Xiao 2009 加权估计长暴的红移
用多种方法估计红移, 然后给每个方法一个权重, 得到加权平均值. (不觉得这样就可以得到更好的估计值)
・ Find Similar Abstracts (with default settings below) Title: Estimating Redshifts for Long Gamma-Ray Bursts Authors:
Xiao, Limin; Schaefer, Bradley E. Publication: eprint arXiv:0910.4945 Publication Date:
10/2009 Origin: ARXIV Keywords: Astrophysics - Cosmology and Extragalactic Astrophysics Comment: The Astrophysical Journal accepted Bibliographic Code: 2009arXiv0910.4945X Abstract
We are constructing a program to estimate the redshifts for GRBs from the original Swift light curves and spectra, aiming to get redshifts for the Swift bursts \textit{without} spectroscopic or photometric redshifts. We derive the luminosity indicators from the light curves and spectra of each burst, including the lag time between low and high photon energy light curves, the variability of the light curve, the peak energy of the spectrum, the number of peaks in the light curve, and the minimum rise time of the peaks. These luminosity indicators can each be related directly to the luminosity, and we combine their independent luminosities into one weighted average. Then with our combined luminosity value, the observed burst peak brightness, and the concordance redshift-distance relation, we can derive the redshift for each burst. In this paper, we test the accuracy of our method on 107 bursts with known spectroscopic redshift. The reduced $\chi^2$ of our best redshifts ($z_{best}$) compared with known spectroscopic redshifts ($z_{spec}$) is 0.86, and the average value of $log_{10}(z_{best}/z_{spec})$ is 0.01, with this indicating that our error bars are good and our estimates are not biased. The RMS scatter of $log_{10}(z_{best}/z_{spec})$ is 0.26. For Swift bursts measured over a relatively narrow energy band, the uncertainty in determining the peak energy is one of the main restrictions on our accuracy. Although the accuracy of our $z_{best}$ values are not as good as that of spectroscopic redshifts, it is very useful for demographic studies, as our sample is nearly complete and the redshifts do not have the severe selection effects associated with optical spectroscopy.
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