Constraining the Galactic millisecond pulsar population usingFermiLarge Area Telescope
- 4 June 2013
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 554, A62
- https://doi.org/10.1051/0004-6361/201219676
Abstract
No abstract availableThis publication has 33 references indexed in Scilit:
- FERMI-LAT OBSERVATIONS OF THE DIFFUSE γ-RAY EMISSION: IMPLICATIONS FOR COSMIC RAYS AND THE INTERSTELLAR MEDIUMThe Astrophysical Journal, 2012
- FERMI LARGE AREA TELESCOPE FIRST SOURCE CATALOGThe Astrophysical Journal Supplement Series, 2010
- THE FIRST FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARSThe Astrophysical Journal Supplement Series, 2010
- DISCOVERY OF PULSED γ-RAYS FROM PSR J0034–0534 WITH THEFERMILARGE AREA TELESCOPE: A CASE FOR CO-LOCATED RADIO AND γ-RAY EMISSION REGIONSThe Astrophysical Journal, 2010
- Spectrum of the Isotropic Diffuse Gamma-Ray Emission Derived from First-Year Fermi Large Area Telescope DataPhysical Review Letters, 2010
- A Population of Gamma-Ray Millisecond Pulsars Seen with the Fermi Large Area TelescopeScience, 2009
- PULSED GAMMA RAYS FROM THE MILLISECOND PULSAR J0030+0451 WITH THEFERMILARGE AREA TELESCOPEThe Astrophysical Journal, 2009
- The magnetic fields, ages, and original spin periods of millisecond pulsarsThe Astrophysical Journal, 1994
- A new class of radio pulsarsNature, 1982
- Parameter estimation in astronomy through application of the likelihood ratioThe Astrophysical Journal, 1979