Phase-Resolved Spectroscopy of Fermi LAT Blind Search Pulsars

Details Phase-Resolved Spectroscopy of Fermi LAT Blind Search Pulsars Phase-Resolved Spectroscopy of Fermi LAT Blind Search Pulsars

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21538807d&link_type=abstract

American Astronomical Society, AAS Meeting #215, #388.07; Bulletin of the American Astronomical Society, Vol. 42, p.604

Astronomy and Astrophysics

Astronomy

Scientific paper

The high sensitivity of the Fermi Large Area Telescope has led to the discovery of 16 gamma-ray pulsars, found without the aid of radio ephemerides. Most of these blind search pulsars are either radio-faint or radio-quiet, and represent a population with a different set of observational biases than those inherent in radio pulsars. For example, they likely exhibit a broader range of inclinations relative to the magnetic axis, presenting an opportunity to study previously unobserved magnetospheric geometries. We present here energy-dependent light curves and phase-dependent spectral parameters of a selection of the blind search pulsars, and show there is significant variation in the cutoff energy with phase.

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