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20092026
most citedThe Baryon Oscillation Spectroscopic Survey of SDSS-III

2.1k citations · 10.4k across the 79 of their papers we have counts for

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Showing astro-ph.IMShow all

9 papers · 1 filter

astro-ph.IM2024★ 12 cited

The Wide-field Spectroscopic Telescope (WST) Science White Paper

Vincenzo Mainieri, Richard I. Anderson, Jarle Brinchmann +214

The Wide-field Spectroscopic Telescope (WST) is proposed as a new facility dedicated to the efficient delivery of spectroscopic surveys. This white paper summarises the initial con…

astro-ph.IM2019★ 14 cited

FOBOS: A Next-Generation Spectroscopic Facility at the W. M. Keck Observatory

K. Bundy, K. Westfall, N. MacDonald +38

High-multiplex and deep spectroscopic follow-up of upcoming panoramic deep-imaging surveys like LSST, Euclid, and WFIRST is a widely recognized and increasingly urgent necessity. N…

astro-ph.IM2019

SpecTel: A 10-12 meter class Spectroscopic Survey Telescope

Richard Ellis, Kyle Dawson, Joss Bland-Hawthorn +25

We recommend a conceptual design study for a spectroscopic facility in the southern hemisphere comprising a large diameter telescope, fiber system, and spectrographs collectively o…

astro-ph.IM2019★ 37 cited

The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

The MSE Science Team, Carine Babusiaux, Maria Bergemann +258

(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unvei…

astro-ph.IM2016★ 31 cited

The Detailed Science Case for the Maunakea Spectroscopic Explorer: the Composition and Dynamics of the Faint Universe

Alan McConnachie, Carine Babusiaux, Michael Balogh +173

MSE is an 11.25m aperture observatory with a 1.5 square degree field of view that will be fully dedicated to multi-object spectroscopy. More than 3200 fibres will feed spectrograph…

astro-ph.IM2014★ 54 cited

Model-based asymptotically optimal dispersion measure correction for pulsar timing

K. J. Lee, C. G. Bassa, G. H. Janssen +8

In order to reach the sensitivity required to detect gravitational waves, pulsar timing array experiments need to mitigate as much noise as possible in timing data. A dominant amou…