Unbiased clustering estimates with the DESI fibre assignment

The Emission Line Galaxy survey made by the Dark Energy Spectroscopic Instrument (DESI) survey will be created from five passes of the instrument on the sky. On each pass, the constrained mobility of the ends of the fibres in the DESI focal plane means that the angular distribution of targets that c...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2018-12, Vol.481 (2), p.2338-2348
Hauptverfasser: Bianchi, Davide, Burden, Angela, Percival, Will J, Brooks, David, Cahn, Robert N, Forero-Romero, Jaime E, Levi, Michael, Ross, Ashley J, Tarle, Gregory
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Sprache:eng
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