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THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
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 are neutron stars
The First Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
The dramatic increase in the number of known gamma-ray pulsars since the launch of the Fermi Gamma-ray Space Telescope (formerly GLAST) offers the first opportunity to study a population of these
LOFAR - low frequency array
TLDR
In dit artikel zullen the authors LOFAR beschrijven: van de astronomische mogelijkheden met de nieuwe telescoop tot aan een nadere technische beshrijving of het instrument.
A Population of Gamma-Ray Millisecond Pulsars Seen with the Fermi Large Area Telescope
TLDR
Fermi Large Area Telescope data is searched for pulsations from all known millisecond pulsars outside of stellar clusters, finding gamma-ray pulsations for eight of them, suggesting that they share the same basic emission mechanism with standard gamma-Ray pulsars.
Evolution of the Magnetic Field Structure of the Crab Pulsar
TLDR
Long-term measurements show the systematic evolution of the radiation pattern of the pulsar in the Crab Nebula, one of the youngest neutron stars known, and the changing component separation indicates that the axis of the dipolar magnetic field, embedded in the neutron star, is moving toward the stellar equator.
The subpulse modulation properties of pulsars at 21 cm
We present the results of a systematic, unbiased search for subpulse modulation of 187 pulsars performed with the Westerbork Synthesis Radio Telescope (WSRT) in the Netherlands at an observing
DETECTION OF THE ENERGETIC PULSAR PSR B1509–58 AND ITS PULSAR WIND NEBULA IN MSH 15–52 USING THEFERMI-LARGE AREA TELESCOPE
We report the detection of high-energy gamma-ray emission from the young and energetic pulsar PSR B1509-58 and its pulsar wind nebula (PWN) in the composite supernova remnant G320.4-1.2 (aka MSH 15
An Atlas for Interpreting γ-Ray Pulsar Light Curves
We have simulated a population of young spin-powered pulsars and computed the beaming pattern and light curves for the three main geometrical models: polar-cap emission, two-pole caustic (slot gap)
The glitch-induced identity changes of PSR J1119−6127
Rotation-powered radio pulsars are generally observed to pulse regularly in the radio band, but this is not the case for so-called rotating radio transients (RRATs) which emit only sporadic bursts of
Precise γ-ray timing and radio observations of 17 Fermi γ-ray pulsars
We present precise phase-connected pulse timing solutions for 16 γ-ray-selected pulsars recently discovered using the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope plus one very
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