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Robert C. Nichol
Researcher at Institute of Cosmology and Gravitation, University of Portsmouth
Publications - 860
Citations - 176885
Robert C. Nichol is an academic researcher from Institute of Cosmology and Gravitation, University of Portsmouth. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 187, co-authored 851 publications receiving 162994 citations. Previous affiliations of Robert C. Nichol include University of Chicago & South East Physics Network.
Papers
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Galaxy Zoo: Blue Early-type Galaxies
Kevin Schawinski,Chris Lintott,Daniel Thomas,Marc Sarzi,Dan Andreescu,Steven P. Bamford,Sugata Kaviraj,Sadegh Khochfar,Kate Land,P. G. Murray,Robert C. Nichol,Jordan Raddick,Anze Slosar,Alexander S. Szalay,Jan Vandenberg,Sukyoung K. Yi +15 more
Journal Article
The spectral energy distribution of the proto-galaxy candidate MS1512-cB58.
D. M. Cole,D. E. Vanden Berk,Scott A. Severson,Robert C. Nichol,Jean M. Quashnock,M. C. Miller,D. Q. Lamb +6 more
Book ChapterDOI
Estimation of Correlations in Large Samples
István Szapudi,J. R. Bond,Stéphane Colombi,A. J. Connolly,Christopher R. Genovese,Andrew W. Moore,Robert C. Nichol,Simon Prunet,Dmitry Pogosyan,Jeff Schneider,Alexander S. Szalay,Larry Wasserman +11 more
Book ChapterDOI
Automated Classification Techniques for Large Spectroscopic Surveys
A. J. Connolly,Francisco J. Castander,Christopher R. Genovese,Eric J. Hilton,A. Merrelli,Andrew W. Moore,Robert C. Nichol,Jeff Schneider,Yehuda Snir,Alexander S. Szalay,István Szapudi,Larry Wasserman,Ching-Wa Yip +12 more
TL;DR: In this paper, a series of statistical techniques, ranging from Karhunen-Lo'eve transform to wavelet transforms, are applied to the spectra from the Sloan Digital Sky Survey in order to define a statistically robust and objective spectral classification scheme.
Posted Content
Measuring Dark Energy with the Wide-Field Multi-Object Spectrograph (WFMOS)
TL;DR: The Wide Field Multi-Object Spectrograph (WFMOS) as mentioned in this paper was proposed by the Subaru and Gemini communities to perform massive spectroscopic surveys of both distant galaxies and faint stars in our own Galaxy.