Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-
spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …

Fewer than a dozen gamma-ray pulsars were known when the Fermi Gamma-ray Space
Telescope was launched on 2008 June 11, and the extent and diversity of the population …

The rapid proliferation of online content producing and sharing technologies resulted in an
explosion of user-generated content (UGC), which now extends to scientific data. Citizen …

ABSTRACT The Fermi Large Area Telescope gamma-ray source 3FGL J2039. 6–5618
contains a periodic optical and X-ray source that was predicted to be a 'redback'millisecond …

Identifying as many gamma-ray pulsars as possible in the Fermi Large Area Telescope
(LAT) data helps test pulsar emission models by comparing predicted and observed …

We present results from deep observations toward the Cygnus region using 300 hr of very
high energy (VHE) γ-ray data taken with the VERITAS Cerenkov telescope array and over 7 …

The population of young, non-recycled pulsars with spin-down energies erg s− 1 is sampled
predominantly at γ-ray and radio wavelengths. A total of 137 such pulsars are known, with …

We present observations of 35 high spin-down energy radio pulsars using the MeerKAT
telescope. Polarization profiles and associated parameters are also presented. We derive …

Context. The latest source catalog of the Fermi-LAT telescope contains more than 7000 γ-
ray sources at giga-electronvolt energies, with the two dominant source classes thought to …

We report the identification from multiwavelength observations of the Fermi Large Area
Telescope (LAT) source 4FGL J1405. 1− 6119 (= 3FGL J1405. 4− 6119) as a high-mass …