A blind H i mass function from the Arecibo Ultra-Deep Survey (AUDS) | Zendy

L. Hoppmann | Zendy; L. StaveleySmith | Zendy; W. Freudling | Zendy; M. A. Zwaan | Zendy; Robert Minchin | Zendy; M. R. Calabretta | Zendy

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A blind H i mass function from the Arecibo Ultra-Deep Survey (AUDS)

Author(s) -

L. Hoppmann,

L. StaveleySmith,

W. Freudling,

M. A. Zwaan,

Robert Minchin,

M. R. Calabretta

Publication year - 2015

Publication title -

monthly notices of the royal astronomical society

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.058

H-Index - 383

eISSN - 1365-8711

pISSN - 0035-8711

DOI - 10.1093/mnras/stv1084

Subject(s) - physics , redshift , galaxy , cosmic variance , astrophysics , omega , homogeneous , universe , sensitivity (control systems) , quantum mechanics , electronic engineering , engineering , thermodynamics

The Arecibo Ultra-Deep Survey (AUDS) combines the unique sensitivity of the telescope with the wide field of the Arecibo L-band Feed Array (ALFA) to directly detect 21 cm ${\rm H\,{\small i}}$ emission from galaxies at distances beyond the local Universe bounded by the lower frequency limit of ALFA (z = 0.16). AUDS has collected 700 h of integration time in two fields with a combined area of 1.35 ...

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