A dataset provided by the European Space Agency

Name 065281
Title Solving the Mystery of Dark Matter with XMM-Newton
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652810101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652810201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652810301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652810401

DOI 10.5270/esa-cm07j5a
Author Dr Michael Loewenstein
Description The sterile neutrino is a dark matter candidate that emits an X-ray through radiative decay. We initiated the first dedicated X-ray search for dark matter, deriving new constraints on sterile neutrinos from Suzaku data on the Ursa Minor dwarf spheroidal galaxy, and a marginal detection of a sterile neutrino line at 2.5 keV in the extreme dark matter dwarf spheroidal Willman 1. This tentative detection can only be tested with XMM-Newton EPIC. We propose 75-100 ksec observations (including offset pointings) of Willman 1, as well as Segue 1 and Ursa Major II. Confirmation by XMM-Newton would be of incomparable astrophysical importance, pointing the way to new physics, and implying that future X-ray spectroscopic missions will directly map the dark distribution and its evolution.
Publication Dark Matter Search Using XMM-Newton Observations of Willman 1 . Loewenstein, Michael, Kusenko, Alexander, . ApJ . 751-82 . 2012 . 2012ApJ...751...82L ,
Constraints on 3.55 keV line emission from stacked observations of dwarf spheroidal galaxies . Malyshev, D., Neronov, A., . PhRvD . 90-103506 . 2014 . 2014PhRvD..90j3506M ,
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 ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function . Vagnetti, F., Middei, R., et all. . A&A . 593-55 . 2016 . 2016A&A...593A..55V ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Searching for gamma-ray signature in WHSP blazars. Fermi-LAT detection of 150 excess signal in the 0.3-500 GeV band . Arsioli, B., Chang, Y.-L., . A&A . 598-134 . 2017 . 2017A&A...598A.134A ,
AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton . Svoboda, J., Guainazzi, M., . A&A . 603-127 . 2017 . 2017A&A...603A.127S ,
XMM-Newton study of X-ray sources in the field of Willman 1 dw...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-10-22T02:02:05Z/2010-11-01T09:35:04Z
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 2011-12-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-12-23T00:00:00Z, 065281, 17.56_20190403_1200. https://doi.org/10.5270/esa-cm07j5a