Clustering in real space and in redshift space
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About: This article is published in Monthly Notices of the Royal Astronomical Society. The article was published on 01 Jul 1987. and is currently open access. The article focuses on the topics: Redshift survey & 2dF Galaxy Redshift Survey.
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Citations
Optimising the measurement of relativistic distortions in large-scale structure
TL;DR: In this paper, an optimal estimator to measure the relativistic dipole with multiple populations of galaxies with different luminosities or colours has been proposed to increase the signal-to-noise of the dipole by up to 35 percent.
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Nature or nurture? Clues from the distribution of specific star formation rates in SDSS galaxies
J. Casado,J. Casado,Yago Ascasibar,Yago Ascasibar,M. Gavilán,M. Gavilán,Roberto Terlevich,Elena Terlevich,Carlos Hoyos,Carlos Hoyos,A. I. Díaz,A. I. Díaz +11 more
TL;DR: In this article, the authors investigated the main mechanism(s) that regulate specific star formation rate (SSFR) in nearby galaxies, cross-correlating two proxies of this quantity with other physical properties (mass, metallicity, environment, morphology, and the presence of close companions) in a sample of $\sim82500$ galaxies extracted from the Sloan Digital Sky Survey (SDSS).
40
Weak Lensing Mass Measurements of Substructures in COMA Cluster with Subaru/Suprime-Cam
TL;DR: The contribution of background large-scale structure (LSS) on the projected mass distributions using SDSS multi-bands and photometric data, under the assumption of mass-to-light ratio for field galaxies, was quantified in this paper.
Tests of General Relativity on Astrophysical Scales
TL;DR: In this article, the main tests of general relativity focusing on the large scale structure and more particularly weak lensing are reviewed, and the complementarity with other tests (including those on Solar system scales and the equivalence principle) is discussed.
40
Line intensity mapping with [CII] and CO(1-0) as probes of primordial non-Gaussianity
TL;DR: In this article, the authors explore the potential of wide field [CII] and CO intensity mapping surveys in constraining primordial non-Gaussianity (PNG) of the local shape, which induces a distinct, scale-dependent correction to the line bias.
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References
The large-scale structure of the universe
P. J. E. Peebles
- 01 Jan 1980
TL;DR: Peebles as discussed by the authors argues that the evolution of the early universe went from a nearly uniform initial state to a progressively more irregular and clumpy universe, based on the largest known structures of the universe.
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