330.03 Properties of Radio Sources in the FRB 121102 Field (Geoffrey C. Bower)

Date & Time

Jan 6th at 2:20 PM until 2:30 PM




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Author(s): Geoffrey C. Bower1, Shami Chatterjee3, Robert Wharton3, Casey J. Law9, Jason Hessels2, Sarah Spolaor8, Matthew W. Abruzzo4, Cees Bassa2, Bryan J. Butler8, James M. Cordes3, Paul Demorest8, Victoria M. Kaspi5, Maura McLaughlin10, Scott M. Ransom8, Paul Scholz5, Andrew Seymour7, Laura Spitler6, Shriharsh P. Tendulkar5

Institution(s): 1. ASIAA, 2. ASTRON, 3. Cornell University, 4. Haverford College, 5. McGill, 6. MPIfR, 7. NAIC, 8. NRAO, 9. UC Berkeley, 10. WVU

Contributing team(s): PALFA Survey, VLA+AO FRB121102 Simultaneous Campaign Team, EVN FRB121102 Campaign Team, realfast team

Fast radio bursts are millisecond duration radio pulses of unknown origin. With dispersion measures substantially in excess of expected Galactic contributions, FRBs are inferred to originate extragalactically, implying very high luminosities. Models include a wide range of high energy systems such as magnetars, merging neutron star binaries, black holes, and strong stellar magnetic fields driving coherent radio emission. Central to the mystery of FRB origins are the absence of confirmed host objects at any wavelength. This is primarily the result of the poor localization from single dish detection of FRBs. Of the approximately 20 known examples, only one, FRB 121102, has been observed to repeat. This repetition presents an opportunity for detailed follow-up if interferometric localization to arcsecond accuracy can be obtained. The Very Large Array has previously been used to localize individual pulses from pulsars and rotating radio transients to arcsecond localizaiton. We present here the results of radio observations of the field of FRB 121102 that permit us to constrain models of possible progenitors of this bursting source. These observations can characterize active galactic nuclei, stars, and other progenitor objects.

Presenting Authors