A dataset provided by the European Space Agency

Name 055570
Title Pulse Searches of Probable GeV Pulsars Associated with TeV Sources
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555700101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555700201

DOI 10.5270/esa-n7vyfuo
Author Dr Mallory Roberts
Description There are several likely pulsars in EGRET error boxes which have been detected in X-rays and are probably associated with known TeV sources. Here we propose XMM-Newton studies of three of them: GeV J1825-1310 (the Eel), the Rabbit, and GeV J1907+0557, with the primary goal of detecting pulsations using the PN in small window mode. They are also within X-ray pulsar wind nebulae, and the MOS imagers will be useful in studying the large scale structure of the nebulae.
Publication The Second Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars . Abdo, A. A., Ajello, M., et all. . ApJS . 208-17 . 2013 . 2013ApJS..208...17A ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
The soft gamma-ray pulsar population: a high-energy overview . Kuiper, L., Hermsen, W., . MNRAS . 449-3827 . 2015 . 2015MNRAS.449.3827K ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Characterizing X-Ray Properties of the Gamma-Ray Pulsar PSR J1418-6058 in the Rabbit Pulsar Wind Nebula . Kim, Minjun, An, Hongjun, . ApJ . 892-5 . 2020 . 2020ApJ...892....5K ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-02-21T14:13:00Z/2009-02-23T03:39:40Z
Version PPS_NOT_AVAILABLE
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 2010-03-31T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-03-31T00:00:00Z, 055570, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-n7vyfuo