| Issue |
EAS Publications Series
Volume 20, 2006
Mass Profiles and Shapes of Cosmological Structures
|
|
|---|---|---|
| Page(s) | 295 - 296 | |
| DOI | https://doi.org/10.1051/eas:2006097 | |
| Published online | 19 May 2006 | |
G.A. Mamon, F. Combes, C. Deffayet and B. Fort (eds)
EAS Publications Series, 20 (2006) 295-296
Bias on Estimates of X-ray Cluster Mass
1
Dipartimento di Astronomia, Università di Padova,
vicolo dell'Osservatorio 2, 35122 Padova, Italy,
2
INAF, Osservatorio Astronomia di Bologna, via
Ranzani 1, 40127 Bologna, Italy
3
Dipartimento di Astronomia, Università di
Bologna, via Ranzani 1, 40127 Bologna, Italy
4
Dipartimento di Fisica, Università di Roma Tor
Vergata, via della Ricerca Scientifica 1, 00133 Roma, Italy
5
Dipartimento di Astronomia, Università di
Trieste, via Tiepolo 11, 34131 Trieste, Italy
6
MPA,
Karl-Schwarzschild Strasse 1, 85748 Garching bei München, Germany
7
Institute of Theoretical Physics, Chinese
Accademy of Sciences, Beijing 100080, China
8
Dipartimento di Fisica, Università di Torino, via Giuria 1, 10125 Torino, Italy
Corresponding author: rasia@pd.astro.it
We examine the systematics affecting the X-ray mass estimators applied to Chandra-like long exposures images of five simulated clusters.
© EAS, EDP Sciences, 2006