AMI-LA 15.5 GHz Observations of the Nearby Supernova SN2020oi

Itai Sfaradi; David Williams; Assaf Horesh; Rob Fender; Dave Green; David Titterington; Yvette Perrott

AMI-LA 15.5 GHz Observations of the Nearby Supernova SN2020oi

Itai Sfaradi, David Williams, Assaf Horesh, Rob Fender, Dave Green, David Titterington, Yvette Perrott

Astronomy and Astrophysics Theory Group

Research output: Other contribution

Abstract

Here we report our AMI-LA observation of the Nearby supernova SN2020oi. We detect a ~10 mJy source at 15.5 GHz. We conclude that the detected emission is comprised of contribution of SN2020oi emission and emission from the two nearby radio sources that previously detected in the FIRST survey....

Original language	English
Publication status	Published - Jan 2020

Keywords

Supernova
Radio
ZTF20aaelulu
2020oi
SN2020oi

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title = "AMI-LA 15.5 GHz Observations of the Nearby Supernova SN2020oi",

abstract = "Here we report our AMI-LA observation of the Nearby supernova SN2020oi. We detect a ~10 mJy source at 15.5 GHz. We conclude that the detected emission is comprised of contribution of SN2020oi emission and emission from the two nearby radio sources that previously detected in the FIRST survey....",

keywords = "Supernova, Radio, ZTF20aaelulu, 2020oi, SN2020oi",

author = "Itai Sfaradi and David Williams and Assaf Horesh and Rob Fender and Dave Green and David Titterington and Yvette Perrott",

year = "2020",

month = jan,

language = "English",

type = "Other",

}

TY - GEN

T1 - AMI-LA 15.5 GHz Observations of the Nearby Supernova SN2020oi

AU - Sfaradi, Itai

AU - Williams, David

AU - Horesh, Assaf

AU - Fender, Rob

AU - Green, Dave

AU - Titterington, David

AU - Perrott, Yvette

PY - 2020/1

Y1 - 2020/1

N2 - Here we report our AMI-LA observation of the Nearby supernova SN2020oi. We detect a ~10 mJy source at 15.5 GHz. We conclude that the detected emission is comprised of contribution of SN2020oi emission and emission from the two nearby radio sources that previously detected in the FIRST survey....

AB - Here we report our AMI-LA observation of the Nearby supernova SN2020oi. We detect a ~10 mJy source at 15.5 GHz. We conclude that the detected emission is comprised of contribution of SN2020oi emission and emission from the two nearby radio sources that previously detected in the FIRST survey....

KW - Supernova

KW - Radio

KW - ZTF20aaelulu

KW - 2020oi

KW - SN2020oi

M3 - Other contribution

ER -

AMI-LA 15.5 GHz Observations of the Nearby Supernova SN2020oi

Abstract

Keywords

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