activity
19942009
most citedThe redshift dependence of the structure of massive LCDM halos

510 citations · 5.9k across the 44 of their papers we have counts for

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Showing 2008Show all

12 papers · 1 filter

astro-ph2008228 cited

Phase-space structure in the local dark matter distribution and its signature in direct detection experiments

Mark Vogelsberger, Amina Helmi, Volker Springel +6

We study predictions for dark matter phase-space structure near the Sun based on high-resolution simulations of six galaxy halos taken from the Aquarius Project. The local DM densi…

astro-ph2008154 cited

The environments of starburst and post-starburst galaxies at z=0.4-0.8

Bianca M. Poggianti, Alfonso Aragon-Salamanca, Dennis Zaritsky +16

Post-starburst (E+A or k+a) spectra, characterized by their exceptionally strong Balmer lines in absorption and the lack of emission lines, belong to galaxies in which the star for…

astro-ph200893 cited

Alignment between galaxies and large-scale structure

A. Faltenbacher, Cheng Li, Simon D. M. White +3

Based on the Sloan Digital Sky Survey DR6 (SDSS) and Millennium Simulation (MS) we investigate the alignment between galaxies and large-scale structure. For this purpose we develop…

astro-ph200832 cited

Dark Matter Caustics

Simon D. M. White, Mark Vogelsberger

Caustics are a generic feature of the nonlinear growth of structure in the dark matter distribution. If the dark matter were absolutely cold, its mass density would diverge at caus…

astro-ph2008111 cited

Halo masses for optically-selected and for radio-loud AGN from clustering and galaxy-galaxy lensing

Rachel Mandelbaum, Cheng Li, Guinevere Kauffmann +1

We compute two-point correlation functions and measure the shear signal due to galaxy-galaxy lensing for 80,000 optically identified and 5,700 radio-loud AGN from Data Release 4 (D…

astro-ph2008155 cited

The relation between star formation, morphology and local density in high redshift clusters and groups

Bianca M. Poggianti, Vandana Desai, Rose Finn +17

We investigate how the [OII] properties and the morphologies of galaxies in clusters and groups at z=0.4-0.8 depend on projected local galaxy density, and compare with the field at…