Deep XMM Observations of Draco rule out a dark matter decay origin for
the 3.5 keV line
T. Jeltema, and S. Profumo. (2015)cite arxiv:1512.01239Comment: 4 pages, 3 figures, submitted to MNRAS.
Abstract
We searched for an X-ray line at energies around 3.5 keV in deep, ~1.6 Msec
XMM-Newton observations of the dwarf spheroidal galaxy Draco. No line was
found. The data in this energy range are completely consistent with a simple
power law X-ray background, dominated by particle background, plus instrumental
lines; the addition of a ~3.5 keV line feature gives no improvement to the fit.
The corresponding upper limit on the line flux rules out a dark matter decay
origin for the 3.5 keV line found in observations of clusters of galaxies and
in the Galactic Center at greater than 99% C.L..
Description
[1512.01239] Deep XMM Observations of Draco rule out a dark matter decay origin for the 3.5 keV line
%0 Generic
%1 jeltema2015observations
%A Jeltema, Tesla E.
%A Profumo, Stefano
%D 2015
%K dark decay dwarf emission line matter
%T Deep XMM Observations of Draco rule out a dark matter decay origin for
the 3.5 keV line
%U http://arxiv.org/abs/1512.01239
%X We searched for an X-ray line at energies around 3.5 keV in deep, ~1.6 Msec
XMM-Newton observations of the dwarf spheroidal galaxy Draco. No line was
found. The data in this energy range are completely consistent with a simple
power law X-ray background, dominated by particle background, plus instrumental
lines; the addition of a ~3.5 keV line feature gives no improvement to the fit.
The corresponding upper limit on the line flux rules out a dark matter decay
origin for the 3.5 keV line found in observations of clusters of galaxies and
in the Galactic Center at greater than 99% C.L..
@misc{jeltema2015observations,
abstract = {We searched for an X-ray line at energies around 3.5 keV in deep, ~1.6 Msec
XMM-Newton observations of the dwarf spheroidal galaxy Draco. No line was
found. The data in this energy range are completely consistent with a simple
power law X-ray background, dominated by particle background, plus instrumental
lines; the addition of a ~3.5 keV line feature gives no improvement to the fit.
The corresponding upper limit on the line flux rules out a dark matter decay
origin for the 3.5 keV line found in observations of clusters of galaxies and
in the Galactic Center at greater than 99% C.L..},
added-at = {2015-12-07T10:09:18.000+0100},
author = {Jeltema, Tesla E. and Profumo, Stefano},
biburl = {https://www.bibsonomy.org/bibtex/24515c9c7dae10f71c143ae94a958e363/miki},
description = {[1512.01239] Deep XMM Observations of Draco rule out a dark matter decay origin for the 3.5 keV line},
interhash = {54b7054cb6be4cc60cc77f8ef1811ae2},
intrahash = {4515c9c7dae10f71c143ae94a958e363},
keywords = {dark decay dwarf emission line matter},
note = {cite arxiv:1512.01239Comment: 4 pages, 3 figures, submitted to MNRAS},
timestamp = {2015-12-07T10:09:18.000+0100},
title = {Deep XMM Observations of Draco rule out a dark matter decay origin for
the 3.5 keV line},
url = {http://arxiv.org/abs/1512.01239},
year = 2015
}