2017A&A...605A..51K


Query : 2017A&A...605A..51K

2017A&A...605A..51K - Astronomy and Astrophysics, volume 605A51-51 (2017/9-1)

On the use of C-stat in testing models for X-ray spectra.

KAASTRA J.S.

Abstract (from CDS):

Context. It has been shown that for the analysis of X-ray spectra the C-statistic, contrary to the χ2-statistic, provides unbiased estimates of the model parameters and their uncertainty ranges.
Aims. However, it is often stated that the C-statistic cannot be used to carry out statistical tests on the goodness of fit of the model, and therefore several investigations are still based on χ2-statistics.
Methods. Here we show that it is straightforward to calculate the expected value and variance of the C-statistic so that it can be used in tests.
Results. We provide formulae and simple numerical approximations to evaluate these expected values and variances. We also give examples indicating that tests based on only the expected value and variance of the C-statistic are reliable for spectra even with only ∼30 counts.
Conclusions. The C-statistic can be used for statistical tests such as assessing the goodness of fit of a spectral model.

Abstract Copyright: © ESO, 2017

Journal keyword(s): instrumentation: spectrographs - methods: data analysis - methods: statistical - X-rays: general - X-rays: general

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 ACO 426 ClG 03 19 47.6 +41 30 54           ~ 2508 1
2 * alf Aur SB* 05 16 41.35871 +45 59 52.7693 1.33 0.88 0.08 -0.52 -0.96 G3III: 1207 0

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