Cosmological constraints from the clustering of the Sloan Digital Sky Survey DR7 luminous red galaxies [PDF]
We present the power spectrum of the reconstructed halo density field derived from a sample of luminous red galaxies (LRGs) from the Sloan Digital Sky Survey (SDSS) Seventh Data Release (DR7).
Weinberg, D. H. +63 more
core +1 more source
A Time-symmetric Hubble-like Law: Light Rays Grazing Randomly Moving Galaxies Show Distance-Proportional Redshift [PDF]
A new class of dissipative structures is proposed that live in real space rather than phase space. A light ray passing through a soup of randomly moving gravitating masses is a case in point. It suffers a “dynamic path elongation” since the random pushes and pulls have a greater probability of increasing than decreasing its path length.
O. E. Rössler, D. Fröhlich, N. Kleiner
openaire +1 more source
The Lens Parallax Method: Determining Redshifts of Faint Blue Galaxies through Gravitational Lensing [PDF]
We propose a new technique, which we call the lens parallax method, to determine simultaneously the redshift distribution of the faint blue galaxies and the mass distributions of foreground clusters of galaxies.
Narayan, Ramesh, Bartelmann, Matthias
core +1 more source
Direct comparison of observed magnitude–redshift relations in complete galaxy samples with systematic predictions of alternative redshift–distance laws [PDF]
La magnitude apparente moyenne directement observee comme fonction du redshift dans chacun des echantillons complets de galaxies est comparee aux predictions des lois en puissance hypothetiques distance-redshift d'un point de vue ...
openaire +1 more source
The scaling relation of early-type galaxies in clusters II. Spectroscopic data for galaxies in eight nearby clusters [PDF]
Galaxies: elliptical and lenticulars, cD, distances and redshifts - clusters: general Udgivelsesdato ...
D. Bettoni +9 more
core +1 more source
Searching for Highly Magnified Stars at Cosmological Distances: Discovery of a Redshift 0.94 Blue Supergiant in Archival Images of the Galaxy Cluster MACS J0416.1-2403 [PDF]
Abstract Individual highly magnified stars have been recently discovered at lookback times of more than half the age of the universe, in lensed galaxies that straddle the critical curves of massive galaxy clusters. Having established their detectability, it is now important to carry out systematic searches for them in order to establish ...
Wenlei Chen +14 more
openaire +5 more sources
Measuring the distance-redshift relation with the cross-correlation of gravitational wave standard sirens and galaxies [PDF]
Gravitational waves from inspiraling compact binaries are known to be an excellent absolute distance indicator, yet it is unclear whether electromagnetic counterparts of these events are securely identified for measuring their redshifts, especially in the case of black hole-black hole mergers such as the one recently observed with the Advanced LIGO. We
openaire +2 more sources
The THESEUS Space Mission and the Infrared Telescope Calibration Unit
ABSTRACT The Transient High‐Energy Sky and Early Universe Surveyor (THESEUS) is an ESA M7 mission concept currently in Phase A, designed to exploit gamma‐ray bursts to probe the early Universe while advancing multi‐messenger and time‐domain astrophysics. To achieve its ambitious goals, THESEUS will combine wide‐band x‐ray and gamma‐ray monitors with an
András Péter Joó +9 more
wiley +1 more source
Mapping the dynamics, star-formation rates, and chemical properties of galaxies with integral field spectroscopy [PDF]
Major advances in the development of instruments for eight and ten meter class telescopes are revolutionising our understanding of galaxy formation. In particular, Integral Field Spectrographs (which produce a three dimensional {x, y, velocity) map of a ...
Swinbank, Anthony Mark +1 more
core
The many flavours of photometric redshifts [PDF]
International audienceSince more than 70 years ago, the colours of galaxies derived from flux measurements at different wavelengths have been used to estimate their cosmological distances.
Olivier Ilbert +8 more
core +1 more source

