Volume 472, Number 1, September II 2007
|Page(s)||21 - 27|
|Section||Cosmology (including clusters of galaxies)|
|Published online||09 July 2007|
In search of an unbiased temperature estimator for statistically poor X-ray spectra
Università degli Studi di Milano, Dip. di Fisica, via Celoria 16, 20133 Milano, Italy e-mail: email@example.com
2 INAF-IASF Milano, via Bassini 15, 20133 Milano, Italy
Accepted: 29 May 2007
Although commonly employed by X-ray astronomers, maximum likelihood estimators are known to be biased. In this paper we investigate the bias associated with 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 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 overcoming this problem and the most effective is a technique that allows us to correct the bias a posteriori. Extensive Monte Carlo simulations show that our correction returns excellent results under different conditions.
Key words: methods: statistical / X-rays: galaxies: clusters
© ESO, 2007
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