Astrophysics with the laser interferometer space antenna
P Amaro-Seoane, J Andrews, M Arca Sedda… - Living Reviews in …, 2023 - Springer
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
[HTML][HTML] The cosmological constant
SM Carroll - Living reviews in relativity, 2001 - Springer
This is a review of the physics and cosmology of the cosmological constant. Focusing on
recent developments, I present a pedagogical overview of cosmology in the presence of a …
recent developments, I present a pedagogical overview of cosmology in the presence of a …
Planck 2013 results. XX. Cosmology from Sunyaev–Zeldovich cluster counts
PAR Ade, N Aghanim, C Armitage-Caplan… - Astronomy & …, 2014 - aanda.org
We present constraints on cosmological parameters using number counts as a function of
redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The …
redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The …
Measurements of Ω and Λ from 42 high-redshift supernovae
S Perlmutter, G Aldering, G Goldhaber… - The Astrophysical …, 1999 - iopscience.iop.org
We report measurements of the mass density, Ω $\mathstrut {_ {M}} $, and cosmological-
constant energy density, Ω $\mathstrut {_ {{\Lambda}}} $, of the universe based on the …
constant energy density, Ω $\mathstrut {_ {{\Lambda}}} $, of the universe based on the …
Observational evidence from supernovae for an accelerating universe and a cosmological constant
AG Riess, AV Filippenko, P Challis… - The astronomical …, 1998 - iopscience.iop.org
We present spectral and photometric observations of 10 Type Ia supernovae (SNe Ia) in the
redshift range 0.16≤ z≤ 0.62. The luminosity distances of these objects are determined by …
redshift range 0.16≤ z≤ 0.62. The luminosity distances of these objects are determined by …
[HTML][HTML] The cosmological constant
SM Carroll, WH Press, EL Turner - … . Vol. 30 (A93-25826 09-90) …, 1992 - adsabs.harvard.edu
The cosmological constant ADS Classic is now deprecated. It will be completely retired in
October 2019. This page will automatically redirect to the new ADS interface at that point …
October 2019. This page will automatically redirect to the new ADS interface at that point …
Constraints on the relationship between stellar mass and halo mass at low and high redshift
BP Moster, RS Somerville, C Maulbetsch… - The Astrophysical …, 2010 - iopscience.iop.org
We use a statistical approach to determine the relationship between the stellar masses of
galaxies and the masses of the dark matter halos in which they reside. We obtain a …
galaxies and the masses of the dark matter halos in which they reside. We obtain a …
The cosmic baryon budget
M Fukugita, CJ Hogan, PJE Peebles - The Astrophysical Journal, 1998 - iopscience.iop.org
We present an estimate of the global budget of baryons in all states, with conservative
estimates of the uncertainties, based on all relevant information we have been able to …
estimates of the uncertainties, based on all relevant information we have been able to …
Analytic model for galaxy and dark matter clustering
U Seljak - Monthly Notices of the Royal Astronomical Society, 2000 - academic.oup.com
We investigate an analytic model to compute the non-linear power spectrum of dark matter,
galaxies and their cross-correlation. The model is based on Press-Schechter haloes, which …
galaxies and their cross-correlation. The model is based on Press-Schechter haloes, which …
Galaxy groups in the SDSS DR4. I. The catalog and basic properties
X Yang, HJ Mo, FC Van den Bosch… - The Astrophysical …, 2007 - iopscience.iop.org
We use a modified version of the halo-based group finder developed by Yang et al. to select
galaxy groups from the Sloan Digital Sky Survey (SDSS DR4). In the first step, a combination …
galaxy groups from the Sloan Digital Sky Survey (SDSS DR4). In the first step, a combination …