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The WEAVE-LOFAR survey

Abstract:

In these proceedings we highlight the primary scientific goals and design of the WEAVE-LOFAR survey, which will use the new WEAVE spectrograph on the 4.2m William Herschel Telescope to provide the primary source of spectroscopic information for the LOFAR Surveys Key Science Project. Beginning in 2018, WEAVE-LOFAR will generate more than 10$^6$ R=5000 365-960 nm spectra of low-frequency selected radio sources, across three tiers designed to efficiently sample the redshift-luminosity plane, and...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Accepted Manuscript

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
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Publisher:
Société Francaise d’Astronomie et d’Astrophysique (SF2A) Publisher's website
Pages:
271-280
Publication date:
2016-12-01
Pubs id:
pubs:809885
URN:
uri:3d948d1e-9e54-4eda-835f-f1652e72cf5e
UUID:
uuid:3d948d1e-9e54-4eda-835f-f1652e72cf5e
Local pid:
pubs:809885

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