Add to ORKGWe report the status of a search for pulsars in the Galactic Centre, using acompletely revised and improved high-sensitivity double-horn system at4.85-GHz. We also present calculations about the success rate of periodicitysearches for such a survey, showing that in contrast to conclusions in recentliterature pulsars can be indeed detected at the chosen search frequency
We performed a drift-scan pulsar survey using the Green Bank Telescope (GBT) in West Virginia, USA....
Context. Millisecond pulsars are very useful for determining the properties of neutron stars, for te...
The recent discovery of a magnetar in the Galactic Centre region has allowed Spitler et al. to chara...
We report the status of a search for pulsars in the Galactic Centre, using a completely revised and ...
We report the discovery of two highly dispersed pulsars in the direction of the Galactic Centre made...
We have used the Effelsberg 100-m radio telescope to conduct a 1400-MHz ($\lambda$ 21-cm) search for...
Pulsars in the Galactic centre promise to enable unparalleled tests of gravity theories and black ho...
The lack of detected pulsars at the Galactic Center (GC) region is a long-standing mystery. We argue...
Pulsars are rapidly-rotating, highly-magnetized compact neutron stars. Their strong gravitational an...
Contains fulltext : 252348.pdf (Publisher’s version ) (Open Access
International audienceThe high stellar density in the central parsecs around the Galactic Centre mak...
Radio pulsars in relativistic binary systems are unique tools to study the curved space-time around ...
Searches for millisecond pulsars (which we here loosely define as those with periods \u3c 20 ms) in ...
This dissertation concerns the planning, implementation, and results from a highly sensitive, automa...
Although high-sensitivity surveys have revealed a number of highly dispersed pulsars in the inner Ga...
We performed a drift-scan pulsar survey using the Green Bank Telescope (GBT) in West Virginia, USA....
Context. Millisecond pulsars are very useful for determining the properties of neutron stars, for te...
The recent discovery of a magnetar in the Galactic Centre region has allowed Spitler et al. to chara...
We report the status of a search for pulsars in the Galactic Centre, using a completely revised and ...
We report the discovery of two highly dispersed pulsars in the direction of the Galactic Centre made...
We have used the Effelsberg 100-m radio telescope to conduct a 1400-MHz ($\lambda$ 21-cm) search for...
Pulsars in the Galactic centre promise to enable unparalleled tests of gravity theories and black ho...
The lack of detected pulsars at the Galactic Center (GC) region is a long-standing mystery. We argue...
Pulsars are rapidly-rotating, highly-magnetized compact neutron stars. Their strong gravitational an...
Contains fulltext : 252348.pdf (Publisher’s version ) (Open Access
International audienceThe high stellar density in the central parsecs around the Galactic Centre mak...
Radio pulsars in relativistic binary systems are unique tools to study the curved space-time around ...
Searches for millisecond pulsars (which we here loosely define as those with periods \u3c 20 ms) in ...
This dissertation concerns the planning, implementation, and results from a highly sensitive, automa...
Although high-sensitivity surveys have revealed a number of highly dispersed pulsars in the inner Ga...
We performed a drift-scan pulsar survey using the Green Bank Telescope (GBT) in West Virginia, USA....
Context. Millisecond pulsars are very useful for determining the properties of neutron stars, for te...
The recent discovery of a magnetar in the Galactic Centre region has allowed Spitler et al. to chara...