SEARCHING FOR THE 3.5 keV LINE IN THE STACKED SUZAKU OBSERVATIONS OF GALAXY CLUSTERS
We perform a detailed study of the stacked Suzaku observations of 47 galaxy clusters, spanning a redshift range of 0.01–0.45, to search for the unidentified 3.5 keV line. This sample provides an independent test for the previously detected line. We detect a 2σ-significant spectral feature at 3.5 keV...
Main Authors: | Markevitch, Maxim, Foster, Adam, Loewenstein, Mike, Randall, Scott W., Smith, Randall K., Bulbul, Gul E, Miller, Eric D, Bautz, Mark |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2017
|
Online Access: | http://hdl.handle.net/1721.1/108042 |
Similar Items
-
Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster
by: Bulbul, Gul E, et al.
Published: (2017) -
RADIAL PROFILE OF THE 3.5 keV LINE OUT TO R[subscript 200] IN THE PERSEUS CLUSTER
by: Franse, Jeroen, et al.
Published: (2017) -
Was There a 3.5 keV Line?
by: Christopher Dessert, et al.
Published: (2024-01-01) -
THERMAL AND CHEMICAL EVOLUTIONS OF GALAXY CLUSTERS OBSERVED WITH SUZAKU
by: Kosuke Sato, et al.
Published: (2013-12-01) -
The 3.5 keV line from stringy axions
by: Michele Cicoli, et al.
Published: (2017-10-01)