by 2.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1831133712958068096 | 20:23:29.12 +23:51:59.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.314+/-0.034 (F)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:27.27 +23:51:53.5: 13.74 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:27.27 +23:51:53.5: 15.80 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.74 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1831133712958068096,2461205.6813,12.66,0.05,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
Gaia DR3 1831133712958068096 20260614.1813 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 14.1813 2461205.6813 12.59 20:19:02.21 +23:34:22.9
63.97275 -7.00142 galactic Vul Second-epoch detections are separated by 3.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:02.21 +23:34:22.9 (user input) | T | P | (position from user input) J-Ks=1.008+/-0.028 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:02.21 +23:34:22.9: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:02.21 +23:34:22.9: 15.68 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.59,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.62 20:18:55.22 +23:17:20.0
63.71956 -7.13674 galactic Vul Second-epoch detections are separated by 2.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:55.22 +23:17:20.0 (user input) | T | P | (position from user input) J-Ks=0.814+/-0.030 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:55.22 +23:17:20.0: 13.75 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:55.22 +23:17:20.0: 14.00 +/- 0.07 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.62,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.61 20:14:54.22 +23:33:39.7
63.43698 -6.21789 galactic Vul Second-epoch detections are separated by 2.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.7261+23.5610 | 20:14:54.28 +23:33:39.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.420+/-0.044 (Very red! L if it's a dwarf)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:54.22 +23:33:39.7: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:54.22 +23:33:39.7: 14.75 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J303.7261+23.5610,2461205.6813,12.61,0.05,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
ATO J303.7261+23.5610 20260614.1813 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 14.1813 2461205.6813 12.27 20:19:01.66 +23:09:16.4
63.62063 -7.23171 galactic Vul Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:01.66 +23:09:16.4 (user input) | T | P | (position from user input) J-Ks=0.731+/-0.033 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:01.66 +23:09:16.4: 13.31 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:01.66 +23:09:16.4: 13.32 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.27,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.69 20:25:53.68 +23:04:27.0
64.44587 -8.58499 galactic Vul Second-epoch detections are separated by 4.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:25:53.68 +23:04:27.0 (user input) | T | P | (position from user input) J-Ks=0.798+/-0.028 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:25:53.68 +23:04:27.0: 14.17 +/- 0.07 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:25:53.68 +23:04:27.0: 13.71 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.69,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.71 20:21:15.58 +23:27:47.1
64.16658 -7.48593 galactic Vul Second-epoch detections are separated by 2.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:21:15.58 +23:27:47.1 (user input) | T | P | (position from user input) J-Ks=0.849+/-0.031 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:21:15.58 +23:27:47.1: 14.42 +/- 0.11 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:21:15.58 +23:27:47.1: 15.37 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.71,0.05,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 20260614.1813 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 14.1813 2461205.6813 11.88 20:15:52.02 +23:30:59.8
63.52151 -6.42685 galactic Vul Second-epoch detections are separated by 1.6" and 6.3 pix
The object was found in VSX 2" V0576 Vul
Type: SR
# Max. Min./Amp. JD0 Period
13.300 V 14.400 V 2457818.00000 79.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:52.02 +23:30:59.8: 14.91 +/- 0.19 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:52.02 +23:30:59.8: 14.21 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0576 Vul,2461205.6813,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0576 Vul 20260614.1813 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.27 20:15:58.86 +23:45:04.1
63.73308 -6.31975 galactic Vul Second-epoch detections are separated by 1.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:15:58.86 +23:45:04.1 (user input) | T | P | (position from user input) J-Ks=0.435+/-0.031 (G)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:58.86 +23:45:04.1: 14.58 +/- 0.12 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:58.86 +23:45:04.1: 15.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.58 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.27,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.54 20:16:46.50 +23:38:50.4
63.74658 -6.52863 galactic Vul Second-epoch detections are separated by 1.1" and 6.3 pix
The object was found in VSX 7" Gaia DR3 1830420232991956224
Type: ROT
# Max. Min./Amp. JD0 Period
17.440 G 17.470 G 0.320561000000 K
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:16:46.50 +23:38:50.4: 13.56 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:16:46.50 +23:38:50.4: 15.80 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.56 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830420232991956224,2461205.6813,12.54,0.05,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
Gaia DR3 1830420232991956224 20260614.1813 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 14.1813 2461205.6813 12.59 20:17:00.98 +24:20:22.6
64.35809 -6.19259 galactic Vul Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:17:00.98 +24:20:22.6 (user input) | T | P | (position from user input) J-Ks=0.748+/-0.027 (K)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:00.98 +24:20:22.6: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:00.98 +24:20:22.6: 15.63 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.59,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.64 20:17:06.51 +22:45:43.9
63.04506 -7.08011 galactic Vul Second-epoch detections are separated by 1.6" and 6.0 pix
The object was found in VSX 2" ASASSN-V J201706.66+224544.6
Type: SR
# Max. Min./Amp. JD0 Period
14.410 V 14.980 V 2458648.23440 234.948340800000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:06.51 +22:45:43.9: 13.84 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:06.51 +22:45:43.9: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201706.66+224544.6,2461205.6813,12.64,0.05,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
ASASSN-V J201706.66+224544.6 20260614.1813 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 14.1813 2461205.6813 12.37 20:15:23.82 +23:25:17.7
63.38204 -6.38894 galactic Vul Second-epoch detections are separated by 1.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.8482+23.4206 | 20:15:23.82 +23:25:17.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:15:23.82 +23:25:17.7: 15.02 +/- 0.18 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:15:23.82 +23:25:17.7: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J303.8482+23.4206,2461205.6813,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J303.8482+23.4206 20260614.1813 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 14.1813 2461205.6813 12.79 20:19:01.26 +24:19:06.4
64.59502 -6.58444 galactic Vul Second-epoch detections are separated by 3.1" and 6.4 pix
The object was found in VSX 1" ASASSN-V J201901.33+241907.4
Type: L
# Max. Min./Amp. JD0 Period
14.160 V 14.380 V
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:01.26 +24:19:06.4: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:01.26 +24:19:06.4: 15.78 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201901.33+241907.4,2461205.6813,12.79,0.05,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
ASASSN-V J201901.33+241907.4 20260614.1813 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 14.1813 2461205.6813 12.61 20:19:07.38 +24:06:48.0
64.43636 -6.71778 galactic Vul Second-epoch detections are separated by 1.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.7835+24.1010 | 20:19:07.38 +24:06:48.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.112+/-0.028 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:07.38 +24:06:48.0: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:07.38 +24:06:48.0: 15.63 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.63 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.7835+24.1010,2461205.6813,12.61,0.05,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
ATO J304.7835+24.1010 20260614.1813 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 14.1813 2461205.6813 12.60 20:14:44.74 +23:55:18.5
63.72055 -5.98994 galactic Vul Second-epoch detections are separated by 1.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:14:44.74 +23:55:18.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:14:44.74 +23:55:18.5: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:14:44.74 +23:55:18.5: 15.86 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.60,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.41 20:17:20.37 +23:03:05.1
63.31780 -6.96520 galactic Vul Second-epoch detections are separated by 2.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1830315813728256256 | 20:17:20.37 +23:03:05.1 (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) J-Ks=1.024+/-0.028 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:17:20.37 +23:03:05.1: 13.41 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:17:20.37 +23:03:05.1: 13.48 +/- 0.05 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830315813728256256,2461205.6813,12.41,0.05,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
Large-amplitude variable Gaia DR2 1830315813728256256 20260614.1813 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 14.1813 2461205.6813 12.38 20:22:42.21 +22:58:39.7
63.94768 -8.03237 galactic Vul Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1831014450289015424 | 20:22:42.21 +22:58:39.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.990+/-0.025 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:22:42.21 +22:58:39.7: 13.46 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:22:42.21 +22:58:39.7: 13.35 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1831014450289015424,2461205.6813,12.38,0.05,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
Large-amplitude variable Gaia DR2 1831014450289015424 20260614.1813 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 14.1813 2461205.6813 12.41 20:18:16.41 +23:46:31.2
64.04477 -6.74381 galactic Vul Second-epoch detections are separated by 2.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.5690+23.7753 | 20:18:16.41 +23:46:31.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.322+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:16.41 +23:46:31.2: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:16.41 +23:46:31.2: 15.32 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.32 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J304.5690+23.7753,2461205.6813,12.41,0.05,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
ATO J304.5690+23.7753 20260614.1813 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 14.1813 2461205.6813 12.52 20:18:28.25 +23:38:18.0
63.95509 -6.85730 galactic Vul Second-epoch detections are separated by 2.8" and 6.6 pix
The object was found in VSX 2" ASASSN-V J201828.36+233817.6
Type: SR
# Max. Min./Amp. JD0 Period
14.120 V 14.950 V 2458212.99130 238.787561200000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:28.25 +23:38:18.0: 15.12 +/- 0.20 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:28.25 +23:38:18.0: 15.30 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J201828.36+233817.6,2461205.6813,12.52,0.05,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
ASASSN-V J201828.36+233817.6 20260614.1813 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 14.1813 2461205.6813 12.38 20:19:37.10 +23:58:36.5
64.38542 -6.88769 galactic Vul Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:37.10 +23:58:36.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:37.10 +23:58:36.5: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:37.10 +23:58:36.5: 15.79 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.38,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.56 20:12:34.42 +22:46:51.2
62.48544 -6.19461 galactic Vul Second-epoch detections are separated by 1.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.1531+22.7790 | 20:12:34.42 +22:46:51.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.978+/-0.030 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:12:34.42 +22:46:51.2: 13.66 +/- 0.07 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:12:34.42 +22:46:51.2: 13.71 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.68 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J303.1531+22.7790,2461205.6813,12.56,0.05,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
ATO J303.1531+22.7790 20260614.1813 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 14.1813 2461205.6813 12.51 20:13:45.89 +22:53:30.7
62.72934 -6.36450 galactic Vul Second-epoch detections are separated by 0.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J303.4367+22.8932 | 20:13:45.89 +22:53:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.090+/-0.030 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:13:45.89 +22:53:30.7: 13.53 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:13:45.89 +22:53:30.7: 13.52 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.4367+22.8932,2461205.6813,12.51,0.05,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
ATO J303.4367+22.8932 20260614.1813 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 14.1813 2461205.6813 12.33 20:23:12.86 +25:42:58.4
66.29626 -6.58777 galactic Vul Second-epoch detections are separated by 0.7" and 6.2 pix
The object was found in VSX 1" FF Vul
Type: E/KW
# Max. Min./Amp. JD0 Period
13.100 pg 13.800 pg 2435686.45000 0.444986000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:23:12.86 +25:42:58.4: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:23:12.86 +25:42:58.4: 15.64 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FF Vul,2461205.6813,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FF Vul 20260614.1813 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.40 20:18:25.94 +22:59:55.6
63.41346 -7.20391 galactic Vul Second-epoch detections are separated by 1.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:18:25.94 +22:59:55.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:25.94 +22:59:55.6: 13.51 +/- 0.05 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:25.94 +22:59:55.6: 13.43 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.40,0.05,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 20260614.1813 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 14.1813 2461205.6813 12.57 20:13:37.19 +23:05:18.6
62.87689 -6.22933 galactic Vul Second-epoch detections are separated by 1.8" and 6.5 pix
The object was found in VSX 6" Gaia DR3 1830468645849978624
Type: S
# Max. Min./Amp. JD0 Period
16.450 G 17.510 G O
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:13:37.19 +23:05:18.6: 13.74 +/- 0.06 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:13:37.19 +23:05:18.6: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1830468645849978624,2461205.6813,12.57,0.05,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
Gaia DR3 1830468645849978624 20260614.1813 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 14.1813 2461205.6813 12.87 20:19:06.41 +24:03:24.2
64.38691 -6.74617 galactic Vul Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:06.41 +24:03:24.2 (user input) | T | P | (position from user input) J-Ks=0.887+/-0.028 (M)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:06.41 +24:03:24.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:06.41 +24:03:24.2: 15.80 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1813 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.21 20:19:48.97 +23:21:12.6
63.88878 -7.27196 galactic Vul Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:19:48.97 +23:21:12.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:48.97 +23:21:12.6: 13.53 +/- 0.04 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:48.97 +23:21:12.6: 14.30 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.6813,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.1813 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1813 2461205.6813 12.68 20:19:59.21 +23:31:59.0
64.06116 -7.20464 galactic Vul Second-epoch detections are separated by 2.9" and 6.0 pix
The object was found in VSX23" Gaia DR3 1831856985434557440
Type: E
# Max. Min./Amp. JD0 Period
19.600 G 20.190 G 47.230000000000
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:19:59.21 +23:31:59.0: 14.99 +/- 0.18 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:19:59.21 +23:31:59.0: 15.76 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.99 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1831856985434557440,2461205.6813,12.68,0.05,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 1831856985434557440 20260614.1813 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 14.1813 2461205.6813 12.40 20:18:42.83 +23:26:36.0
63.82264 -7.01170 galactic Vul Second-epoch detections are separated by 0.4" and 6.4 pix
The object was found in VSX 2" Gaia DR3 1830357354668939392
Type: ROT
# Max. Min./Amp. JD0 Period
13.170 G 13.200 G G
The object was not found in astcheck.
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:18:42.83 +23:26:36.0: 14.26 +/- 0.10 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:18:42.83 +23:26:36.0: 14.77 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1830357354668939392,2461205.6813,12.40,0.05,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
Gaia DR3 1830357354668939392 20260614.1813 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461177.93627802 17.05.2026 10:28:04.421 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
First image: 2461177.93627802 17.05.2026 10:28:04.421 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
Last image: 2461205.68156198 14.06.2026 04:21:16.955 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.69
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 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): 31074
Objects passed selection criteria: 30861
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 19387.5
Average stars matched: 18818.2 (97.0638 %)
Memory usage VmPeak: 134476 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 23:28:53 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: 2461177.93627802 17.05.2026 10:28:04.421 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
First image: 2461177.93627802 17.05.2026 10:28:04.421 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
Last image: 2461205.68156198 14.06.2026 04:21:16.955 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 464
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 50 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): 233718
Objects passed selection criteria: 232949
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 157094
Average stars matched: 150456 (95.7748 %)
Memory usage VmPeak: 2434500 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 23:37:36 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/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
SExtractor catalog cache: saved Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.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/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.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: 2461205.68099237
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_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits exists and is non-empty
Saving wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits to local_wcs_cache/
'wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits' -> 'local_wcs_cache/wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits'
wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits exists and is non-empty
Saving wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits to local_wcs_cache/
'wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits' -> 'local_wcs_cache/wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits'
wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits'
wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits (1st reference image)
verification OK: wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
Image size: 937.9'x598.2' 15.6(deg)x10.0(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.62"/pix along the Y axis
Image center: 20:18:29.135 +22:00:01.47 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/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_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits (1st new image)
verification OK: wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
Image size: 942.6'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 20:18:19.690 +21:56:50.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:18:29.135 +22:00:01.47
Second-epoch image center 20:18:19.690 +21:56:50.08
Angular distance between the image centers 0.0645 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits (2nd new image)
verification OK: wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
Image size: 942.6'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 20:18:17.135 +21:57:04.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:18:29.135 +22:00:01.47
Second-epoch image center 20:18:17.135 +21:57:04.86
Angular distance between the image centers 0.0675 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 20:18:19.690 +21:56:50.08
Second-epoch second image center 20:18:17.135 +21:57:04.86
Angular distance between the image centers 0.01069 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/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits &> /tmp/tmp.TbcEm80bDU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits &> /tmp/tmp.Fyl7QqU4oE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits &> /tmp/tmp.NL8PU9cQwo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits &> /tmp/tmp.RPRdQfvMBb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.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_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits and wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.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_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits and wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat
Found non-empty wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits and wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat
The reference image (wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits) and catalog (wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat) found
'wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat' -> 'wcsmag.cat'
Read 33800 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 296.0492 to 313.3855 deg, Dec +16.6404 to +27.1058 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 296.0492 to 313.3855 deg, Dec 16.6404 to 27.1058 deg
Loaded 22937 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): 461 out of 514 total matches.
Matched with Tycho-2 514 out of 33800 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.708700
a=0.000000 b=1.000000 c=22.708700
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 33800 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 296.0492 to 313.3855 deg, Dec +16.6404 to +27.1058 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 296.0492 to 313.3855 deg, Dec 16.6404 to 27.1058 deg
Loaded 22937 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): 461 out of 514 total matches.
Matched with Tycho-2 514 out of 33800 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits:
Forced-photometry filter: calibrated wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits -> calib.txt_param_ref_wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits (aperture=6.3)
Read 33277 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 295.8260 to 313.1957 deg, Dec +16.5624 to +27.4485 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 295.8260 to 313.1957 deg, Dec 16.5624 to 27.4485 deg
Loaded 23846 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): 480 out of 547 total matches.
Matched with Tycho-2 547 out of 33277 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits:
Forced-photometry filter: calibrated wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits -> calib.txt_param_ref_wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
2.3 pix Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
2.5 pix fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
2.5 pix fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
2.3 pix wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
2.3 pix wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
Limiting magnitude estimates:
15.0 mag. Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
15.0 mag. Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
12.7 mag. fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
12.7 mag. fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 10.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.TbcEm80bDU (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/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.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_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits' -> 'wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
WCS-calibrated image found: wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
Checking if the catalog wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat corresponding to the image wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat corresponding to the image wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits
WCS catalog name: wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3526, passed=33800
Got 33800 stars (including 30252 good ones) from the SExtractor catalog wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat
util/solve_plate_with_UCAC5 got 33800 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 533 to 587 (Dec 16.6 to 27.1)
Done reading UCAC5 zone files...
Matched 526 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 434 matched stars entering correct_measured_positions(), 386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 422 matched stars entering correct_measured_positions(), 15513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.99"
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 533 to 587 (Dec 16.6 to 27.1)
Done reading UCAC5 zone files...
Matched 604 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 538 matched stars entering correct_measured_positions(), 15555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.93"
Accuracy estimation diagnostic: 537 matched stars entering correct_measured_positions(), 19339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.90"
Excluding outliers - 537 stars left (next iteration limit 464)
WCS_QUALITY_DIAG: file=Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits N_match=537 sigma_overall_arcsec=9.253 sigma_q1_arcsec=17.023 sigma_q2_arcsec=11.034 sigma_q3_arcsec=10.554 sigma_q4_arcsec=3.946 n_q1=135 n_q2=165 n_q3=89 n_q4=148 worst_quadrant_to_overall_ratio=1.840
The image catalog is written to wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits -region wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.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.Fyl7QqU4oE (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/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.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_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits' -> 'wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
WCS-calibrated image found: wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
Checking if the catalog wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits.wcscat corresponding to the image wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits.wcscat corresponding to the image wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits
WCS catalog name: wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3468, passed=33277
Got 33277 stars (including 29783 good ones) from the SExtractor catalog wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits.wcscat
util/solve_plate_with_UCAC5 got 33277 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.5'
Seting catalog search parameters based on the expected field of view 936.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013007 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010406 (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 532 to 589 (Dec 16.6 to 27.4)
Done reading UCAC5 zone files...
Matched 570 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 464 matched stars entering correct_measured_positions(), 417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 450 matched stars entering correct_measured_positions(), 15535 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 589 (Dec 16.6 to 27.5)
Done reading UCAC5 zone files...
Matched 614 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 557 matched stars entering correct_measured_positions(), 15587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.59"
Accuracy estimation diagnostic: 554 matched stars entering correct_measured_positions(), 19210 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.10"
Excluding outliers - 554 stars left (next iteration limit 495)
WCS_QUALITY_DIAG: file=Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits N_match=554 sigma_overall_arcsec=7.529 sigma_q1_arcsec=9.050 sigma_q2_arcsec=6.227 sigma_q3_arcsec=6.570 sigma_q4_arcsec=10.848 n_q1=159 n_q2=201 n_q3=105 n_q4=89 worst_quadrant_to_overall_ratio=1.441
The image catalog is written to wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits -region wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.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.NL8PU9cQwo (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_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.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_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
Checking if the catalog wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits.wcscat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits.wcscat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.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_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
WCS catalog name: wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=204, passed=5594
Got 5594 stars (including 5384 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits.wcscat
util/solve_plate_with_UCAC5 got 5594 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 5274 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 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 5273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 5264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 929 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits N_match=929 sigma_overall_arcsec=0.426 sigma_q1_arcsec=0.518 sigma_q2_arcsec=0.576 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.366 n_q1=118 n_q2=116 n_q3=327 n_q4=368 worst_quadrant_to_overall_ratio=1.351
The image catalog is written to wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits -region wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.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.RPRdQfvMBb (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_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.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_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
Checking if the catalog wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits.wcscat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits.wcscat corresponding to the image wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.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_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
WCS catalog name: wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=183, passed=5324
Got 5324 stars (including 5135 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits.wcscat
util/solve_plate_with_UCAC5 got 5324 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 4978 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 4979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 4972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 924 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits N_match=924 sigma_overall_arcsec=0.408 sigma_q1_arcsec=0.524 sigma_q2_arcsec=0.506 sigma_q3_arcsec=0.397 sigma_q4_arcsec=0.334 n_q1=105 n_q2=137 n_q3=268 n_q4=414 worst_quadrant_to_overall_ratio=1.285
The image catalog is written to wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits -region wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.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=Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits sigma_overall=9.253 worst_q_ratio=1.840
ref2=Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits sigma_overall=7.529 worst_q_ratio=1.441
new1=fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits sigma_overall=0.426 worst_q_ratio=1.351
new2=fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits sigma_overall=0.408 worst_q_ratio=1.285
reference average sigma_overall=8.391 worst_q_ratio=1.6405
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315_astrometric_residuals.png (537 matched stars from wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 4.59 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316_astrometric_residuals.png (554 matched stars from wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062_astrometric_residuals.png (929 matched stars from wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063_astrometric_residuals.png (924 matched stars from wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-20-27_20.00sec_-0.00C_LIGHTs_0062.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Vul-02-Q1b1x1_232326_TTUQ1b1x1_2269204_am0iFkYc/wcs_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063.fits'
Preparing the HTML report for the field Vul-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:42:36.71 +16:41:34.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:42:36.71 +16:41:34.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 20:42:36.71 +16:41:34.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-04_20.00sec_-0.00C_LIGHT_1315.fits at 20:27:25.00 +23:26:56.7: 12.33 +/- 0.02 detection
Forced photometry on wcs_Vul-02-Q1b1x1_2026-05-17_05-28-49_20.00sec_-0.00C_LIGHT_1316.fits at 20:27:25.00 +23:26:56.7: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter KEPT candidate at 20:27:25.00 +23:26:56.7: ref_mag=12.45 +/- 0.01 new_mean_mag=10.9522 delta=1.50 (need > 0.90)
Adding exclusion_list_local.txt__out22993.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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 52110_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 52110_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:26.17 +16:54:11.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52117_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 52117_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:46.39 +16:46:11.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52123_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 52123_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:43:04.83 +17:05:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52134_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 52134_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:40:54.16 +17:34:13.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52137_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 52137_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:32.32 +16:54:09.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52144_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 52144_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:43:27.93 +16:56:39.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52182_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 52182_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:14.40 +17:58:45.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52228_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 52228_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:16:27.57 +23:43:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.960 1830608588770832512 304.11541904341 +23.73175235897 13.4420 12.4706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.960#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293854_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293854_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:34:36.65 +21:03:12.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293859_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293859_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:52:27.84 +20:44:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293860_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293860_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:23:23.46 +21:00:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.975 1817034847146912896 305.84663897055 +21.00659352643 12.9189 12.4261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293861_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293861_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:44:05.34 +26:14:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293862_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293862_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:34:46.93 +25:53:05.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293869_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293869_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:18.11 +25:19:45.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293872_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293872_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:56:28.37 +19:55:50.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293875_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293875_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:01:41.83 +25:14:12.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293877_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293877_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:29:56.42 +21:50:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293878_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293878_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:59:14.39 +21:37:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293881_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293881_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:22:05.92 +27:00:17.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293882_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293882_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293883_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293883_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:04.03 +26:19:07.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293890_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293890_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:26.16 +16:54:11.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293896_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293896_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:46.41 +16:46:11.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293916_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293916_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:40:54.15 +17:34:14.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293918_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293918_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:32.31 +16:54:09.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293926_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293926_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:43:27.91 +16:56:40.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293966_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 293966_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:14.37 +17:58:45.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294014_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294014_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294030_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294030_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:49.60 +16:44:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294034_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294034_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:44:44.69 +17:14:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294079_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294079_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:37.24 +16:49:37.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294084_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294084_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:39.29 +18:46:26.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294086_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294086_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:40:21.74 +20:52:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294095_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294095_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:37:35.85 +16:53:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294110_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294110_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:42:07.00 +16:48:48.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294122_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294122_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294181_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294181_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:44:36.35 +17:27:15.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294220_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294220_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:11.18 +16:53:44.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294223_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294223_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:45:46.43 +17:28:11.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294224_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294224_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:00.75 +16:44:03.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294230_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294230_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294235_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294235_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:43.70 +17:34:30.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294244_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294244_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:49:08.92 +17:00:54.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294268_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294268_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:50:01.35 +19:54:48.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294283_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294283_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294286_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294286_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:56.74 +16:52:29.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294307_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294307_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:45:56.81 +17:10:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294322_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294322_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:38:30.15 +21:10:11.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294323_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294323_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:51:00.11 +25:57:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294328_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294328_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:59:11.03 +23:04:04.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294335_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294335_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:45:36.14 +17:14:12.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294341_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294341_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:55.69 +18:37:50.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294344_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294344_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:45:41.28 +18:34:33.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294345_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294345_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:43:18.79 +17:03:25.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294347_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294347_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:37:38.94 +17:10:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294360_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294360_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:53:35.88 +22:58:32.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294366_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294366_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:36.82 +16:59:46.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294372_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294372_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294382_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294382_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:43:37.03 +17:04:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294386_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294386_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:40:12.97 +17:31:03.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294388_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294388_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:23:00.88 +26:12:47.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294389_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294389_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:44:03.83 +17:22:53.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294401_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294401_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:42.75 +19:51:31.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294403_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294403_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:13.96 +16:50:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294409_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294409_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:59:07.81 +23:04:41.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294412_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294412_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:44:39.45 +17:16:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294427_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294427_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294433_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294433_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:44:40.37 +18:16:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294441_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294441_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:44:11.99 +18:36:19.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294442_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294442_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294445_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294445_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:17.68 +17:31:39.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294451_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294451_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:39:06.36 +17:13:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294465_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294465_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:38:06.43 +17:01:10.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294482_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294482_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294488_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294488_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:18:47.40 +27:00:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.229 1836077353446582784 304.69761016864 +27.01189156038 12.2050 11.3211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294516_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294516_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:38:05.07 +17:15:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294524_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294524_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:10:39.00 +26:55:53.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294553_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294553_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:36:05.41 +16:52:05.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294566_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294566_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:49:01.72 +16:44:51.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294567_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294567_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:16:52.25 +24:41:42.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294571_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294571_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:49:10.74 +17:31:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294580_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294580_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:48.46 +17:13:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294592_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294592_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:31.23 +16:40:52.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294594_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294594_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:30:44.17 +25:45:02.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294598_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294598_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294607_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294607_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:39:23.01 +26:02:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294610_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294610_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:16:53.49 +27:02:11.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294611_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294611_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:25:49.48 +26:42:31.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294617_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294617_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:49:13.44 +17:11:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294634_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294634_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:58.26 +16:54:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294635_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294635_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:49:18.03 +16:59:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294644_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294644_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:16.19 +16:39:54.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294656_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294656_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:59:15.40 +23:07:26.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294658_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294658_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:45:51.29 +18:33:09.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294659_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294659_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294684_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294684_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:42:37.96 +18:23:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294692_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294692_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294700_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294700_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:03:34.76 +21:28:56.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294706_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294706_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:38:52.61 +17:00:30.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294735_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294735_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:44:48.16 +17:18:04.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294745_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294745_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:23:14.46 +24:00:39.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294748_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294748_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:28.42 +16:50:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294762_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294762_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:37:10.08 +16:50:28.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294773_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294773_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:37.92 +19:14:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294779_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294779_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:48:53.41 +17:14:55.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294780_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294780_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294799_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294799_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:40:42.41 +26:03:16.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294821_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294821_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294827_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294827_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294837_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294837_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:11:15.49 +21:53:27.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294843_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294843_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294866_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294866_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:36:46.24 +17:04:10.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294874_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294874_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:19:28.08 +23:00:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 2.773 1829575704980712064 304.86763396410 +23.01255858431 12.8441 11.8954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294878_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294878_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:23:29.04 +23:38:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294884_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294884_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:41:17.24 +18:02:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294885_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294885_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:28:32.47 +25:53:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294895_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294895_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:45:01.89 +18:40:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294909_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294909_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 294917_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294917_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:45:10.65 +17:01:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294928_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294928_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:29:58.51 +21:49:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294954_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294954_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:22:44.36 +24:03:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294957_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294957_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 294970_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294970_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:44:28.05 +18:23:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294971_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294971_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:05.59 +19:17:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294975_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294975_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:20:32.02 +26:42:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294984_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294984_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:54:56.01 +23:28:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294997_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 294997_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:40:52.08 +17:37:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295009_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295009_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:45:39.72 +16:57:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295020_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295020_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:45:43.55 +17:14:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295065_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295065_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:15:11.45 +24:52:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.798 1835224201137873152 303.79820380396 +24.87099542249 13.2562 12.4425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 295073_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295073_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:53:47.25 +18:46:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295074_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295074_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 295087_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295087_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:15.55 +17:55:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295088_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295088_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295090_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295090_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:47:52.68 +16:41:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295095_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295095_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:39:07.64 +17:21:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295101_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295101_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 295130_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295130_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:08:38.33 +22:10:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.962 1829921531434674560 302.16029101793 +22.16695084276 12.8576 11.9809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 295142_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295142_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:25:14.77 +25:41:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295146_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295146_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 295152_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295152_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:19:40.59 +24:13:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.505 1831963878598495360 304.92019120308 +24.23013467874 13.1677 12.2221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 295160_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295160_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:11:12.94 +21:52:37.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 295166_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295166_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:45:03.53 +17:32:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295175_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295175_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:24:28.90 +25:11:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295204_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295204_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:36:01.98 +25:53:21.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 295206_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295206_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:17:36.25 +26:21:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295220_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295220_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:40:25.81 +17:51:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295237_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295237_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:46.05 +18:59:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295259_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295259_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:37:09.62 +17:01:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295274_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295274_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:39:33.50 +20:52:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295283_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295283_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 295298_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295298_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:00:32.48 +22:40:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 0.683 1827242266446049920 300.13553632239 +22.67091949059 11.1840 9.6383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 295316_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295316_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295358_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295358_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:15:23.62 +23:44:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.700 1830601137014429568 303.84918884228 +23.74322292265 13.7521 13.2073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 295367_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295367_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 295376_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295376_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:59:01.70 +23:05:57.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 295391_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 295391_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:03:32.50 +21:48:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162860_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 162860_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:57:56.79 +22:40:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189791_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 189791_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 198859_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 198859_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 171515_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 171515_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 180452_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 180452_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:57:12.00 +23:23:15.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)
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Considering the candidate 189943_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 189943_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 180998_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 180998_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 195654_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 195654_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 170912_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 170912_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 181371_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 181371_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 175492_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 175492_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 190746_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 190746_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 199755_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 199755_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167888_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 167888_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179798_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 179798_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173273_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 173273_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 102725_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 102725_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169795_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 169795_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116491_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 116491_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 167335_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 167335_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183781_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 183781_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170300_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 170300_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180223_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 180223_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178630_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 178630_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153452_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 153452_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183219_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 183219_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174677_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 174677_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170580_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 170580_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172671_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 172671_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180374_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 180374_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182670_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 182670_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177602_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 177602_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172841_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 172841_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166208_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 166208_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151563_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 151563_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177964_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 177964_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:13:16.91 +23:22:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155543_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 155543_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:08:07.44 +22:31:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177018_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 177018_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154645_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 154645_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159256_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 159256_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187701_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 187701_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184860_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 184860_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146113_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 146113_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166497_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 166497_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173595_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 173595_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181671_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 181671_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165901_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 165901_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191814_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 191814_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200983_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 200983_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187940_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 187940_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196687_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 196687_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178679_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 178679_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199311_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 199311_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:13:24.25 +24:18:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208277_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 208277_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:26:50.17 +24:43:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196200_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 196200_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169106_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 169106_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181899_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 181899_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163321_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 163321_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183270_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 183270_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:19:25.20 +23:37:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159784_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 159784_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171832_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 171832_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118022_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 118022_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187741_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 187741_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208294_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 208294_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136268_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 136268_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:02:57.31 +21:41:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183544_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 183544_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198051_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 198051_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172512_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 172512_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185520_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 185520_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188320_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 188320_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171075_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 171075_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175151_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 175151_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194891_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 194891_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 231213_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 231213_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:53:48.34 +25:34:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156699_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 156699_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176646_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 176646_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169311_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 169311_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196029_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 196029_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 95676_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 95676_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:30:11.64 +20:23:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174238_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 174238_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 160214_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 160214_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 195440_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 195440_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245979_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 245979_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173544_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 173544_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 195246_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 195246_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 188892_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 188892_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:14:47.19 +23:48:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 3.306 1830604156363361024 303.69760711984 +23.80469871555 12.4089 11.3060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150653_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 150653_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166641_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 166641_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181292_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 181292_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162295_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 162295_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 168082_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 168082_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165091_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 165091_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 198569_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 198569_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 184348_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 184348_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179779_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 179779_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176127_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 176127_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116026_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 116026_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117156_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 117156_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:00:44.92 +21:05:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187316_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 187316_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186374_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 186374_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179540_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 179540_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170246_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 170246_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192112_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 192112_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171612_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 171612_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173021_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 173021_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152832_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 152832_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170689_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 170689_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180316_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 180316_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170174_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 170174_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172425_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 172425_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178514_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 178514_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204651_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 204651_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170064_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 170064_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190424_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 190424_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182326_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 182326_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 167389_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 167389_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186817_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 186817_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152936_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 152936_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:15:38.01 +22:27:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 179140_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 179140_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 184224_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 184224_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157722_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 157722_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194894_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 194894_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172697_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 172697_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179721_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 179721_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 190472_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 190472_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173628_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 173628_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136471_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 136471_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 193585_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 193585_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 166679_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 166679_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202372_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 202372_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170511_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 170511_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195254_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 195254_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188202_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 188202_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 174604_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 174604_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165132_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 165132_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 199430_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 199430_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179541_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 179541_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 182538_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 182538_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:23:11.93 +23:33:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191845_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 191845_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197300_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 197300_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181633_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 181633_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187069_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 187069_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 19:57:52.79 +23:37:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157833_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 157833_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 167755_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 167755_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 246344_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 246344_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151391_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 151391_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 199127_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 199127_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 196347_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 196347_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 16946_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 16946_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:46:36.69 +17:22:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81234_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 81234_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 190009_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 190009_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 166343_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 166343_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:36:42.16 +22:54:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174748_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 174748_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 185866_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 185866_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 249260_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 249260_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 172516_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 172516_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 169835_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 169835_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 171013_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 171013_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 173625_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 173625_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 158009_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 158009_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 198519_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 198519_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
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Considering the candidate 187235_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 187235_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 186755_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 186755_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 172084_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 172084_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 159309_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 159309_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 182944_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 182944_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 182626_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 182626_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 182904_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 182904_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 190029_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 190029_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 158837_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 158837_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 177684_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 177684_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 137305_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 137305_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:06:02.27 +21:49:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188996_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 188996_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 182200_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 182200_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 175104_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 175104_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 181960_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 181960_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 171652_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 171652_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 169579_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 169579_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 179814_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 179814_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 181158_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 181158_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 186436_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 186436_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 184114_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 184114_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 199518_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 199518_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 161349_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 161349_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 178893_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 178893_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 199065_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 199065_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 194471_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 194471_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 190473_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 190473_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 168999_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 168999_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 271878_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 271878_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:16:44.71 +24:53:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.613 1832248171075795968 304.18673095930 +24.88609351862 13.6606 13.0720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167073_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 167073_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 187010_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 187010_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 183865_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 183865_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 191565_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 191565_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 162007_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 162007_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 257312_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
The candidate 257312_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063 did not pass the final checks
**** FOUND 20:17:37.22 +26:53:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164831_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 164831_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 230849_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 230849_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 167585_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 167585_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 170155_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 170155_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 193239_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 193239_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 176791_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 176791_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 181108_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 181108_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
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Considering the candidate 179148_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
Preparing report for the candidate 179148_fd_Vul-02-Q1b1x1_2026-06-13_23-21-16_20.00sec_-0.00C_LIGHTs_0063
make_report_in_HTML.sh Phase 2 (HTML assembly): 13s
make_report_in_HTML.sh TOTAL: 290s
Prepared the HTML report for the field Vul-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:27:25.00 +23:26:56.7
20:32:06.83 +20:39:08.3
20:30:19.38 +21:06:49.9
20:26:47.98 +21:11:16.6
20:25:28.11 +21:50:31.3
20:23:52.00 +22:11:29.8
20:23:12.59 +22:21:31.5
20:09:36.24 +22:21:24.4
20:22:39.53 +22:24:00.1
20:14:50.01 +22:26:23.0
20:23:34.94 +22:27:35.4
20:21:51.27 +22:31:05.7
20:22:12.40 +22:35:35.5
20:08:52.27 +22:36:04.1
20:22:52.68 +22:37:20.1
20:23:26.74 +22:38:49.1
20:01:57.99 +22:35:02.4
20:27:03.70 +22:40:42.4
20:11:33.09 +22:40:44.6
20:11:23.36 +22:41:21.9
20:21:59.75 +22:43:25.2
20:17:06.51 +22:45:43.9
20:12:34.42 +22:46:51.2
20:20:25.79 +22:50:29.7
20:13:45.89 +22:53:30.7
20:23:04.80 +22:54:38.6
20:18:35.60 +22:54:41.2
20:18:01.86 +22:56:24.8
20:19:07.28 +22:57:03.6
20:18:41.39 +22:57:37.7
20:17:28.92 +22:57:52.5
20:15:46.06 +22:57:45.7
20:22:42.21 +22:58:39.7
20:17:35.60 +22:59:09.7
20:18:40.19 +22:59:37.7
20:18:25.94 +22:59:55.6
20:18:38.31 +23:00:33.2
20:13:26.81 +22:59:53.1
20:19:02.12 +23:01:14.4
20:17:20.37 +23:03:05.1
20:18:55.93 +23:03:42.1
20:17:45.56 +23:03:50.7
20:25:53.68 +23:04:27.0
20:21:41.24 +23:04:49.3
20:16:27.05 +23:04:10.8
20:23:04.63 +23:05:54.5
20:13:37.19 +23:05:18.6
20:19:37.91 +23:05:43.5
20:22:46.53 +23:06:20.7
20:19:08.58 +23:06:10.5
20:17:43.69 +23:06:52.6
20:19:40.58 +23:06:45.1
20:19:37.76 +23:06:32.2
20:16:37.88 +23:06:36.9
20:13:33.45 +23:07:15.5
20:14:24.38 +23:07:33.9
20:19:31.65 +23:09:14.8
20:18:10.49 +23:09:22.8
20:19:01.66 +23:09:16.4
20:14:31.75 +23:09:11.9
20:23:46.74 +23:09:26.9
20:18:28.04 +23:11:01.8
20:18:36.33 +23:11:17.1
20:26:41.34 +23:10:53.0
20:20:13.86 +23:11:39.9
20:20:02.81 +23:11:46.8
20:18:54.67 +23:11:49.1
20:14:02.44 +23:12:03.1
20:13:46.81 +23:13:04.3
20:25:23.34 +23:12:25.1
20:12:46.59 +23:13:21.8
20:21:39.38 +23:14:06.8
20:21:00.10 +23:15:20.0
20:18:57.60 +23:16:23.1
20:24:07.18 +23:16:29.3
20:19:36.32 +23:16:27.0
20:18:55.22 +23:17:20.0
20:14:18.66 +23:16:57.2
20:23:45.75 +23:18:06.7
20:12:57.35 +23:18:54.0
20:14:28.85 +23:20:02.8
20:19:48.97 +23:21:12.6
20:17:50.89 +23:21:37.3
20:24:40.42 +23:23:01.0
20:22:40.14 +23:23:18.4
20:18:16.35 +23:25:22.4
20:18:36.22 +23:25:39.9
20:18:39.74 +23:25:31.1
20:15:23.82 +23:25:17.7
20:18:42.83 +23:26:36.0
20:23:40.99 +23:27:45.3
20:23:45.85 +23:27:44.0
20:18:46.17 +23:28:12.9
20:19:25.08 +23:28:38.5
20:21:15.58 +23:27:47.1
20:26:30.94 +23:29:03.1
20:13:56.23 +23:29:05.4
20:18:37.75 +23:28:46.6
20:18:23.54 +23:31:23.8
20:19:59.21 +23:31:59.0
20:15:52.02 +23:30:59.8
20:19:02.45 +23:32:09.7
20:15:15.95 +23:31:59.5
20:18:41.36 +23:32:44.5
20:19:15.78 +23:33:07.6
20:17:59.47 +23:33:41.6
20:14:54.22 +23:33:39.7
20:19:02.21 +23:34:22.9
20:22:33.21 +23:34:59.6
20:22:20.55 +23:36:06.2
20:20:06.83 +23:36:13.4
20:14:42.77 +23:36:31.4
20:15:26.19 +23:37:25.0
20:20:45.40 +23:37:30.3
20:18:28.25 +23:38:18.0
20:16:46.50 +23:38:50.4
20:16:46.15 +23:39:25.9
20:12:57.05 +23:39:07.6
20:18:45.82 +23:41:06.2
20:19:54.65 +23:42:39.3
20:16:22.76 +23:43:05.7
20:14:40.28 +23:44:03.1
20:15:58.86 +23:45:04.1
20:16:47.43 +23:45:57.0
20:15:49.06 +23:46:14.4
20:18:16.41 +23:46:31.2
20:19:40.21 +23:46:58.6
20:19:20.82 +23:47:36.0
20:19:13.10 +23:48:41.8
20:15:40.67 +23:47:48.2
20:19:32.91 +23:49:30.8
20:20:11.91 +23:50:00.5
20:19:07.33 +23:50:31.1
20:23:27.27 +23:51:53.5
20:22:26.00 +23:52:46.0
20:15:28.35 +23:54:07.5
20:15:21.93 +23:54:04.4
20:15:24.28 +23:54:20.4
20:16:34.82 +23:55:41.4
20:14:26.27 +23:55:18.5
20:14:44.74 +23:55:18.5
20:27:50.30 +23:55:49.5
20:19:37.10 +23:58:36.5
20:19:58.50 +23:59:34.2
20:20:05.96 +23:59:41.3
20:21:04.73 +23:59:58.4
20:19:06.41 +24:03:24.2
20:15:47.40 +24:03:53.9
20:19:07.38 +24:06:48.0
20:19:26.11 +24:07:44.6
20:23:46.41 +24:07:33.9
20:16:37.13 +24:06:43.1
20:21:03.59 +24:08:50.5
20:27:47.52 +24:08:40.9
20:19:56.50 +24:09:40.9
20:17:05.18 +24:10:42.5
20:14:48.97 +24:10:43.3
20:19:44.53 +24:10:49.4
20:23:31.80 +24:12:35.5
20:28:25.05 +24:13:43.6
20:20:26.10 +24:16:27.2
20:16:05.07 +24:17:55.9
20:28:42.22 +24:18:09.9
20:19:01.26 +24:19:06.4
20:19:07.60 +24:19:07.1
20:17:20.32 +24:20:12.9
20:17:00.98 +24:20:22.6
20:16:26.22 +24:21:00.1
20:19:05.11 +24:23:29.0
20:15:44.83 +24:28:19.7
20:18:13.34 +24:34:56.0
20:23:49.18 +24:45:14.6
20:23:12.86 +25:42:58.4
20:17:43.06 +24:59:39.7
20:18:16.35 +24:59:08.1
20:34:17.99 +24:48:14.1
20:29:27.06 +19:53:19.8
########### Completed Vul-02-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 ####
20:27:25.00 +23:26:56.7
20:22:26.00 +23:52:46.0
20:28:42.22 +24:18:09.9
20:19:31.65 +23:09:14.8
20:15:28.35 +23:54:07.5
20:18:23.54 +23:31:23.8
20:19:56.50 +24:09:40.9
20:16:37.88 +23:06:36.9
20:15:15.95 +23:31:59.5
20:23:45.75 +23:18:06.7
20:27:50.30 +23:55:49.5
20:16:26.22 +24:21:00.1
20:13:26.81 +22:59:53.1
20:19:25.08 +23:28:38.5
20:32:06.83 +20:39:08.3
20:21:41.24 +23:04:49.3
20:30:19.38 +21:06:49.9
20:17:35.60 +22:59:09.7
20:20:45.40 +23:37:30.3
20:19:08.58 +23:06:10.5
20:26:30.94 +23:29:03.1
20:18:36.22 +23:25:39.9
20:23:34.94 +22:27:35.4
20:14:42.77 +23:36:31.4
20:24:07.18 +23:16:29.3
20:19:40.58 +23:06:45.1
20:20:13.86 +23:11:39.9
20:18:37.75 +23:28:46.6
20:24:40.42 +23:23:01.0
20:18:54.67 +23:11:49.1
20:19:07.28 +22:57:03.6
20:22:39.53 +22:24:00.1
20:17:50.89 +23:21:37.3
20:21:51.27 +22:31:05.7
20:27:03.70 +22:40:42.4
20:19:13.10 +23:48:41.8
20:18:45.82 +23:41:06.2
20:23:52.00 +22:11:29.8
20:18:41.39 +22:57:37.7
20:25:23.34 +23:12:25.1
20:19:15.78 +23:33:07.6
20:18:01.86 +22:56:24.8
20:19:58.50 +23:59:34.2
20:19:05.11 +24:23:29.0
20:19:32.91 +23:49:30.8
20:23:31.80 +24:12:35.5
20:18:39.74 +23:25:31.1
20:14:48.97 +24:10:43.3
20:18:55.93 +23:03:42.1
20:17:59.47 +23:33:41.6
20:20:25.79 +22:50:29.7
20:11:23.36 +22:41:21.9
20:14:31.75 +23:09:11.9
20:26:47.98 +21:11:16.6
20:15:40.67 +23:47:48.2
20:23:49.18 +24:45:14.6
20:15:26.19 +23:37:25.0
20:20:26.10 +24:16:27.2
20:18:36.33 +23:11:17.1
20:19:54.65 +23:42:39.3
20:19:07.33 +23:50:31.1
20:14:24.38 +23:07:33.9
20:14:18.66 +23:16:57.2
20:19:26.11 +24:07:44.6
20:22:12.40 +22:35:35.5
20:14:28.85 +23:20:02.8
20:17:45.56 +23:03:50.7
20:17:05.18 +24:10:42.5
20:21:00.10 +23:15:20.0
20:21:59.75 +22:43:25.2
20:27:47.52 +24:08:40.9
20:17:43.06 +24:59:39.7
20:13:46.81 +23:13:04.3
20:16:37.13 +24:06:43.1
20:23:12.59 +22:21:31.5
20:17:28.92 +22:57:52.5
20:19:02.45 +23:32:09.7
20:19:02.12 +23:01:14.4
20:23:04.80 +22:54:38.6
20:16:05.07 +24:17:55.9
20:12:57.05 +23:39:07.6
20:18:46.17 +23:28:12.9
20:12:57.35 +23:18:54.0
20:19:20.82 +23:47:36.0
20:14:40.28 +23:44:03.1
20:23:40.99 +23:27:45.3
20:22:46.53 +23:06:20.7
20:21:04.73 +23:59:58.4
20:18:10.49 +23:09:22.8
20:14:02.44 +23:12:03.1
20:14:50.01 +22:26:23.0
20:19:37.76 +23:06:32.2
20:13:56.23 +23:29:05.4
20:19:37.91 +23:05:43.5
20:18:28.04 +23:11:01.8
20:18:16.35 +23:25:22.4
20:18:13.34 +24:34:56.0
20:23:04.63 +23:05:54.5
20:16:34.82 +23:55:41.4
20:18:40.19 +22:59:37.7
20:15:49.06 +23:46:14.4
20:16:46.15 +23:39:25.9
20:08:52.27 +22:36:04.1
20:23:46.41 +24:07:33.9
20:20:02.81 +23:11:46.8
20:14:26.27 +23:55:18.5
20:21:39.38 +23:14:06.8
20:25:28.11 +21:50:31.3
20:15:47.40 +24:03:53.9
20:15:46.06 +22:57:45.7
20:15:44.83 +24:28:19.7
20:17:43.69 +23:06:52.6
20:21:03.59 +24:08:50.5
20:20:11.91 +23:50:00.5
20:18:57.60 +23:16:23.1
20:18:35.60 +22:54:41.2
20:17:20.32 +24:20:12.9
20:23:45.85 +23:27:44.0
20:20:05.96 +23:59:41.3
20:28:25.05 +24:13:43.6
20:18:41.36 +23:32:44.5
20:22:52.68 +22:37:20.1
20:18:38.31 +23:00:33.2
20:18:16.35 +24:59:08.1
20:09:36.24 +22:21:24.4
20:19:07.60 +24:19:07.1
20:19:44.53 +24:10:49.4
20:29:27.06 +19:53:19.8
20:15:21.93 +23:54:04.4
20:19:36.32 +23:16:27.0
20:16:22.76 +23:43:05.7
20:34:17.99 +24:48:14.1
20:26:41.34 +23:10:53.0
20:16:27.05 +23:04:10.8
20:13:33.45 +23:07:15.5
20:12:46.59 +23:13:21.8
20:23:26.74 +22:38:49.1
20:19:40.21 +23:46:58.6
20:16:47.43 +23:45:57.0
20:23:46.74 +23:09:26.9
20:11:33.09 +22:40:44.6
20:20:06.83 +23:36:13.4
20:22:33.21 +23:34:59.6
20:22:20.55 +23:36:06.2
20:15:24.28 +23:54:20.4
20:01:57.99 +22:35:02.4
20:22:40.14 +23:23:18.4
20:23:27.27 +23:51:53.5
20:19:02.21 +23:34:22.9
20:18:55.22 +23:17:20.0
20:14:54.22 +23:33:39.7
20:19:01.66 +23:09:16.4
20:25:53.68 +23:04:27.0
20:21:15.58 +23:27:47.1
20:15:52.02 +23:30:59.8
20:15:58.86 +23:45:04.1
20:16:46.50 +23:38:50.4
20:17:00.98 +24:20:22.6
20:17:06.51 +22:45:43.9
20:15:23.82 +23:25:17.7
20:19:01.26 +24:19:06.4
20:19:07.38 +24:06:48.0
20:14:44.74 +23:55:18.5
20:17:20.37 +23:03:05.1
20:22:42.21 +22:58:39.7
20:18:16.41 +23:46:31.2
20:18:28.25 +23:38:18.0
20:19:37.10 +23:58:36.5
20:12:34.42 +22:46:51.2
20:13:45.89 +22:53:30.7
20:23:12.86 +25:42:58.4
20:18:25.94 +22:59:55.6
20:13:37.19 +23:05:18.6
20:19:06.41 +24:03:24.2
20:19:48.97 +23:21:12.6
20:19:59.21 +23:31:59.0
20:18:42.83 +23:26:36.0
###################################################################################
20:27:25.00 +23:26:56.7 -- not an asteroid (will add it to exclusion list)
20:22:26.00 +23:52:46.0 -- not an asteroid (will add it to exclusion list)
20:28:42.22 +24:18:09.9 -- not an asteroid (will add it to exclusion list)
20:19:31.65 +23:09:14.8 -- not an asteroid (will add it to exclusion list)
20:15:28.35 +23:54:07.5 -- not an asteroid (will add it to exclusion list)
20:18:23.54 +23:31:23.8 -- not an asteroid (will add it to exclusion list)
20:19:56.50 +24:09:40.9 -- not an asteroid (will add it to exclusion list)
20:16:37.88 +23:06:36.9 -- not an asteroid (will add it to exclusion list)
20:15:15.95 +23:31:59.5 -- not an asteroid (will add it to exclusion list)
20:23:45.75 +23:18:06.7 -- not an asteroid (will add it to exclusion list)
20:27:50.30 +23:55:49.5 -- not an asteroid (will add it to exclusion list)
20:16:26.22 +24:21:00.1 -- not an asteroid (will add it to exclusion list)
20:13:26.81 +22:59:53.1 -- not an asteroid (will add it to exclusion list)
20:19:25.08 +23:28:38.5 -- not an asteroid (will add it to exclusion list)
20:32:06.83 +20:39:08.3 -- not an asteroid (will add it to exclusion list)
20:21:41.24 +23:04:49.3 -- not an asteroid (will add it to exclusion list)
20:30:19.38 +21:06:49.9 -- not an asteroid (will add it to exclusion list)
20:17:35.60 +22:59:09.7 -- not an asteroid (will add it to exclusion list)
20:20:45.40 +23:37:30.3 -- not an asteroid (will add it to exclusion list)
20:19:08.58 +23:06:10.5 -- not an asteroid (will add it to exclusion list)
20:26:30.94 +23:29:03.1 -- not an asteroid (will add it to exclusion list)
20:18:36.22 +23:25:39.9 -- not an asteroid (will add it to exclusion list)
20:23:34.94 +22:27:35.4 -- not an asteroid (will add it to exclusion list)
20:14:42.77 +23:36:31.4 -- not an asteroid (will add it to exclusion list)
20:24:07.18 +23:16:29.3 -- not an asteroid (will add it to exclusion list)
20:19:40.58 +23:06:45.1 -- not an asteroid (will add it to exclusion list)
20:20:13.86 +23:11:39.9 -- not an asteroid (will add it to exclusion list)
20:18:37.75 +23:28:46.6 -- not an asteroid (will add it to exclusion list)
20:24:40.42 +23:23:01.0 -- not an asteroid (will add it to exclusion list)
20:18:54.67 +23:11:49.1 -- not an asteroid (will add it to exclusion list)
20:19:07.28 +22:57:03.6 -- not an asteroid (will add it to exclusion list)
20:22:39.53 +22:24:00.1 -- not an asteroid (will add it to exclusion list)
20:17:50.89 +23:21:37.3 -- not an asteroid (will add it to exclusion list)
20:21:51.27 +22:31:05.7 -- not an asteroid (will add it to exclusion list)
20:27:03.70 +22:40:42.4 -- not an asteroid (will add it to exclusion list)
20:19:13.10 +23:48:41.8 -- not an asteroid (will add it to exclusion list)
20:18:45.82 +23:41:06.2 -- not an asteroid (will add it to exclusion list)
20:23:52.00 +22:11:29.8 -- not an asteroid (will add it to exclusion list)
20:18:41.39 +22:57:37.7 -- not an asteroid (will add it to exclusion list)
20:25:23.34 +23:12:25.1 -- not an asteroid (will add it to exclusion list)
20:19:15.78 +23:33:07.6 -- not an asteroid (will add it to exclusion list)
20:18:01.86 +22:56:24.8 -- not an asteroid (will add it to exclusion list)
20:19:58.50 +23:59:34.2 -- not an asteroid (will add it to exclusion list)
20:19:05.11 +24:23:29.0 -- not an asteroid (will add it to exclusion list)
20:19:32.91 +23:49:30.8 -- not an asteroid (will add it to exclusion list)
20:23:31.80 +24:12:35.5 -- not an asteroid (will add it to exclusion list)
20:18:39.74 +23:25:31.1 -- not an asteroid (will add it to exclusion list)
20:14:48.97 +24:10:43.3 -- not an asteroid (will add it to exclusion list)
20:18:55.93 +23:03:42.1 -- not an asteroid (will add it to exclusion list)
20:17:59.47 +23:33:41.6 -- not an asteroid (will add it to exclusion list)
20:20:25.79 +22:50:29.7 -- not an asteroid (will add it to exclusion list)
20:11:23.36 +22:41:21.9 -- not an asteroid (will add it to exclusion list)
20:14:31.75 +23:09:11.9 -- not an asteroid (will add it to exclusion list)
20:26:47.98 +21:11:16.6 -- not an asteroid (will add it to exclusion list)
20:15:40.67 +23:47:48.2 -- not an asteroid (will add it to exclusion list)
20:23:49.18 +24:45:14.6 -- not an asteroid (will add it to exclusion list)
20:15:26.19 +23:37:25.0 -- not an asteroid (will add it to exclusion list)
20:20:26.10 +24:16:27.2 -- not an asteroid (will add it to exclusion list)
20:18:36.33 +23:11:17.1 -- not an asteroid (will add it to exclusion list)
20:19:54.65 +23:42:39.3 -- not an asteroid (will add it to exclusion list)
20:19:07.33 +23:50:31.1 -- not an asteroid (will add it to exclusion list)
20:14:24.38 +23:07:33.9 -- not an asteroid (will add it to exclusion list)
20:14:18.66 +23:16:57.2 -- not an asteroid (will add it to exclusion list)
20:19:26.11 +24:07:44.6 -- not an asteroid (will add it to exclusion list)
20:22:12.40 +22:35:35.5 -- not an asteroid (will add it to exclusion list)
20:14:28.85 +23:20:02.8 -- not an asteroid (will add it to exclusion list)
20:17:45.56 +23:03:50.7 -- not an asteroid (will add it to exclusion list)
20:17:05.18 +24:10:42.5 -- not an asteroid (will add it to exclusion list)
20:21:00.10 +23:15:20.0 -- not an asteroid (will add it to exclusion list)
20:21:59.75 +22:43:25.2 -- not an asteroid (will add it to exclusion list)
20:27:47.52 +24:08:40.9 -- not an asteroid (will add it to exclusion list)
20:17:43.06 +24:59:39.7 -- not an asteroid (will add it to exclusion list)
20:13:46.81 +23:13:04.3 -- not an asteroid (will add it to exclusion list)
20:16:37.13 +24:06:43.1 -- not an asteroid (will add it to exclusion list)
20:23:12.59 +22:21:31.5 -- not an asteroid (will add it to exclusion list)
20:17:28.92 +22:57:52.5 -- not an asteroid (will add it to exclusion list)
20:19:02.45 +23:32:09.7 -- not an asteroid (will add it to exclusion list)
20:19:02.12 +23:01:14.4 -- not an asteroid (will add it to exclusion list)
20:23:04.80 +22:54:38.6 -- not an asteroid (will add it to exclusion list)
20:16:05.07 +24:17:55.9 -- not an asteroid (will add it to exclusion list)
20:12:57.05 +23:39:07.6 -- not an asteroid (will add it to exclusion list)
20:18:46.17 +23:28:12.9 -- not an asteroid (will add it to exclusion list)
20:12:57.35 +23:18:54.0 -- not an asteroid (will add it to exclusion list)
20:19:20.82 +23:47:36.0 -- not an asteroid (will add it to exclusion list)
20:14:40.28 +23:44:03.1 -- not an asteroid (will add it to exclusion list)
20:23:40.99 +23:27:45.3 -- not an asteroid (will add it to exclusion list)
20:22:46.53 +23:06:20.7 -- not an asteroid (will add it to exclusion list)
20:21:04.73 +23:59:58.4 -- not an asteroid (will add it to exclusion list)
20:18:10.49 +23:09:22.8 -- not an asteroid (will add it to exclusion list)
20:14:02.44 +23:12:03.1 -- not an asteroid (will add it to exclusion list)
20:14:50.01 +22:26:23.0 -- not an asteroid (will add it to exclusion list)
20:19:37.76 +23:06:32.2 -- not an asteroid (will add it to exclusion list)
20:13:56.23 +23:29:05.4 -- not an asteroid (will add it to exclusion list)
20:19:37.91 +23:05:43.5 -- not an asteroid (will add it to exclusion list)
20:18:28.04 +23:11:01.8 -- not an asteroid (will add it to exclusion list)
20:18:16.35 +23:25:22.4 -- not an asteroid (will add it to exclusion list)
20:18:13.34 +24:34:56.0 -- not an asteroid (will add it to exclusion list)
20:23:04.63 +23:05:54.5 -- not an asteroid (will add it to exclusion list)
20:16:34.82 +23:55:41.4 -- not an asteroid (will add it to exclusion list)
20:18:40.19 +22:59:37.7 -- not an asteroid (will add it to exclusion list)
20:15:49.06 +23:46:14.4 -- not an asteroid (will add it to exclusion list)
20:16:46.15 +23:39:25.9 -- not an asteroid (will add it to exclusion list)
20:08:52.27 +22:36:04.1 -- not an asteroid (will add it to exclusion list)
20:23:46.41 +24:07:33.9 -- not an asteroid (will add it to exclusion list)
20:20:02.81 +23:11:46.8 -- not an asteroid (will add it to exclusion list)
20:14:26.27 +23:55:18.5 -- not an asteroid (will add it to exclusion list)
20:21:39.38 +23:14:06.8 -- not an asteroid (will add it to exclusion list)
20:25:28.11 +21:50:31.3 -- not an asteroid (will add it to exclusion list)
20:15:47.40 +24:03:53.9 -- not an asteroid (will add it to exclusion list)
20:15:46.06 +22:57:45.7 -- not an asteroid (will add it to exclusion list)
20:15:44.83 +24:28:19.7 -- not an asteroid (will add it to exclusion list)
20:17:43.69 +23:06:52.6 -- not an asteroid (will add it to exclusion list)
20:21:03.59 +24:08:50.5 -- not an asteroid (will add it to exclusion list)
20:20:11.91 +23:50:00.5 -- not an asteroid (will add it to exclusion list)
20:18:57.60 +23:16:23.1 -- not an asteroid (will add it to exclusion list)
20:18:35.60 +22:54:41.2 -- not an asteroid (will add it to exclusion list)
20:17:20.32 +24:20:12.9 -- not an asteroid (will add it to exclusion list)
20:23:45.85 +23:27:44.0 -- not an asteroid (will add it to exclusion list)
20:20:05.96 +23:59:41.3 -- not an asteroid (will add it to exclusion list)
20:28:25.05 +24:13:43.6 -- not an asteroid (will add it to exclusion list)
20:18:41.36 +23:32:44.5 -- not an asteroid (will add it to exclusion list)
20:22:52.68 +22:37:20.1 -- not an asteroid (will add it to exclusion list)
20:18:38.31 +23:00:33.2 -- not an asteroid (will add it to exclusion list)
20:18:16.35 +24:59:08.1 -- not an asteroid (will add it to exclusion list)
20:09:36.24 +22:21:24.4 -- not an asteroid (will add it to exclusion list)
20:19:07.60 +24:19:07.1 -- not an asteroid (will add it to exclusion list)
20:19:44.53 +24:10:49.4 -- not an asteroid (will add it to exclusion list)
20:29:27.06 +19:53:19.8 -- not an asteroid (will add it to exclusion list)
20:15:21.93 +23:54:04.4 -- not an asteroid (will add it to exclusion list)
20:19:36.32 +23:16:27.0 -- not an asteroid (will add it to exclusion list)
20:16:22.76 +23:43:05.7 -- not an asteroid (will add it to exclusion list)
20:34:17.99 +24:48:14.1 -- not an asteroid (will add it to exclusion list)
20:26:41.34 +23:10:53.0 -- not an asteroid (will add it to exclusion list)
20:16:27.05 +23:04:10.8 -- not an asteroid (will add it to exclusion list)
20:13:33.45 +23:07:15.5 -- not an asteroid (will add it to exclusion list)
20:12:46.59 +23:13:21.8 -- not an asteroid (will add it to exclusion list)
20:23:26.74 +22:38:49.1 -- not an asteroid (will add it to exclusion list)
20:19:40.21 +23:46:58.6 -- not an asteroid (will add it to exclusion list)
20:16:47.43 +23:45:57.0 -- not an asteroid (will add it to exclusion list)
20:23:46.74 +23:09:26.9 -- not an asteroid (will add it to exclusion list)
20:11:33.09 +22:40:44.6 -- not an asteroid (will add it to exclusion list)
20:20:06.83 +23:36:13.4 -- not an asteroid (will add it to exclusion list)
20:22:33.21 +23:34:59.6 -- not an asteroid (will add it to exclusion list)
20:22:20.55 +23:36:06.2 -- not an asteroid (will add it to exclusion list)
20:15:24.28 +23:54:20.4 -- not an asteroid (will add it to exclusion list)
20:01:57.99 +22:35:02.4 -- not an asteroid (will add it to exclusion list)
20:22:40.14 +23:23:18.4 -- not an asteroid (will add it to exclusion list)
20:23:27.27 +23:51:53.5 -- not an asteroid (will add it to exclusion list)
20:19:02.21 +23:34:22.9 -- not an asteroid (will add it to exclusion list)
20:18:55.22 +23:17:20.0 -- not an asteroid (will add it to exclusion list)
20:14:54.22 +23:33:39.7 -- not an asteroid (will add it to exclusion list)
20:19:01.66 +23:09:16.4 -- not an asteroid (will add it to exclusion list)
20:25:53.68 +23:04:27.0 -- not an asteroid (will add it to exclusion list)
20:21:15.58 +23:27:47.1 -- not an asteroid (will add it to exclusion list)
20:15:52.02 +23:30:59.8 -- not an asteroid (will add it to exclusion list)
20:15:58.86 +23:45:04.1 -- not an asteroid (will add it to exclusion list)
20:16:46.50 +23:38:50.4 -- not an asteroid (will add it to exclusion list)
20:17:00.98 +24:20:22.6 -- not an asteroid (will add it to exclusion list)
20:17:06.51 +22:45:43.9 -- not an asteroid (will add it to exclusion list)
20:15:23.82 +23:25:17.7 -- not an asteroid (will add it to exclusion list)
20:19:01.26 +24:19:06.4 -- not an asteroid (will add it to exclusion list)
20:19:07.38 +24:06:48.0 -- not an asteroid (will add it to exclusion list)
20:14:44.74 +23:55:18.5 -- not an asteroid (will add it to exclusion list)
20:17:20.37 +23:03:05.1 -- not an asteroid (will add it to exclusion list)
20:22:42.21 +22:58:39.7 -- not an asteroid (will add it to exclusion list)
20:18:16.41 +23:46:31.2 -- not an asteroid (will add it to exclusion list)
20:18:28.25 +23:38:18.0 -- not an asteroid (will add it to exclusion list)
20:19:37.10 +23:58:36.5 -- not an asteroid (will add it to exclusion list)
20:12:34.42 +22:46:51.2 -- not an asteroid (will add it to exclusion list)
20:13:45.89 +22:53:30.7 -- not an asteroid (will add it to exclusion list)
20:23:12.86 +25:42:58.4 -- not an asteroid (will add it to exclusion list)
20:18:25.94 +22:59:55.6 -- not an asteroid (will add it to exclusion list)
20:13:37.19 +23:05:18.6 -- not an asteroid (will add it to exclusion list)
20:19:06.41 +24:03:24.2 -- not an asteroid (will add it to exclusion list)
20:19:48.97 +23:21:12.6 -- not an asteroid (will add it to exclusion list)
20:19:59.21 +23:31:59.0 -- not an asteroid (will add it to exclusion list)
20:18:42.83 +23:26:36.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
20:01:57.99 +22:35:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:52.27 +22:36:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:09:36.24 +22:21:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:23.36 +22:41:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:33.09 +22:40:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:34.42 +22:46:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:46.59 +23:13:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:57.05 +23:39:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:57.35 +23:18:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:26.81 +22:59:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:33.45 +23:07:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:37.19 +23:05:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:45.89 +22:53:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:46.81 +23:13:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:56.23 +23:29:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:02.44 +23:12:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:18.66 +23:16:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:24.38 +23:07:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:26.27 +23:55:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:28.85 +23:20:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:31.75 +23:09:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:40.28 +23:44:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:42.77 +23:36:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:44.74 +23:55:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:48.97 +24:10:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:50.01 +22:26:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:54.22 +23:33:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:15.95 +23:31:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:21.93 +23:54:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:23.82 +23:25:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:24.28 +23:54:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:26.19 +23:37:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:28.35 +23:54:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:40.67 +23:47:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:44.83 +24:28:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:46.06 +22:57:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:47.40 +24:03:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:49.06 +23:46:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:52.02 +23:30:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:58.86 +23:45:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:05.07 +24:17:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:22.76 +23:43:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:26.22 +24:21:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:27.05 +23:04:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:34.82 +23:55:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:37.13 +24:06:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:37.88 +23:06:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:46.15 +23:39:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:46.50 +23:38:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:47.43 +23:45:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:00.98 +24:20:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:05.18 +24:10:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:06.51 +22:45:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:20.32 +24:20:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:20.37 +23:03:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:28.92 +22:57:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:35.60 +22:59:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:43.06 +24:59:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:43.69 +23:06:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:45.56 +23:03:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:50.89 +23:21:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:59.47 +23:33:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:01.86 +22:56:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:10.49 +23:09:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:13.34 +24:34:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:16.35 +23:25:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:16.35 +24:59:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:16.41 +23:46:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:23.54 +23:31:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:25.94 +22:59:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:28.04 +23:11:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:28.25 +23:38:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:35.60 +22:54:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:36.22 +23:25:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:36.33 +23:11:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:37.75 +23:28:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:38.31 +23:00:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:39.74 +23:25:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:40.19 +22:59:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:41.36 +23:32:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:41.39 +22:57:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:42.83 +23:26:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:45.82 +23:41:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:46.17 +23:28:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:54.67 +23:11:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:55.22 +23:17:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:55.93 +23:03:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:18:57.60 +23:16:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:01.26 +24:19:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:01.66 +23:09:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:02.12 +23:01:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:02.21 +23:34:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:02.45 +23:32:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:05.11 +24:23:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:06.41 +24:03:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:07.28 +22:57:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:07.33 +23:50:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:07.38 +24:06:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:07.60 +24:19:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:08.58 +23:06:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:13.10 +23:48:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:15.78 +23:33:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:20.82 +23:47:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:25.08 +23:28:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:26.11 +24:07:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:31.65 +23:09:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:32.91 +23:49:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:36.32 +23:16:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:37.10 +23:58:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:37.76 +23:06:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:37.91 +23:05:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:40.21 +23:46:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:40.58 +23:06:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:44.53 +24:10:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:48.97 +23:21:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:54.65 +23:42:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:56.50 +24:09:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:58.50 +23:59:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:59.21 +23:31:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:02.81 +23:11:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:05.96 +23:59:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:06.83 +23:36:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:11.91 +23:50:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:13.86 +23:11:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:25.79 +22:50:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:26.10 +24:16:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:20:45.40 +23:37:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:00.10 +23:15:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:03.59 +24:08:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:04.73 +23:59:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:15.58 +23:27:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:39.38 +23:14:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:41.24 +23:04:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:51.27 +22:31:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:59.75 +22:43:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:12.40 +22:35:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:20.55 +23:36:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:26.00 +23:52:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:33.21 +23:34:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:39.53 +22:24:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:40.14 +23:23:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:42.21 +22:58:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:46.53 +23:06:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:22:52.68 +22:37:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:04.63 +23:05:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:04.80 +22:54:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:12.59 +22:21:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:12.86 +25:42:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:26.74 +22:38:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:27.27 +23:51:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:31.80 +24:12:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:34.94 +22:27:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:40.99 +23:27:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:45.75 +23:18:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:45.85 +23:27:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:46.41 +24:07:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:46.74 +23:09:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:49.18 +24:45:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:23:52.00 +22:11:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:07.18 +23:16:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:40.42 +23:23:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:23.34 +23:12:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:28.11 +21:50:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:25:53.68 +23:04:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:30.94 +23:29:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:41.34 +23:10:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:47.98 +21:11:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:03.70 +22:40:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:25.00 +23:26:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:47.52 +24:08:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:50.30 +23:55:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:28:25.05 +24:13:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:28:42.22 +24:18:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:27.06 +19:53:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:19.38 +21:06:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:32:06.83 +20:39:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:34:17.99 +24:48:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
20:01:57.99 +22:35:02.4 -- a known variable star
20:08:52.27 +22:36:04.1 -- a known variable star
20:09:36.24 +22:21:24.4 -- a known variable star
20:11:23.36 +22:41:21.9 -- not a known variable star
20:11:33.09 +22:40:44.6 -- a known variable star
20:12:34.42 +22:46:51.2 -- not a known variable star
20:12:46.59 +23:13:21.8 -- not a known variable star
20:12:57.05 +23:39:07.6 -- not a known variable star
20:12:57.35 +23:18:54.0 -- not a known variable star
20:13:26.81 +22:59:53.1 -- not a known variable star
20:13:33.45 +23:07:15.5 -- not a known variable star
20:13:37.19 +23:05:18.6 -- a known variable star
20:13:45.89 +22:53:30.7 -- not a known variable star
20:13:46.81 +23:13:04.3 -- not a known variable star
20:13:56.23 +23:29:05.4 -- not a known variable star
20:14:02.44 +23:12:03.1 -- not a known variable star
20:14:18.66 +23:16:57.2 -- not a known variable star
20:14:24.38 +23:07:33.9 -- not a known variable star
20:14:26.27 +23:55:18.5 -- not a known variable star
20:14:28.85 +23:20:02.8 -- not a known variable star
20:14:31.75 +23:09:11.9 -- a known variable star
20:14:40.28 +23:44:03.1 -- a known variable star
20:14:42.77 +23:36:31.4 -- not a known variable star
20:14:44.74 +23:55:18.5 -- not a known variable star
20:14:48.97 +24:10:43.3 -- not a known variable star
20:14:50.01 +22:26:23.0 -- not a known variable star
20:14:54.22 +23:33:39.7 -- not a known variable star
20:15:15.95 +23:31:59.5 -- not a known variable star
20:15:21.93 +23:54:04.4 -- not a known variable star
20:15:23.82 +23:25:17.7 -- not a known variable star
20:15:24.28 +23:54:20.4 -- not a known variable star
20:15:26.19 +23:37:25.0 -- not a known variable star
20:15:28.35 +23:54:07.5 -- not a known variable star
20:15:40.67 +23:47:48.2 -- a known variable star
20:15:44.83 +24:28:19.7 -- not a known variable star
20:15:46.06 +22:57:45.7 -- not a known variable star
20:15:47.40 +24:03:53.9 -- not a known variable star
20:15:49.06 +23:46:14.4 -- not a known variable star
20:15:52.02 +23:30:59.8 -- a known variable star
20:15:58.86 +23:45:04.1 -- not a known variable star
20:16:05.07 +24:17:55.9 -- not a known variable star
20:16:22.76 +23:43:05.7 -- not a known variable star
20:16:26.22 +24:21:00.1 -- not a known variable star
20:16:27.05 +23:04:10.8 -- a known variable star
20:16:34.82 +23:55:41.4 -- not a known variable star
20:16:37.13 +24:06:43.1 -- a known variable star
20:16:37.88 +23:06:36.9 -- a known variable star
20:16:46.15 +23:39:25.9 -- not a known variable star
20:16:46.50 +23:38:50.4 -- a known variable star
20:16:47.43 +23:45:57.0 -- not a known variable star
20:17:00.98 +24:20:22.6 -- not a known variable star
20:17:05.18 +24:10:42.5 -- not a known variable star
20:17:06.51 +22:45:43.9 -- a known variable star
20:17:20.32 +24:20:12.9 -- not a known variable star
20:17:20.37 +23:03:05.1 -- not a known variable star
20:17:28.92 +22:57:52.5 -- a known variable star
20:17:35.60 +22:59:09.7 -- not a known variable star
20:17:43.06 +24:59:39.7 -- a known variable star
20:17:43.69 +23:06:52.6 -- not a known variable star
20:17:45.56 +23:03:50.7 -- not a known variable star
20:17:50.89 +23:21:37.3 -- not a known variable star
20:17:59.47 +23:33:41.6 -- not a known variable star
20:18:01.86 +22:56:24.8 -- not a known variable star
20:18:10.49 +23:09:22.8 -- a known variable star
20:18:13.34 +24:34:56.0 -- a known variable star
20:18:16.35 +23:25:22.4 -- not a known variable star
20:18:16.35 +24:59:08.1 -- not a known variable star
20:18:16.41 +23:46:31.2 -- not a known variable star
20:18:23.54 +23:31:23.8 -- not a known variable star
20:18:25.94 +22:59:55.6 -- not a known variable star
20:18:28.04 +23:11:01.8 -- not a known variable star
20:18:28.25 +23:38:18.0 -- a known variable star
20:18:35.60 +22:54:41.2 -- not a known variable star
20:18:36.22 +23:25:39.9 -- a known variable star
20:18:36.33 +23:11:17.1 -- a known variable star
20:18:37.75 +23:28:46.6 -- not a known variable star
20:18:38.31 +23:00:33.2 -- not a known variable star
20:18:39.74 +23:25:31.1 -- not a known variable star
20:18:40.19 +22:59:37.7 -- not a known variable star
20:18:41.36 +23:32:44.5 -- not a known variable star
20:18:41.39 +22:57:37.7 -- not a known variable star
20:18:42.83 +23:26:36.0 -- a known variable star
20:18:45.82 +23:41:06.2 -- not a known variable star
20:18:46.17 +23:28:12.9 -- not a known variable star
20:18:54.67 +23:11:49.1 -- not a known variable star
20:18:55.22 +23:17:20.0 -- not a known variable star
20:18:55.93 +23:03:42.1 -- not a known variable star
20:18:57.60 +23:16:23.1 -- not a known variable star
20:19:01.26 +24:19:06.4 -- a known variable star
20:19:01.66 +23:09:16.4 -- not a known variable star
20:19:02.12 +23:01:14.4 -- not a known variable star
20:19:02.21 +23:34:22.9 -- not a known variable star
20:19:02.45 +23:32:09.7 -- not a known variable star
20:19:05.11 +24:23:29.0 -- not a known variable star
20:19:06.41 +24:03:24.2 -- not a known variable star
20:19:07.28 +22:57:03.6 -- not a known variable star
20:19:07.33 +23:50:31.1 -- not a known variable star
20:19:07.38 +24:06:48.0 -- not a known variable star
20:19:07.60 +24:19:07.1 -- not a known variable star
20:19:08.58 +23:06:10.5 -- not a known variable star
20:19:13.10 +23:48:41.8 -- not a known variable star
20:19:15.78 +23:33:07.6 -- not a known variable star
20:19:20.82 +23:47:36.0 -- not a known variable star
20:19:25.08 +23:28:38.5 -- not a known variable star
20:19:26.11 +24:07:44.6 -- not a known variable star
20:19:31.65 +23:09:14.8 -- not a known variable star
20:19:32.91 +23:49:30.8 -- not a known variable star
20:19:36.32 +23:16:27.0 -- a known variable star
20:19:37.10 +23:58:36.5 -- not a known variable star
20:19:37.76 +23:06:32.2 -- a known variable star
20:19:37.91 +23:05:43.5 -- a known variable star
20:19:40.21 +23:46:58.6 -- not a known variable star
20:19:40.58 +23:06:45.1 -- not a known variable star
20:19:44.53 +24:10:49.4 -- not a known variable star
20:19:48.97 +23:21:12.6 -- not a known variable star
20:19:54.65 +23:42:39.3 -- not a known variable star
20:19:56.50 +24:09:40.9 -- not a known variable star
20:19:58.50 +23:59:34.2 -- not a known variable star
20:19:59.21 +23:31:59.0 -- a known variable star
20:20:02.81 +23:11:46.8 -- not a known variable star
20:20:05.96 +23:59:41.3 -- not a known variable star
20:20:06.83 +23:36:13.4 -- not a known variable star
20:20:11.91 +23:50:00.5 -- not a known variable star
20:20:13.86 +23:11:39.9 -- not a known variable star
20:20:25.79 +22:50:29.7 -- not a known variable star
20:20:26.10 +24:16:27.2 -- not a known variable star
20:20:45.40 +23:37:30.3 -- a known variable star
20:21:00.10 +23:15:20.0 -- a known variable star
20:21:03.59 +24:08:50.5 -- not a known variable star
20:21:04.73 +23:59:58.4 -- a known variable star
20:21:15.58 +23:27:47.1 -- not a known variable star
20:21:39.38 +23:14:06.8 -- not a known variable star
20:21:41.24 +23:04:49.3 -- not a known variable star
20:21:51.27 +22:31:05.7 -- not a known variable star
20:21:59.75 +22:43:25.2 -- a known variable star
20:22:12.40 +22:35:35.5 -- not a known variable star
20:22:20.55 +23:36:06.2 -- not a known variable star
20:22:26.00 +23:52:46.0 -- a known variable star
20:22:33.21 +23:34:59.6 -- not a known variable star
20:22:39.53 +22:24:00.1 -- not a known variable star
20:22:40.14 +23:23:18.4 -- not a known variable star
20:22:42.21 +22:58:39.7 -- not a known variable star
20:22:46.53 +23:06:20.7 -- not a known variable star
20:22:52.68 +22:37:20.1 -- a known variable star
20:23:04.63 +23:05:54.5 -- not a known variable star
20:23:04.80 +22:54:38.6 -- a known variable star
20:23:12.59 +22:21:31.5 -- a known variable star
20:23:12.86 +25:42:58.4 -- a known variable star
20:23:26.74 +22:38:49.1 -- a known variable star
20:23:27.27 +23:51:53.5 -- not a known variable star
20:23:31.80 +24:12:35.5 -- not a known variable star
20:23:34.94 +22:27:35.4 -- a known variable star
20:23:40.99 +23:27:45.3 -- a known variable star
20:23:45.75 +23:18:06.7 -- not a known variable star
20:23:45.85 +23:27:44.0 -- not a known variable star
20:23:46.41 +24:07:33.9 -- a known variable star
20:23:46.74 +23:09:26.9 -- a known variable star
20:23:49.18 +24:45:14.6 -- a known variable star
20:23:52.00 +22:11:29.8 -- not a known variable star
20:24:07.18 +23:16:29.3 -- not a known variable star
20:24:40.42 +23:23:01.0 -- not a known variable star
20:25:23.34 +23:12:25.1 -- a known variable star
20:25:28.11 +21:50:31.3 -- not a known variable star
20:25:53.68 +23:04:27.0 -- not a known variable star
20:26:30.94 +23:29:03.1 -- a known variable star
20:26:41.34 +23:10:53.0 -- a known variable star
20:26:47.98 +21:11:16.6 -- not a known variable star
20:27:03.70 +22:40:42.4 -- a known variable star
20:27:25.00 +23:26:56.7 -- not a known variable star
20:27:47.52 +24:08:40.9 -- not a known variable star
20:27:50.30 +23:55:49.5 -- a known variable star
20:28:25.05 +24:13:43.6 -- not a known variable star
20:28:42.22 +24:18:09.9 -- not a known variable star
20:29:27.06 +19:53:19.8 -- a known variable star
20:30:19.38 +21:06:49.9 -- a known variable star
20:32:06.83 +20:39:08.3 -- a known variable star
20:34:17.99 +24:48:14.1 -- a known variable star
Found 126 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
177 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 177 (excluding asteroids and hot pixels, 126 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)2461205.68099237 -observatory V36
07:15:13.33 +23:35:14.1 Mercury (0.5mag)
08:12:36.12 +22:01:54.4 Venus (-4.0mag)
03:07:03.32 +17:00:56.9 Mars (1.3mag)
07:53:29.27 +21:18:28.8 Jupiter (-1.8mag)
00:50:59.69 +02:57:23.5 Saturn (0.8mag)
04:01:37.03 +20:29:29.7 Uranus (5.8mag)
00:16:27.60 +00:18:32.0 Neptune (7.8mag)
20:32:59.91 -23:06:51.4 Pluto (14.5mag)
04:25:30.94 +25:56:12.5 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Jun 13 23:28 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461205.68099237:
07:53:35.00 +21:18:10.0 Io (6.0mag)
07:53:21.03 +21:18:54.4 Europa (6.2mag)
07:53:23.44 +21:18:42.7 Ganymede (5.6mag)
07:53:00.92 +21:19:56.3 Callisto (6.8mag)
07:53:25.14 +20:55:23.1 Himalia (15.6mag)
07:53:32.81 +21:18:17.9 Thebe (16.5mag)
07:53:14.62 +21:08:15.5 Elara (17.6mag)
07:55:58.00 +21:26:54.3 Pasiphae (17.7mag)
07:59:48.17 +21:20:39.7 Carme (18.9mag)
00:51:11.38 +02:57:11.7 Titan (8.6mag)
00:50:58.93 +02:57:15.9 Rhea (9.9mag)
00:51:25.76 +02:59:55.3 Iapetus (11.3mag)
00:51:14.26 +02:57:05.5 Hyperion (14.6mag)
00:51:34.54 +02:58:28.0 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 13 23:28 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461205.68099237:
17:28:12.45 -35:35:16.6 JWST
17:16:17.02 +43:31:48.3 Chandra
18:47:53.67 -17:45:33.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 13 23:28 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461205.68099237 -observatory V36
18:39:10.52 -33:04:29.3 13.6mag P/2010 H2 (Vales)
05:59:23.83 -68:00:54.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:51:16.35 +32:02:52.8 17.5mag C/2017 K2 (PANSTARRS)
17:12:20.38 +15:37:12.5 17.8mag C/2021 G2 (ATLAS)
22:10:28.54 -44:56:08.2 16.4mag P/2021 N1 (ZTF)
23:11:06.80 +31:48:25.7 17.2mag C/2022 E2 (ATLAS)
05:41:21.76 +27:00:08.7 16.5mag C/2022 N2 (PANSTARRS)
09:34:08.18 +30:51:59.0 16.7mag C/2022 QE78 (ATLAS)
08:53:49.95 +04:12:07.6 17.7mag C/2022 R6 (PANSTARRS)
18:24:16.90 +21:41:08.4 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:17:19.72 -11:01:41.0 17.6mag P/2023 B1 (PANSTARRS)
22:11:57.52 +66:52:31.0 17.8mag C/2023 H5 (Lemmon)
17:31:29.82 -07:17:24.5 13.7mag C/2023 R1 (PANSTARRS)
13:16:35.54 +81:36:31.3 18.0mag C/2023 X2 (Lemmon)
07:18:55.49 +64:31:15.5 17.7mag C/2024 A1 (ATLAS)
06:56:15.11 +28:20:29.7 13.8mag C/2024 E1 (Wierzchos)
15:32:42.26 +14:00:53.6 17.4mag C/2024 G6 (ATLAS)
20:08:42.81 +32:53:24.3 13.9mag C/2024 J3 (ATLAS)
04:24:01.44 -15:26:51.9 16.0mag C/2024 T5 (ATLAS)
06:11:28.21 +33:27:31.9 17.9mag C/2025 J1 (Borisov)
11:32:47.02 +52:23:31.9 17.6mag C/2025 L1 (ATLAS)
06:51:47.08 -11:09:01.6 14.7mag C/2025 R3 (PANSTARRS)
09:29:15.70 +23:14:40.8 17.9mag C/2025 V2 (Rankin)
12:39:44.79 +04:38:54.1 17.2mag C/2025 Y1 (ATLAS)
18:02:09.41 +76:20:34.6 17.8mag C/2026 A2 (Bok)
02:10:45.16 +43:49:29.4 16.2mag C/2026 B2 (Sun-Gao)
11:12:50.33 -01:44:28.2 16.6mag A/2026 E1
20:34:27.62 -09:06:45.4 8.4mag 10P/Tempel
11:03:33.00 -01:04:09.2 16.0mag 29P/Schwassmann-Wachmann
03:20:57.71 +26:26:02.4 17.7mag 47P/Ashbrook-Jackson
09:12:44.91 +22:02:16.5 16.9mag 63P/Wild
00:31:53.32 -06:00:24.3 15.6mag 65P/Gunn
07:02:53.46 +33:56:48.7 17.1mag 76P/West-Kohoutek-Ikemura
03:23:41.34 +17:56:44.0 13.8mag 78P/Gehrels
01:33:30.28 +06:06:41.4 15.7mag 88P/Howell
05:13:53.97 +30:40:38.5 15.3mag 93P/Lovas
03:00:08.45 +28:32:25.5 17.5mag 114P/Wiseman-Skiff
07:04:54.03 +32:46:58.0 15.5mag 123P/West-Hartley
10:00:39.88 +12:05:00.4 16.6mag 124P/Mrkos
04:08:55.10 +19:37:54.4 16.3mag 128P/Shoemaker-Holt
04:45:26.92 +19:19:50.6 17.8mag 131P/Mueller
06:23:16.45 +17:53:32.7 15.4mag 141P/Machholz
06:26:17.45 +17:52:47.9 15.4mag 141P-A/Machholz
05:23:42.63 +16:51:40.9 12.2mag 141P-D/Machholz
03:01:49.38 -23:53:51.6 16.6mag 161P/Hartley-IRAS
04:01:26.82 +26:07:40.7 15.0mag 162P/SidingSpring
19:35:28.74 +03:35:01.8 16.5mag 169P/NEAT
00:34:22.33 +03:36:28.5 17.8mag 220P/McNaught
16:47:46.33 -08:14:06.0 16.5mag 235P/LINEAR
07:48:08.67 +35:12:39.8 17.6mag 240P/NEAT
00:48:08.08 +00:06:48.0 16.2mag 260P/McNaught
04:20:42.15 +33:31:32.5 17.5mag 295P/LINEAR
00:26:44.10 -02:38:48.7 17.7mag 320P/McNaught
15:12:42.63 +07:51:34.0 17.5mag 391P/Kowalski
08:11:58.80 +20:35:04.3 17.9mag 450P/LONEOS
07:09:43.98 +41:15:51.9 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 13 23:28 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 23:28 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 23:28 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
15:25:24.694 +28:06:12.15 AT 2026oke 2026-06-06.78 19.63
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
-rw-r--r-- 1 apache apache 30K Jun 13 23:28 tns_transients_list.txt
