BG162

Measuring the Proper Motion and Expansion Velocity of SN2001em

Abstract

SN2001em has a bright, rising optically thin radio emission and an extremely large X-ray luminosity, ~ 2-3 yr after the supernova. These characteristics are hard to reconcile with typical SNR expansion velocities, but arise naturally for a relativistic jet pointing away from us. Thus, SN2001em is the best known candidate for a core collapse supernova that harbors a relativistic jet, making it unique and of great interest for both supernovae and gamma-ray bursts. Its apparent size in the radio has been recently constrained to be < 0.23ct. However, the head of the jet, which is likely to be the brightest, might appear smaller than the distance that it has traveled. Thus, the key observation for confirming or ruling out relativistic motion, which we propose to do, is measuring the proper motion. Such an observation would provide crucial information about this fascinating source, and probably resolve the controversy.

Investigators
Name Other * Institution Email Phone
Jonathon Granot PI KIPAC/Stanford granot@slac.stanford.edu
Enrico Ramirez-Ruiz IAS, Princeton enrico@ias.edu
Greg Taylor Univ. of New Mexico gbtaylor@unm.edu 505 277-5238
Chris Stockdale Marquette U christopher.stockdale@mu.edu
Schuyler Van Dyk Caltech vandyk@ipac.caltech.edu 626 397-7044,626 397-7021
Kurt Weiler Naval Research Lab Kurt.Weiler@nrl.navy.mil
Dick Sramek NRAO-SOC rsramek@nrao.edu
N. Panagia Space Telescope Science Instit panagia@stsci.edu 410 338 4916
M. Kelley S Marquette U matthew.kelley@mu.edu
* PI = Principal Investigator; CO = Contact author; T = Thesis observations; S = Student

Front Ends
Gregorian X(8.2 to 10.0 GHz)

Back Ends
VLBA recorder and DAR

Type of Observing
Very Long Baseline Interferometry

Switching Type

Processor (correlator)
Socorro

Allotted time 10.00 hours

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Updated 09/19/2007