The connection between galaxies and their dark matter halos
RH Wechsler, JL Tinker - Annual Review of Astronomy and …, 2018 - annualreviews.org
In our modern understanding of galaxy formation, every galaxy forms within a dark matter
halo. The formation and growth of galaxies over time is connected to the growth of the halos …
halo. The formation and growth of galaxies over time is connected to the growth of the halos …
Dark energy two decades after: observables, probes, consistency tests
D Huterer, DL Shafer - Reports on Progress in Physics, 2017 - iopscience.iop.org
The discovery of the accelerating universe in the late 1990s was a watershed moment in
modern cosmology, as it indicated the presence of a fundamentally new, dominant …
modern cosmology, as it indicated the presence of a fundamentally new, dominant …
The atacama cosmology telescope: A catalog of> 4000 Sunyaev–Zel'dovich galaxy clusters
We present a catalog of 4195 optically confirmed Sunyaev–Zel'dovich (SZ) selected galaxy
clusters detected with signal-to-noise ratio> 4 in 13,211 deg 2 of sky surveyed by the …
clusters detected with signal-to-noise ratio> 4 in 13,211 deg 2 of sky surveyed by the …
Overview of the DESI legacy imaging surveys
Abstract The DESI Legacy Imaging Surveys (http://legacysurvey. org/) are a combination of
three public projects (the Dark Energy Camera Legacy Survey, the Beijing–Arizona Sky …
three public projects (the Dark Energy Camera Legacy Survey, the Beijing–Arizona Sky …
The MillenniumTNG Project: the hydrodynamical full physics simulation and a first look at its galaxy clusters
R Pakmor, V Springel, JP Coles, T Guillet… - Monthly Notices of …, 2023 - academic.oup.com
Cosmological simulations are an important theoretical pillar for understanding non-linear
structure formation in our Universe and for relating it to observations on large scales. In …
structure formation in our Universe and for relating it to observations on large scales. In …
Dark Energy Survey Year 1 Results: Cosmological constraints from cluster abundances and weak lensing
We perform a joint analysis of the counts and weak lensing signal of redMaPPer clusters
selected from the Dark Energy Survey (DES) Year 1 dataset. Our analysis uses the same …
selected from the Dark Energy Survey (DES) Year 1 dataset. Our analysis uses the same …
The eROSITA Final Equatorial-Depth Survey (eFEDS)-Catalog of galaxy clusters and groups
Aims. The eROSITA Final Equatorial-Depth Survey has been carried out during the
performance verification phase of the Spectrum-Roentgen-Gamma/eROSITA telescope and …
performance verification phase of the Spectrum-Roentgen-Gamma/eROSITA telescope and …
The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
The total mass of a galaxy cluster is one of its most fundamental properties. Together with
the redshift, the mass links observation and theory, allowing us to use the cluster population …
the redshift, the mass links observation and theory, allowing us to use the cluster population …
Probing Galactic haloes with fast radio bursts
JX Prochaska, Y Zheng - Monthly Notices of the Royal …, 2019 - academic.oup.com
Abstract The precise localization (< 1 arcsec) of multiple fast radio bursts (FRBs) to> 0.1
galaxies has confirmed that the dispersion measures (DMs) of these enigmatic sources …
galaxies has confirmed that the dispersion measures (DMs) of these enigmatic sources …
The SPTPoL extended cluster survey
We describe the observations and resultant galaxy cluster catalog from the 2770 deg 2
SPTpol Extended Cluster Survey (SPT-ECS). Clusters are identified via the Sunyaev …
SPTpol Extended Cluster Survey (SPT-ECS). Clusters are identified via the Sunyaev …