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Francisco S. Kitaura

Researcher at University of La Laguna

Publications -  27
Citations -  9547

Francisco S. Kitaura is an academic researcher from University of La Laguna. The author has contributed to research in topics: Redshift & Galaxy. The author has an hindex of 19, co-authored 27 publications receiving 7976 citations. Previous affiliations of Francisco S. Kitaura include Leibniz Institute for Astrophysics Potsdam & University of California, Berkeley.

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The eleventh and twelfth data releases of the Sloan Digital Sky Survey: final data from SDSS-III

Shadab Alam, +363 more
TL;DR: The third generation of the Sloan Digital Sky Survey (SDSS-III) took data from 2008 to 2014 using the original SDSS wide-field imager, the original and an upgraded multi-object fiber-fed optical spectrograph, a new near-infrared high-resolution spectrogram, and a novel optical interferometer.
Journal ArticleDOI

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Shadab Alam, +90 more
TL;DR: In this article, the authors present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III.
Journal ArticleDOI

The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

Shadab Alam, +273 more
TL;DR: The third generation of the Sloan Digital Sky Survey (SDSS-III) took data from 2008 to 2014 using the original SDSS wide-field imager, the original and an upgraded multi-object fiber-fed optical spectrograph, a new near-infrared high-resolution spectrogram, and a novel optical interferometer as discussed by the authors.
Journal ArticleDOI

Cosmological implications of baryon acoustic oscillation measurements

Éric Aubourg, +94 more
- 14 Dec 2015 - 
TL;DR: This paper derived constraints on cosmological parameters and tests of dark energy models from the combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave background (CMB) data and a recent reanalysis of Type Ia supernova (SN) data.