output
19922026
most citedAstropy: A Community Python Package for Astronomy

14.6k citations

Showing 2002 · astro-phShow all

97 papers · 2 filters

astro-ph2002★ 19 cited

Completeness of USNO-B for High Proper-Motion Stars

Andrew Gould

I test the completeness of USNO-B detections of high proper-motion (mu>0.18"/yr) stars and the accuracy of its measurements by comparing them to the revised NLTT (rNLTT) catalog of…

astro-ph2002★ 154 cited

Circumnuclear Dust in Nearby Active and Inactive Galaxies. I. Data

Paul Martini, Michael W. Regan, John S. Mulchaey +1

The detailed morphology of the interstellar medium (ISM) in the central kiloparsec of galaxies is controlled by pressure and gravitation. The combination of these forces shapes bot…

astro-ph2002★ 2 cited

Lyman Alpha Absorber Correlations and the Bias of the Lyman Alpha Forest

Romeel Davé, Neal Katz, David H. Weinberg

Lyman alpha absorber correlations contain information about the underlying density distribution associated with a particular class of absorbers. As such, they provide an opportunit…

astro-ph2002★ 186 cited

Circumnuclear Dust in Nearby Active and Inactive Galaxies. II. Bars, Nuclear Spirals, and the Fueling of Active Galactic Nuclei

Paul Martini, Michael W. Regan, John S. Mulchaey +1

(Abridged) We present a detailed study of the relation between circumnuclear dust morphology, host galaxy properties, and nuclear activity in nearby galaxies. We use our sample of…

astro-ph2002★ 51 cited

An Intrinsic Baldwin Effect in the H-beta Broad Emission Line in the Spectrum of NGC 5548

Karoline M. Gilbert, Bradley M. Peterson

We investigate the possibility of an intrinsic Baldwin Effect (i.e.,nonlinear emission-line response to continuum variations) in the broad H-beta emission line of the active galaxy…

astro-ph2002★ 140 cited

Galaxy Clustering and Galaxy Bias in a Lambda-CDM Universe

David H. Weinberg, Romeel Dav'e, Neal Katz +1

We investigate galaxy clustering and galaxy-mass correlations in the LCDM cosmological model using a large volume SPH simulation. For the most part, the predicted biases between ga…