GP044

A Misaligned Relativistic Jet in SN 2007gr?

Abstract

The most powerful supernovae Ib/c are believed to be connected to long duration gamma-ray burst events. Although there were clear associations between three gamma bursts and type Ib/c supernovae, not all long duration gamma bursts were related to supernovae, and not all type Ib/c supernovae have an associated GRB. It has been proposed that some of the orphan type Ib/c supernovae produce relativistic GRB jets, that are not oriented within our line of sight, explaining the lack of an observable gamma-ray burst. So far this idea has never been confirmed. We propose follow-up EVN+GBT observations of the recent SN 2007gr, which was successfully detected in an e-VLBI experiment on 6-7 September 2007. The distance of the source is only 7.3 Mpc, the closest ever radio-detected type Ib/c supernova, which makes it an ideal case to study the supernova-GRB connection.

Investigators
Name Other * Institution Email Phone
Zolt Paragi PI FOMI Satellite Geodetic Observ zparagi@jive.nl 3627310980
Chryssa Kouveliotou MSFC/NASA chryssa.kouveliotou@nasa.gov 256-544-7711
Mike Garrett JIVE garrett@astron.nl 31-521-596511
Enrico Ramirez-Ruiz IAS, Princeton enrico@ucolick.org
Huib van Langevelde Joint Institute for VLBI in Eu langevelde@jive.nl 31-521-596515
Arpad Szomoru Joint Institute for VLBI in Eu szomoru@jive.nl +31 (0)521 596 513
Megan Argo Manchester mkargo@jb.man.ac.uk
* PI = Principal Investigator; CO = Contact author; T = Thesis observations; S = Student

Front Ends
Gregorian C(3.95 to 5.85 GHz)

Back Ends
Mark 5 recorder (disks)

Type of Observing
Monitor Very Long Baseline Interferometry

Switching Type

Processor (correlator)
JIVE

Allotted time 14.00 hours

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Updated 10/11/2007