activity
19942004
collaborators

17 papers

astro-ph2004

Rotation Velocities of Two Low Luminosity Field Galaxies

James Pizagno, Michael R. Blanton, David H. Weinberg +2

We present H-alpha rotation curves of two low luminosity field galaxies with r-band absolute magnitudes M_r=-13.9^{+0.8}_{-0.5} and M_r=-14.7^{+0.3}_{-0.2} (for h=0.7; the large er…

astro-ph2002

Studying Structure Formation with the Sloan Digital Sky Survey

David H. Weinberg

I review recent SDSS results related to galaxies and large scale structure, including: (1) discovery of coherent, unbound structures in the stellar halo, (2) demonstration that Pal…

astro-ph2001

Sub-mm Galaxies in Cosmological Simulations

Mark A. Fardal, Neal Katz, David H. Weinberg +2

We study the predicted sub-mm emission from massive galaxies in a Lambda-CDM universe, using hydrodynamic cosmological simulations. Assuming that most of the emission from newly fo…

astro-ph1999

Evolution of Clustering and Bias in a Lambda-CDM Universe

Romeel Davé, Lars Hernquist, Neal Katz +1

We determine the evolution from of the galaxy and mass correlation functions and bias factor in a Mpc CDM hydrodynamic simulation with kpc resolut…

astro-ph1999

The Nature of Lyman Break Galaxies in Cosmological Hydrodynamic Simulations

Romeel Davé, Jeffrey P. Gardner, Lars Hernquist +2

What type of objects are being detected as "Lyman break galaxies"? Are they predominantly the most massive galaxies at that epoch, or are many of them smaller galaxies un…

astro-ph1999

What is Beta?

Andreas A. Berlind, Vijay K. Narayanan, David H. Weinberg

Measurements of the cosmological density parameter (Omega) using techniques that exploit the gravity-induced motions of galaxies yield, in linear perturbation theory, the degenerat…