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The UKIRT Infrared Deep Sky Survey (UKIDSS)

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TLDR
The final version published in MNRAS August 2007 included significant revisions including significant revisions to the original version April 2006.
Abstract
Final published version including significant revisions. Twenty four pages, fourteen figures. Original version April 2006; final version published in MNRAS August 2007

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Sdss-iii: massive spectroscopic surveys of the distant universe, the milky way, and extra-solar planetary systems

Daniel J. Eisenstein, +263 more
TL;DR: SDSS-III as mentioned in this paper 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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CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey

Norman A. Grogin, +108 more
TL;DR: The Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey (CANDELS) as discussed by the authors was designed to document the first third of galactic evolution, from z approx. 8 - 1.5 to test their accuracy as standard candles for cosmology.
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Candels: The cosmic assembly near-infrared deep extragalactic legacy survey - The hubble space telescope observations, imaging data products, and mosaics

Anton M. Koekemoer, +124 more
TL;DR: In this paper, the authors describe the Hubble Space Telescope imaging data products and data reduction procedures for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS).
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The baryon oscillation spectroscopic survey of sdss-iii

Kyle S. Dawson, +184 more
TL;DR: The Baryon Oscillation Spectroscopic Survey (BOSS) as discussed by the authors was designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the combined efforts of all previous spectroscopic surveys of large-scale structure.
References
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Journal ArticleDOI

A Wide Area Survey for High-Redshift Massive Galaxies. I. Number Counts and Clustering of BzKs and EROs

TL;DR: In this article, the results of a deep, wide area, optical and near-IR survey of massive high-redshift galaxies are presented, with the properties of K-band-selected galaxies, identified from a total area of ~920 arcmin2 to KVega = 19.
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Automatic Analysis of Crowded Fields

TL;DR: There are many important 2D data reduction problems in Astronomy that are not amenable to conventional automatic analysis as mentioned in this paper, typically these problem areas arise in fields where the number density of images is high and where the local sky background may vary rapidly.
Journal ArticleDOI

CCD photometry of Abell clusters. I - Magnitudes and redshifts for 84 brightest cluster galaxies

TL;DR: In this article, the luminosity of the brightest cluster galaxy varies with cluster parameters in a sample of 84 Abell clusters of moderate redshift and of richness classes in the zero-to-5 range.
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