Cosmic rays are particles (mostly protons) accelerated to relativistic speeds. Despite wide
agreement that supernova remnants (SNRs) are the sources of galactic cosmic rays, …

This catalog summarizes 117 high-confidence⩾ 0. 1 GeV gamma-ray pulsar detections using
three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite. Half …

We present observations of the young supernova remnant (SNR) RX J1713. 7− 3946 with the
Fermi Large Area Telescope (LAT). We clearly detect a source positionally coincident with …

The Fermi Large Area Telescope (LAT) First Source Catalog (1FGL) provided spatial,
spectral, and temporal properties for a large number of γ-ray sources using a uniform analysis …

… of the Vela pulsar (De Luca, Mignani, & Caraveo 2000) and to quantify the overall reliability
of our astrometric approach (De Luca, Mignani, & Caraveo 2001). In the following we shall …

… them as σ(R 68 , R 95 ) and γ(R 68 , R 95 ). We model the energy dependence of the 68%
and 95% containment radii with two independent scaling functions, R 68 (E) and R 95 (E), …

… No candidate counterpart is detected in the Chandra error circle (nor in the intersection of
the MOS ones) down to R ∼ 27.1 and V ∼ 27.3, which we assume as upper limits on the …

… The flux is then F∝R 2 T 4 , where R and T are the radius and temperature of the cap, … of a
cap, the emitting area decreases as R 2 ∝t −0.08 and R 2 ∝t −0.97 before and after the break…

… About 40 years after identification of the optical counterpart of the Crab pulsar, only a few
rotation-powered pulsars have been identified in the optical domain (see Mignani 2009a,b, for …

Context.Our knowledge of the optical spectra of Isolated Neutron Stars (INSs) is limited by
their intrinsic faintness. Among the fourteen optically identified INSs, medium resolution …