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Characterizing the astrometric precision limit for moving targets observed with digital-array detectors

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<i>Aims. <i/>We investigate the maximum astrometric precision that can be reached on moving targets observed with digital-sensor arrays, and provide an estimate for its ultimate lower limit based on the Cramér-Rao bound.<i>Methods. <i/>We extend previous work on one-dimensio...

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Bibliographic Details
Main Authors: Bouquillon, Sébastien (Author) , Altmann, Martin (Author)
Format: Article (Journal)
Language:English
Published: 03 October 2017
In: Astronomy and astrophysics
Year: 2017, Volume: 606
ISSN:1432-0746
DOI:10.1051/0004-6361/201628167
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201628167
Verlag, kostenfrei, Volltext: https://www.aanda.org/articles/aa/abs/2017/10/aa28167-16/aa28167-16.html
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Author Notes:S. Bouquillon, R.A. Mendez, M. Altmann, T. Carlucci, C. Barache, F. Taris, A.H. Andrei, and R. Smart
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Characterizing the astrometric precision limit for moving targets observed with digital-array detectors by Bouquillon, Sébastien (Author) , Altmann, Martin (Author) ,


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