Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-05-29
Phys.Rev.D80:015018,2009
Astronomy and Astrophysics
Astrophysics
9 pages, 9 figures, accepted for publication in A&A
Scientific paper
10.1103/PhysRevD.80.015018
Although commonly employed by X-ray astronomers, maximum likelihood estimators are known to be biased. In this paper we investigate the bias associated to the measure of the temperature from an X-ray thermal spectrum. We show that, in the case of low surface brightness regions, commonly adopted estimators, such as those based on chi squared and Cash statistics, return strongly biased results. We stress that this can have strong implications when measuring the temperature of cluster outer regions with current experiments. We consider various approaches to overcome this problem, the most effective is a technique which allows us to correct the bias a posteriori. Extensive montecarlo simulations show that our correction returns excellent results under different conditions.
Leccardi Alberto
Molendi Silvano
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