activity
20042009
most citedPulsars versus Dark Matter Interpretation of ATIC/PAMELA

197 citations · 531 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2009189 cited

A Dynamical Model for the Evolution of a Pulsar Wind Nebula inside a Non-Radiative Supernova Remnant

Joseph D. Gelfand, Patrick O. Slane, Weiqun Zhang

A pulsar wind nebula inside a supernova remnant provides a unique insight into the properties of the central neutron star, the relativistic wind powered by its loss of rotational e…

astro-ph.IM2009

Research Science and Education: The NSF's Astronomy and Astrophysics Postdoctoral Fellowship

Dara Norman, Marcel Agueros, Timothy M. Brown +29

The NSF's Astronomy and Astrophysics Postdoctoral Fellowship (AAPF) is exceptional among the available postdoctoral awards in Astronomy and Astrophysics. The fellowship is one of t…

astro-ph.HE2009197 cited

Pulsars versus Dark Matter Interpretation of ATIC/PAMELA

Dmitry Malyshev, Ilias Cholis, Joseph Gelfand

In this paper, we study the flux of electrons and positrons injected by pulsars and by annihilating or decaying dark matter in the context of recent ATIC, PAMELA, Fermi, and HESS d…

astro-ph2007118 cited

The Compact X-ray Source 1E 1547.0-5408 and the Radio Shell G327.24-0.13: A New Proposed Association between a Candidate Magnetar and a Candidate Supernova Remnant

Joseph D. Gelfand, B. M. Gaensler

We present X-ray, infrared and radio observations of the field centered on X-ray source 1E 1547.0-5408 in the Galactic Plane. A new Chandra observation of this source shows it is u…

astro-ph200727 cited

The Radio Emission, X-ray Emission, and Hydrodynamics of G328.4+0.2: A Comprehensive Analysis of a Luminous Pulsar Wind Nebula, its Neutron Star, and the Progenitor Supernova Explosion

Joseph D. Gelfand, B. M. Gaensler, Patrick O. Slane +3

We present new observational results obtained for the Galactic non-thermal radio source G328.4+0.2 to determine both if this source is a pulsar wind nebula or supernova remnant, an…

astro-ph2005

A Wide Field, Low Frequency Radio Image of the Field of M31: II. -- Source Classification and Discussion

Joseph D. Gelfand, T. J. W. Lazio, B. M. Gaensler

We have previously presented the results of a 325 MHz radio survey of M31, conducted with the A-configuration of the Very Large Array. In this survey, a total of 405 radio sources…