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A 24-Hour Global Campaign To Assess Precision Timing of the Millisecond Pulsar J1713+0747
T. Dolch, M. T. Lam, J. M. Cordes +40
The radio millisecond pulsar J1713+0747 is regarded as one of the highest-precision clocks in the sky, and is regularly timed for the purpose of detecting gravitational waves. The…
Six Faint Gamma-ray Pulsars Seen with the Fermi Large Area Telescope -- Towards a Sample Blending into the Background
X. Hou, D. A. Smith, L. Guillemot +11
Context: GeV gamma-ray pulsations from over 140 pulsars have been characterized using the Fermi Large Area Telescope, enabling improved understanding of the emission regions within…
Probing the gamma-ray emission from HESS J1834-087 using H.E.S.S. and Fermi LAT observations
The H. E. S. S. Collaboration, :, A. Abramowski +228
Previous observations with HESS have revealed the existence of an extended very-high-energy (VHE; E>100 GeV) gamma-ray source, HESS J1834-087, coincident with the SNR W41. The orig…
Constraints on the Emission Geometries and Spin Evolution of Gamma-ray Millisecond Pulsars
T. J. Johnson, C. Venter, A. K. Harding +9
Millisecond pulsars (MSPs) are a growing class of gamma-ray emitters. Pulsed gamma-ray signals have been detected from more than 40 MSPs with the Fermi Large Area Telescope (LAT).…
On the non-detection of gamma-rays from energetic millisecond pulsars -- dependence on viewing geometry
L. Guillemot, T. M. Tauris
Millisecond pulsars (MSPs) and normal non-recycled pulsars are both detected in -rays. However, it appears that a much larger fraction of known energetic and nearby MSPs are det…