Bayesian model comparison and analysis of the Galactic disc population of gamma-ray millisecond pulsars
Author:
Affiliation:
1. Gravitation Astroparticle Physics Amsterdam (GRAPPA), Institute for Theoretical Physics Amsterdam and Delta Institute for Theoretical Physics, University of Amsterdam, Science Park 904, NL-1098 XH Amsterdam, the Netherlands
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/481/3/3966/25857794/sty2529.pdf
Reference64 articles.
1. The consistency of Fermi-LAT observations of the galactic center with a millisecond pulsar population in the central stellar cluster
2. A Population of Gamma-Ray Millisecond Pulsars Seen with the Fermi Large Area Telescope
3. PULSED GAMMA RAYS FROM THE MILLISECOND PULSAR J0030+0451 WITH THEFERMILARGE AREA TELESCOPE
4. THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
5. FERMI LARGE AREA TELESCOPE THIRD SOURCE CATALOG
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