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ERRATUM: 'MAPPING THE GAS TURBULENCE IN THE COMA CLUSTER: PREDICTIONS FOR ASTRO-H'The published version of this paper contained an error in Figure 5. This figure is intended to show the effect on the structure function of subtracting the bias induced by the statistical and systematic errors on the line shift. The filled circles show the bias-subtracted structure function. The positions of these points in the left panel of the original figure were calculated incorrectly. The figure is reproduced below (with the original caption) with the correct values for the bias-subtracted structure function. No other computations or figures in the original manuscript are affected.
Document ID
20170002479
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Zuhone, J. A.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Markevitch, M.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Zhuravleva, I.
(Stanford Univ. Stanford, CA, United States)
Date Acquired
March 23, 2017
Publication Date
March 1, 2016
Publication Information
Publication: The Astrophysical Journal
Publisher: AAS/IOP Publishing partnership
Volume: 819
Issue: 1
e-ISSN: 1538-4357
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
GSFC-E-DAA-TN40574
Distribution Limits
Public
Copyright
Other
Keywords
galaxies: clusters: intracluster medium- methods: numerical - techniques: spectr

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