The WEAVE-LOFAR Survey Article Swipe
D. J. B. Smith
,
P. N. Best
,
K. J. Duncan
,
N. A. Hatch
,
M. J. Jarvis
,
H. J. A. Röttgering
,
Chris Simpson
,
J. P. Stott
,
R. K. Cochrane
,
K. E. K. Coppin
,
H. Dannerbauer
,
T. A. Davis
,
J. E. Geach
,
C. L. Hale
,
M. J. Hardcastle
,
Peter Hatfield
,
R. C. W. Houghton
,
Natasha Maddox
,
Sean McGee
,
L. K. Morabito
,
D. Nisbet
,
M. Pandey-Pommier
,
I. Prandoni
,
Aayush Saxena
,
T. W. Shimwell
,
M. Tarr
,
I. van Bemmel
,
A. Verma
,
G. J. White
,
W. L. Williams
·
YOU?
·
· 2016
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.1611.02706
YOU?
·
· 2016
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.1611.02706
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 produce a data set of enormous legacy value. The radio frequency selection, combined with the high multiplex and throughput of the WEAVE spectrograph, make obtaining redshifts in this way very efficient, and we expect that the redshift success rate will approach 100 per cent at $z < 1$. This unprecedented spectroscopic sample - which will be complemented by an integral field component - will be transformational in key areas, including studying the star formation history of the Universe, the role of accretion and AGN-driven feedback, properties of the epoch of reionisation, cosmology, cluster haloes and relics, as well as the nature of radio galaxies and protoclusters. Each topic will be addressed in unprecedented detail, and with the most reliable source classifications and redshift information in existence.
Related Topics
Concepts
LOFAR
Redshift
Physics
Astrophysics
Integral field spectrograph
Spectrograph
Astronomy
Radio telescope
Galaxy
Telescope
Spectral line
Metadata
- Type
- article
- Language
- en
- OA Status
- green
- Cited By
- 16
- Related Works
- 20
- OpenAlex ID
- https://openalex.org/W2585901017
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W2585901017Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.48550/arxiv.1611.02706Digital Object Identifier
- Title
-
The WEAVE-LOFAR SurveyWork title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2016Year of publication
- Publication date
-
2016-11-08Full publication date if available
- Authors
-
D. J. B. Smith, P. N. Best, K. J. Duncan, N. A. Hatch, M. J. Jarvis, H. J. A. Röttgering, Chris Simpson, J. P. Stott, R. K. Cochrane, K. E. K. Coppin, H. Dannerbauer, T. A. Davis, J. E. Geach, C. L. Hale, M. J. Hardcastle, Peter Hatfield, R. C. W. Houghton, Natasha Maddox, Sean McGee, L. K. Morabito, D. Nisbet, M. Pandey-Pommier, I. Prandoni, Aayush Saxena, T. W. Shimwell, M. Tarr, I. van Bemmel, A. Verma, G. J. White, W. L. WilliamsList of authors in order
- Open access
-
YesWhether a free full text is available
- OA status
-
greenOpen access status per OpenAlex
- OA URL
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https://arxiv.org/pdf/1611.02706Direct OA link when available
- Concepts
-
LOFAR, Redshift, Physics, Astrophysics, Integral field spectrograph, Spectrograph, Astronomy, Radio telescope, Galaxy, Telescope, Spectral lineTop concepts (fields/topics) attached by OpenAlex
- Cited by
-
16Total citation count in OpenAlex
- Citations by year (recent)
-
2021: 3, 2020: 3, 2019: 2, 2018: 6, 2017: 2Per-year citation counts (last 5 years)
- Related works (count)
-
20Other works algorithmically related by OpenAlex
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