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Heather Campbell

Researcher at University of Cambridge

Publications -  48
Citations -  13966

Heather Campbell is an academic researcher from University of Cambridge. The author has contributed to research in topics: Supernova & Redshift. The author has an hindex of 29, co-authored 48 publications receiving 11996 citations. Previous affiliations of Heather Campbell include Institute of Cosmology and Gravitation, University of Portsmouth & University of Sussex.

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The Gaia mission

T. Prusti, +624 more
TL;DR: Gaia as discussed by the authors is a cornerstone mission in the science programme of the European Space Agency (ESA). The spacecraft construction was approved in 2006, following a study in which the original interferometric concept was changed to a direct-imaging approach.
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SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems

Daniel J. Eisenstein, +239 more
TL;DR: SDSS-III as discussed by the authors is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the history and structure of the Milky Way, and the population of giant planets around other stars.
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Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples

Marc Betoule, +72 more
TL;DR: In this article, the authors presented cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observations obtained by the SDSS-II and SNLS collaborations.
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The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III

Hiroaki Aihara, +179 more
TL;DR: The first data release of SDSS-III (and the eighth counting from the beginning of the Sloan Digital Sky Survey (SDSS) is described in this paper, which includes five-band imaging of roughly 5200 deg^2 in the Southern Galactic Cap.
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Galaxy Zoo: Passive Red Spirals .

TL;DR: In this paper, the spectroscopic properties and environments of red (or passive) spiral galaxies found by the Galaxy Zoo project were studied. But there are no obvious correlations between red spiral properties and environment suggesting that environment alone is not sufficient to determine whether a galaxy will become a red spiral.