The Halo Mass Distribution of Field and Cluster Early-Type Galaxies

Details The Halo Mass Distribution of Field and Cluster Early-Type Galaxies The Halo Mass Distribution of Field and Cluster Early-Type Galaxies

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..220..175b&link_type=abstract

International Astronomical Union Symposium no. 220, held 21 - 25 July, 2003 in Sydney, Australia. Eds: S. D. Ryder, D. J. Pisano

Astronomy and Astrophysics

Astronomy

Scientific paper

We describe an ongoing program to study the halo kinematics of a broad sample of early-type galaxies using integrated light measurements obtained with the Hobby-Eberly and Gemini Telescopes.
The Hobby-Eberly Telescope is operated by McDonald Observatory on behalf of the University of Texas at Austin, The Pennsylvania State University, Stanford University, Ludwid-Maximilians-Universit at Munchen, and Georg-August-Universitat Gottingen.
Part of this project is based on observations obtained at the Gemini Observatory, which is operated by AURA, INC., under a cooperative agreement with the NSF on behalf of the Gemini Partnership: The NSF (USA), PPARC (UK), NRC (Canada), CONICYT (Chile), ARC (Australia), CNPq (Brazil) and CONICET (Argentina ).

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