Add to ORKGWe present an atlas of X and gamma-ray pulse profiles of PSR 0531+21 (Crab pulsar) measured since 1967. This atlas, containing 250 profiles, is useful to study in detail the behaviour with time and energy of this important source and to test models of the emission geometrical pattern. The atlas database is also accessible from Mosaic. An analysis of the energy dependence and time changes of the Crab pulsar light curve (and in particular of the P2/P1 ratio), based on the atlas database, is presented
Context. Studies of the high-energy emission regions of rotation-powered pulsars are typically based...
Observations of the pulsating component of NP 0532 at 2.2 and 1.65 μ are given. The energy density p...
We use 73 h of stereoscopic data taken with the MAGIC telescopes to investigate the very high-energy...
An atlas of X { and γ{ray pulse proles of the Crab pulsar (PSR 0531+21): An analysis of energy and t...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
The FIGARO II experiment observed the Crab pulsar in the energy range 0.15-4 MeV during two transmed...
This article is the first in the series that analyze about 1.87 million periods of PSR B0531+21 (Cr...
The stability of the optical pulse of the Crab pulsar is analyzed based on the 1 $\mu$s resolution o...
We present the time-averaged characteristics of the Crab pulsar in the 0.75-30 MeV energy window usi...
We present the time-averaged characteristics of the Crab pulsar in the 0.75-30 MeV energy window usi...
As is well known, the Crab pulsar displays a light curve with a characteristic double peak profile h...
The spectrum of the Crab pulsar was measued from 2 to 50 keV as a function of pulse phase and a prog...
We use 73 h of stereoscopic data taken with the MAGIC telescopes to investigate the very high-energy...
We use 73 h of stereoscopic data taken with the MAGIC telescopes to investigate the very high-energy...
The results of the Crab pulsar observations with the photometrical MANIA (Multichannel Analysis of N...
Context. Studies of the high-energy emission regions of rotation-powered pulsars are typically based...
Observations of the pulsating component of NP 0532 at 2.2 and 1.65 μ are given. The energy density p...
We use 73 h of stereoscopic data taken with the MAGIC telescopes to investigate the very high-energy...
An atlas of X { and γ{ray pulse proles of the Crab pulsar (PSR 0531+21): An analysis of energy and t...
Restricted Access. An open-access version is available at arXiv.org (one of the alternative location...
The FIGARO II experiment observed the Crab pulsar in the energy range 0.15-4 MeV during two transmed...
This article is the first in the series that analyze about 1.87 million periods of PSR B0531+21 (Cr...
The stability of the optical pulse of the Crab pulsar is analyzed based on the 1 $\mu$s resolution o...
We present the time-averaged characteristics of the Crab pulsar in the 0.75-30 MeV energy window usi...
We present the time-averaged characteristics of the Crab pulsar in the 0.75-30 MeV energy window usi...
As is well known, the Crab pulsar displays a light curve with a characteristic double peak profile h...
The spectrum of the Crab pulsar was measued from 2 to 50 keV as a function of pulse phase and a prog...
We use 73 h of stereoscopic data taken with the MAGIC telescopes to investigate the very high-energy...
We use 73 h of stereoscopic data taken with the MAGIC telescopes to investigate the very high-energy...
The results of the Crab pulsar observations with the photometrical MANIA (Multichannel Analysis of N...
Context. Studies of the high-energy emission regions of rotation-powered pulsars are typically based...
Observations of the pulsating component of NP 0532 at 2.2 and 1.65 μ are given. The energy density p...
We use 73 h of stereoscopic data taken with the MAGIC telescopes to investigate the very high-energy...