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Estimation of the Errors Involved in the Intensity Measurement of Low S/N Ratio Emission Lines

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New Developments in Array Technology and Applications

Part of the book series: International Astronomical Union / Union Astronomique Internationale ((IAUS,volume 167))

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Abstract

We present a detailed analysis on the extent of the errors in the intensity measurements of low signal-to-noise narrow emission lines. Our first goal is to determine a model for the probability distribution function (p.d.f.) associated with the measured intensities of a line characterized by its signal-to-noise ratio. Our final purpose is to provide an error domain: - for the measured signal-to-noise ratio of an observed line; - for the ratio of two lines in terms of their signal-to-noise ratios, and eventually (with the knowledge of the noise energy) to get errors on the corresponding intensities and intensity ratios.

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© 1995 Springer Science+Business Media Dordrecht

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Rola, C., Pelat, D. (1995). Estimation of the Errors Involved in the Intensity Measurement of Low S/N Ratio Emission Lines. In: Philip, A.G.D., Janes, K.A., Upgren, A.R. (eds) New Developments in Array Technology and Applications. International Astronomical Union / Union Astronomique Internationale, vol 167. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0383-1_63

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  • DOI: https://doi.org/10.1007/978-94-011-0383-1_63

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-0-7923-3640-2

  • Online ISBN: 978-94-011-0383-1

  • eBook Packages: Springer Book Archive

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