About: Norbert Werner

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An Entity of Type : wikibase:Item, within Data Space : wikidata.demo.openlinksw.com associated with source document(s)

researcher

Attributes	Values
rdf:type	Item
field of work	wds:Q62634330-DCAEA738-6A11-4442-8FEC-792C3B89D537 wds:Q62634330-E2045A4E-5D75-4CAD-9FE5-D836A613B15B
field of work	physics astrophysics
description	forsker (nb) researcher (en) 研究者 (ja) wetenschapper (nl) дослідник (uk) эрдэмтэн (mn) հետազոտող (hy) slovenský vysokoškolský pedagog fyziky a astrofyziky (cs)
rdfs:label	Norbert Werner (cs) Norbert Werner (en) Norbert Werner (es) Norbert Werner (nb) N. Werner (nl) N. Werner (ast) Norbert Werner (sk) Norbert Werner (sq)
skos:prefLabel	Norbert Werner (cs) Norbert Werner (en) Norbert Werner (es) Norbert Werner (nb) N. Werner (nl) N. Werner (ast) Norbert Werner (sk) Norbert Werner (sq)
name	Norbert Werner (cs) Norbert Werner (en) Norbert Werner (es) Norbert Werner (nb) N. Werner (nl) N. Werner (ast) Norbert Werner (sk) Norbert Werner (sq)
given name	wds:Q62634330-35BEA7E5-FB9F-4842-ADEE-336387D55EA0
given name	Norbert
instance of	wds:Q62634330-08BEDCE1-C528-48E7-A364-29D405402244
NL CR AUT ID	wds:Q62634330-C36090F2-3942-4AEA-BC08-8CF540E881C8
instance of	Homo sapiens
NL CR AUT ID	mub20201073744
Masaryk University person ID	wds:Q62634330-ee30c832-4215-b7c7-326f-705efd386fca
Masaryk University person ID	239396
Google Scholar author ID	wds:Q62634330-f3b59060-49f2-c1fa-0a15-970524bb4ca2
Google Scholar author ID	D93yu9MAAAAJ
skos:altLabel	N. Werner (en)
occupation	wds:Q62634330-44C2C265-B89F-4B93-B800-51C44826DCCD wds:Q62634330-566891E9-171F-45C8-A805-AEFE2C59F8AB wds:Q62634330-81CC3CD0-A02D-425C-B786-B846A0D7237F
languages spoken, written or signed	wds:Q62634330-521E243A-F3CA-4411-A112-A6D64E228EAE
sex or gender	wds:Q62634330-96F5F3EB-7DA3-4C35-961E-B7457A5521CF
VIAF ID	wds:Q62634330-4F0F55CD-471F-4E6A-AEC5-D8D824D09311
date of birth	wds:Q62634330-FCA69CDC-E937-4EDA-B61B-923CF393F5F0
family name	wds:Q62634330-CCE85D51-FF5D-42F3-AE67-6451538AF180
VIAF ID	http://viaf.org/viaf/35154865870559940606
occupation	astrophysicist university teacher physicist
languages spoken, written or signed	Slovak
sex or gender	male
VIAF ID	35154865870559940606
date of birth	1981-01-01 00:00:00Z (xsd:dateTime)
family name	Werner
ORCID iD	wds:Q62634330-69A48F60-4532-476B-9B10-A61E714F8B9F
ORCID iD	https://orcid.org/0000-0003-0392-0120
ORCID iD	0000-0003-0392-0120
ResearcherID	wds:Q62634330-DDAB8A54-E1D4-4A81-A17E-463A0B4D667D
ResearcherID	G-2832-2019
is owl:sameAs of	Norbert Werner
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q62634330
is author of	A filament of dark matter between two clusters of galaxies A uniform metal distribution in the intergalactic medium of the Perseus cluster of galaxies Baryons at the Edge of the X-ray-Brightest Galaxy Cluster Turbulent heating in galaxy clusters brightest in X-rays. The ASTRO-H X-ray astronomy satellite Azimuthally resolved X-ray spectroscopy to the edge of the Perseus Cluster The ASTRO-H X-ray Observatory Hitomi X-ray observation of the pulsar wind nebula G21.5−0.9 Hitomi observations of the LMC SNR N 132 D: Highly redshifted X-ray emission from iron ejecta* Constraining supernova models using the hot gas in clusters of galaxies Chemical evolution in Sérsic 159-03 observed with XMM-Newton Linear Structures in the Core of the Coma Cluster of Galaxies The quiescent intracluster medium in the core of the Perseus cluster Glimpse of the highly obscured HMXB IGR J16318−4848 with Hitomi* Hitomi observation of radio galaxy NGC 1275: The first X-ray microcalorimeter spectroscopy of Fe-Kα line emission from an active galactic nucleus* Origin of central abundances in the hot intra-cluster medium. II. Chemical enrichment and supernova yield models Origin of central abundances in the hot intra-cluster medium. I. Individual and average abundance ratios from XMM-Newton EPIC Serendipitous discovery of an extended X-ray jet without a radio counterpart in a high-redshift quasar X-ray spectra of the Fe-L complex HitomiConstraints on the 3.5 keV Line in the Perseus Galaxy Cluster ORIGIN: metal creation and evolution from the cosmic dawn Atmospheric gas dynamics in the Perseus cluster observed with Hitomi* Search for thermal X-ray features from the Crab nebula with the Hitomi soft X-ray spectrometer* Detection of polarized gamma-ray emission from the Crab nebula with the Hitomi Soft Gamma-ray Detector† Solar chemical composition in the hot gas of cool-core ellipticals, groups, and clusters of galaxies Radial metal abundance profiles in the intra-cluster medium of cool-core galaxy clusters, groups, and ellipticals Mass–metallicity relation from cosmological hydrodynamical simulations and X-ray observations of galaxy groups and clusters Clusters of Galaxies: Beyond the Thermal View

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