A dataset provided by the European Space Agency

Name 080261
Title Searching for soft gamma-ray pulsars in unassociated Fermi LAT sources with XMM
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802610301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802610501

DOI https://doi.org/10.5270/esa-fo6uftt
Author European Space Agency
Description Fermi has detected over 200 gamma-ray pulsars of varying types in 8 years of
operations, but the so-called soft (< 100 MeV) gamma-ray pulsars remain
relatively elusive. Typically single-peaked, younger and more energetic than GeV
pulsars, such pulsars were particularly hard to detect with Fermi prior to the
release of Pass 8. Increasing the size of this population may shed light on our
current understanding of high-energy pulsars and the effect that various
parameters (e.g. geometry) may have on the observed emission. We propose short
5ks XMM observations of our top 5 soft gamma-ray pulsar candidates to enable the
first sensitive blind searches for such pulsars using LAT data below 100 MeV.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2017-07-08T07:53:47Z/2017-12-17T12:31:32Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2019-01-08T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2019, Searching For Soft Gamma-Ray Pulsars In Unassociated Fermi Lat Sources With Xmm, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-fo6uftt