On the ability of the spectroscopic Sunyaev-Zeldovich effect measurements to determine the temperature structure of galaxy clusters

Astronomy and Astrophysics

Volumn 520, Issue 3, 2010, Pages

  Colafrancesco, S ^a,b   Marchegiani, P ^b,c  

^a ASI   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^c UNIVERSITÀ DI ROMA LA SAPIENZA   (Italy)

Author keywords

Cosmology: theory; Galaxies: clusters: general

Indexed keywords

ANALYSIS RESULTS; CLUSTER PROTOTYPE; CLUSTER TEMPERATURE; COSMOLOGY: THEORY; ELECTRON DISTRIBUTION FUNCTION; FITTING PROCEDURE; GALAXIES: CLUSTERS: GENERAL; GALAXY CLUSTERS; HIGH TEMPERATURE; HIGH-REDSHIFT; IMAGING CAPABILITIES; INVERSION TECHNIQUES; LOW TEMPERATURES; MODERATE RESOLUTION; NON-ISOTHERMAL TEMPERATURE; NONTHERMAL; NONUNIFORM TEMPERATURE; OPTIMAL FREQUENCY; PARAMETERS CHARACTERIZING; RADIAL DISTANCE; RADIO GALAXIES; RELATIVISTIC ELECTRON; RELATIVISTIC PLASMAS; SPATIAL RESOLUTION; SPATIALLY RESOLVED; SPECTROSCOPIC MEASUREMENTS; SUNYAEV-ZELDOVICH EFFECTS; SZ EFFECTS; TEMPERATURE DISTRIBUTION MEASUREMENT; TEMPERATURE PROFILES; TEMPERATURE STRUCTURE; THERMAL PLASMA; WIDE FREQUENCY RANGE; X-RAY OBSERVATIONS;

COSMOLOGY; DISTRIBUTION FUNCTIONS; FREQUENCY BANDS; TEMPERATURE CONTROL; TEMPERATURE DISTRIBUTION; THERMOANALYSIS;

GALAXIES;

EID: 77957189324     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913115     Document Type: Article

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