Large-scale structure of the Universe and cosmological perturbation theory
F Bernardeau, S Colombi, E Gaztanaga… - Physics reports, 2002 - Elsevier
We review the formalism and applications of non-linear perturbation theory (PT) to
understanding the large-scale structure of the Universe. We first discuss the dynamics of …
understanding the large-scale structure of the Universe. We first discuss the dynamics of …
The baryon oscillation spectroscopic survey of SDSS-III
KS Dawson, DJ Schlegel, CP Ahn… - The Astronomical …, 2012 - iopscience.iop.org
ABSTRACT The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure
the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger …
the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger …
The multi-object, fiber-fed spectrographs for the sloan digital sky survey and the baryon oscillation spectroscopic survey
SA Smee, JE Gunn, A Uomoto, N Roe… - The Astronomical …, 2013 - iopscience.iop.org
We present the design and performance of the multi-object fiber spectrographs for the Sloan
Digital Sky Survey (SDSS) and their upgrade for the Baryon Oscillation Spectroscopic …
Digital Sky Survey (SDSS) and their upgrade for the Baryon Oscillation Spectroscopic …
The nustar extragalactic surveys: overview and catalog from the COSMOS field
F Civano, RC Hickox, S Puccetti… - The Astrophysical …, 2015 - iopscience.iop.org
To provide the census of the sources contributing to the X-ray background peak above 10
keV, Nuclear Spectroscopic Telescope Array (NuSTAR) is performing extragalactic surveys …
keV, Nuclear Spectroscopic Telescope Array (NuSTAR) is performing extragalactic surveys …
Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release
Abstract The Galaxy and Mass Assembly (GAMA) survey has been operating since 2008
February on the 3.9-m Anglo-Australian Telescope using the AAOmega fibre-fed …
February on the 3.9-m Anglo-Australian Telescope using the AAOmega fibre-fed …
Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
Abstract The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary
spectroscopic surveys of low redshift galaxies. Covering an area of∼ 286 deg2 (split among …
spectroscopic surveys of low redshift galaxies. Covering an area of∼ 286 deg2 (split among …
The 2MASS Redshift Survey—description and data release
JP Huchra, LM Macri, KL Masters… - The Astrophysical …, 2012 - iopscience.iop.org
We present the results of the 2MASS Redshift Survey (2MRS), a ten-year project to map the
full three-dimensional distribution of galaxies in the nearby universe. The Two Micron All Sky …
full three-dimensional distribution of galaxies in the nearby universe. The Two Micron All Sky …
Spectroscopic target selection in the Sloan Digital Sky Survey: the main galaxy sample
MA Strauss, DH Weinberg, RH Lupton… - The Astronomical …, 2002 - iopscience.iop.org
We describe the algorithm that selects the main sample of galaxies for spectroscopy in the
Sloan Digital Sky Survey (SDSS) from the photometric data obtained by the imaging survey …
Sloan Digital Sky Survey (SDSS) from the photometric data obtained by the imaging survey …
The massive relic galaxy NGC 1277 is dark matter deficient-From dynamical models of integral-field stellar kinematics out to five effective radii
According to the Λ cold dark matter (ΛCDM) cosmology, present-day galaxies with stellar
masses M⋆> 10 11 M⊙ should contain a sizable fraction of dark matter within their stellar …
masses M⋆> 10 11 M⊙ should contain a sizable fraction of dark matter within their stellar …
The three-dimensional power spectrum of galaxies from the sloan digital sky survey
We measure the large-scale real-space power spectrum P (k) by using a sample of 205,443
galaxies from the Sloan Digital Sky Survey, covering 2417 effective square degrees with …
galaxies from the Sloan Digital Sky Survey, covering 2417 effective square degrees with …