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Radio Detection of the Fermi LAT Blind Search Millisecond Pulsar J1311-3430

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons40533

Pletsch,  H.
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Volltexte (frei zugänglich)

1210.6676
(Preprint), 263KB

ApJL_763_1_L13.pdf
(beliebiger Volltext), 412KB

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Zitation

Ray, P. S., Ransom, S. M., Cheung, C. C., Giroletti, M., Cognard, I., Camilo, F., et al. (2013). Radio Detection of the Fermi LAT Blind Search Millisecond Pulsar J1311-3430. Astrophysical Journal, 763: L13. doi:10.1088/2041-8205/763/1/L13.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-000E-EA17-E
Zusammenfassung
We report the detection of radio emission from PSR J1311-3430, the first millisecond pulsar discovered in a blind search of Fermi Large Area Telescope (LAT) gamma-ray data. We detected radio pulsations at 2 GHz, visible for <10% of ~4.5-hrs of observations using the Green Bank Telescope (GBT). Observations at 5 GHz with the GBT and at several lower frequencies with Parkes, Nancay, and the Giant Metrewave Radio Telescope resulted in non-detections. We also report the faint detection of a steep spectrum continuum radio source (0.1 mJy at 5 GHz) in interferometric imaging observations with the Jansky Very Large Array. These detections demonstrate that PSR J1311-3430, is not radio quiet and provides additional evidence that the radio beaming fraction of millisecond pulsars is very large. The radio detection yields a distance estimate of 1.4 kpc for the system, yielding a gamma-ray efficiency of 30%, typical of LAT-detected MSPs. We see apparent excess delay in the radio pulsar as the pulsar appears from eclipse and we speculate on possible mechanisms for the non-detections of the pulse at other orbital phases and observing frequencies.