We propose a mini-survey of unclassified Fermi sources from the 2FGL catalog.Using an intelligent parameter selection, we have identified a sub-sample thatis likely to be dominated by pulsars with some inclusion of high-mass XRBs. Weaim to identify 7 new gamma-ray pulsars and their X-ray counterparts, and thussignificantly increase the population of pulsars detected in both gamma-rays andX-rays. The existing limited data hint at an intriguing change in the slope ofthe L(Edot) dependence at log(Edot)=35-36 erg/s. By identifying more pulsars inboth gamma- and X-rays, we will be able to confirm the existence of those breaksand investigate their origin. We will also identify new X-ray bright pulsarssuitable for detailed study using the prudent snap-shot approach.
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2014-10-10T00:04:49Z/2014-11-16T20:48:00Z
Version
17.56_20190403_1200
Mission Description
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
European Space Agency, Dr Blagoy Rangelov, 2015, 'Revealing pulsars hidden in the 2nd Fermi Catalogue', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ady1zfq
