Oscillations of dark matter halos in galaxies
6 pages, 2 figures.
Flambaum, V. V., Samsonov, I. B.
openaire +2 more sources
Density profile of dark matter haloes and galaxies in the horizon–agn simulation: the impact of AGN feedback [PDF]
Sébastien Peirani +9 more
openalex +1 more source
Galaxy Galaxy Lensing as a Probe of Galaxy Dark Matter Halos
Gravitational lensing has now become a popular tool to measure the mass distribution of structures in the Universe on various scales. Here we focus on the study of galaxy's scale dark matter halos with galaxy-galaxy lensing techniques: observing the shapes of distant background galaxies which have been lensed by foreground galaxies allows us to map the
Limousin, M., Kneib, J-P., Natarajan, P.
openaire +2 more sources
Constructing a Galaxy Cluster Catalog in IllustrisTNG300 Using the Mulguisin Algorithm
We present a new simulated galaxy cluster catalog based on the IllustrisTNG simulation. We use the Mulguisin (MGS) algorithm to identify galaxy overdensities.
Lael Shin +4 more
doaj +1 more source
Compound Gravitational Lensing as a Probe of Dark Matter Substructure within Galaxy Halos [PDF]
R. B. Metcalf, Piero Madau
openalex +1 more source
Globular cluster ejection, infall, and the host dark matter halo of the Pegasus dwarf galaxy
Ryan Leaman +12 more
openalex +2 more sources
Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing clusters [PDF]
Taizo Okabe +8 more
openalex +1 more source
Origin and Full Characterization of the Secondary (Assembly) Halo Bias
The clustering of dark matter halos depends not only on their mass, the so-called primary bias, but also on their internal properties, the so-called secondary bias.
Eduard Salvador-Solé +2 more
doaj +1 more source
A forward modeling approach to analyzing galaxy clustering with SimBIG. [PDF]
Hahn C +9 more
europepmc +1 more source
SIDM Concerto: Compilation and Data Release of Self-interacting Dark Matter Zoom-in Simulations
We present SIDM Concerto: 14 cosmological zoom-in simulations in cold dark matter (CDM) and self-interacting dark matter (SIDM) models based on the Symphony and Milky Way-est suites.
Ethan O. Nadler +3 more
doaj +1 more source

