The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample [PDF]
, 2016 We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III.
S. Alam +88 more
semanticscholar +1 more source
Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies [PDF]
, 2013 Supermassive black holes (BHs) have been found in 85 galaxies by dynamical modeling of spatially resolved kinematics. The Hubble Space Telescope revolutionized BH research by advancing the subject from its proof-of-concept phase into quantitative studies
J. Kormendy, L. Ho
semanticscholar +1 more source
Quenched Galaxies in Clusters of Galaxies and Their Outskirts [PDF]
Astrophysical Bulletin, 2020 Based on the SDSS data, the properties of galaxies with quenched star formation (QGs) within the "splashback"-radius of galaxy clusters $R_{\rm sp}$ and beyond it have been studied.
Kopylova, Flera G. +1 more
openaire +2 more sources
The Origin of the Mass-Metallicity Relation: Insights from 53,000 Star-forming Galaxies in the Sloan Digital Sky Survey [PDF]
, 2004 We utilize Sloan Digital Sky Survey imaging and spectroscopy of ~53,000 star-forming galaxies at z ~ 0.1 to study the relation between stellar mass and gas-phase metallicity.
C. Tremonti +11 more
semanticscholar +1 more source
Accretion of galaxy groups into galaxy clusters [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT We study the role of group infall in the assembly and dynamics of galaxy clusters in ΛCDM. We select 10 clusters with virial mass M200 ∼ 1014 $\rm M_\odot$ from the cosmological hydrodynamical simulation Illustris and follow their galaxies with stellar mass M⋆ ≥ 1.5 × 108 $\rm M_\odot$.
José A Benavides +2 more
openaire +3 more sources
Effects of Higher Order Retarded Gravity
Universe, 2021 In a recent paper, we have a shown that the flattening of galactic rotation curves can be explained by retardation. However, this will rely on a temporal change of galactic mass.
Asher Yahalom
doaj +1 more source
CFHTLenS: higher order galaxy–mass correlations probed by galaxy–galaxy–galaxy lensing [PDF]
Monthly Notices of the Royal Astronomical Society, 2013 25 pages, 15 figures, accepted by ...
Simon, P. +18 more
openaire +4 more sources
Acknowledgement to Reviewers of Galaxies in 2016
Galaxies, 2017 The editors of Galaxies would like to express their sincere gratitude to the following reviewers for assessing manuscripts in 2016.[...]
Galaxies Editorial Office
doaj +1 more source
Acknowledgement to Reviewers of Galaxies in 2017
Galaxies, 2018 Peer review is an essential part in the publication process, ensuring that Galaxies maintains high quality standards for its published papers [...]
Galaxies Editorial Office
doaj +1 more source
The physical properties of star-forming galaxies in the low-redshift universe [PDF]
, 2003 We present a comprehensive study of the physical properties of ∼ 10 5 galaxies with measurable star formation in the Sloan Digital Sky Survey (SDSS). By comparing physical information extracted from the emission lines with continuum properties, we build ...
J. Brinchmann +8 more
semanticscholar +1 more source