Chao’s lower bound estimator and the size of the Pleiades
Chao’s lower bound estimator and the size of the Pleiades
In this note we would like to point out that the lower bound estimator of the frequency of hidden units in a target population, developed by Chao in ecology, was developed independently in astro-physics and has been used to estimate the size of flare stars in the Pleiades.
Chao’s lower bound estimator, Dark number estimation in astro-physics, Estimating the number of flare stars
171-173
Bohning, Dankmar
1df635d4-e3dc-44d0-b61d-5fd11f6434e1
1 March 2020
Bohning, Dankmar
1df635d4-e3dc-44d0-b61d-5fd11f6434e1
Bohning, Dankmar
(2020)
Chao’s lower bound estimator and the size of the Pleiades.
Environmental and Ecological Statistics, 27 (1), .
(doi:10.1007/s10651-020-00440-w).
Abstract
In this note we would like to point out that the lower bound estimator of the frequency of hidden units in a target population, developed by Chao in ecology, was developed independently in astro-physics and has been used to estimate the size of flare stars in the Pleiades.
Text
Chao_Astronom
- Accepted Manuscript
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Accepted/In Press date: 10 January 2020
e-pub ahead of print date: 15 February 2020
Published date: 1 March 2020
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© 2020, Springer Science+Business Media, LLC, part of Springer Nature.
Keywords:
Chao’s lower bound estimator, Dark number estimation in astro-physics, Estimating the number of flare stars
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Local EPrints ID: 437049
URI: http://eprints.soton.ac.uk/id/eprint/437049
ISSN: 1352-8505
PURE UUID: 77d3c321-c9a3-4029-bc03-d28c7525cd19
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Date deposited: 16 Jan 2020 17:30
Last modified: 06 Jun 2024 04:19
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