RHAPSODY-G simulations: galaxy clusters as baryonic closed boxes and the covariance between hot gas and galaxies
dc.contributor.author
Wu, Hao-Yi
dc.contributor.author
Evrard, August E.
dc.contributor.author
Hahn, Oliver
dc.contributor.author
Martizzi, Davide
dc.contributor.author
Teyssier, Romain
dc.contributor.author
Wechsler, Risa H.
dc.date.accessioned
2017-06-11T19:30:50Z
dc.date.available
2017-06-11T19:30:50Z
dc.date.issued
2015-09
dc.identifier.issn
0035-8711
dc.identifier.issn
1365-2966
dc.identifier.other
10.1093/mnras/stv1434
dc.identifier.uri
http://hdl.handle.net/20.500.11850/104565
dc.identifier.doi
10.3929/ethz-b-000104565
dc.format
application/pdf
dc.language.iso
en
dc.publisher
Oxford University Press
dc.rights.uri
http://rightsstatements.org/page/InC-NC/1.0/
dc.subject
Methods: numerical
dc.subject
Galaxies: clusters: general
dc.subject
Cosmology: theory
dc.subject
X-rays: galaxies: clusters
dc.title
RHAPSODY-G simulations: galaxy clusters as baryonic closed boxes and the covariance between hot gas and galaxies
dc.type
Journal Article
dc.rights.license
In Copyright - Non-Commercial Use Permitted
ethz.journal.title
Monthly Notices of the Royal Astronomical Society
ethz.journal.volume
452
ethz.journal.issue
2
ethz.journal.abbreviated
Mon. Not. R. Astron. Soc.
ethz.pages.start
1982
ethz.pages.end
1991
ethz.version.deposit
publishedVersion
ethz.notes
Published online 21 July 2015. It was possible to publish this article open access thanks to a Swiss National Licence with the publisher
ethz.identifier.wos
ethz.identifier.scopus
ethz.publication.status
published
ethz.date.deposited
2017-06-11T19:31:44Z
ethz.source
ECIT
ethz.identifier.importid
imp593653809f71631367
ethz.ecitpid
pub:163686
ethz.eth
yes
ethz.availability
Open access
ethz.date.embargoend
2018-07-21
ethz.rosetta.installDate
2017-07-14T13:31:42Z
ethz.rosetta.lastUpdated
2024-02-01T23:16:17Z
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true
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