English

Hardness Ratio Estimation in Low Counting X-ray Photometry

Astrophysics 2008-11-26 v1

Abstract

Hardness ratios are commonly used in X-ray photometry to indicate spectral properties roughly. It is usually defined as the ratio of counts in two different wavebands. This definition, however, is problematic when the counts are very limited. Here we instead define hardness ratio using the λ\lambda parameter of Poisson processes, and develop an estimation method via Bayesian statistics. Our Monte Carlo simulations show the validity of our method. Based on this new definition, we can estimate the hydrogen column density for the photoelectric absorption of X-ray spectra in the case of low counting statistics.

Cite

@article{arxiv.astro-ph/0608579,
  title  = {Hardness Ratio Estimation in Low Counting X-ray Photometry},
  author = {Y. K. Jin and S. N. Zhang and J. F. Wu},
  journal= {arXiv preprint arXiv:astro-ph/0608579},
  year   = {2008}
}

Comments

12 pages, 4 figures, 1 table. Originally submitted on 29-03-2006, and accepted on 24-08-2006 for publication in The Astrophysical Journal

R2 v1 2026-07-22T09:11:56.598Z