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19952004
most citedBlack Hole Mass Determinations From Orbit Superposition Models are Reliable

4 citations · 4 across the 2 of their papers we have counts for

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astro-ph20044 cited

Black Hole Mass Determinations From Orbit Superposition Models are Reliable

Douglas Richstone, Karl Gebhardt, Monique Aller +13

We show that orbit-superposition dynamical models (Schwarzschild's method) provide reliable estimates of nuclear black hole masses and errors when constructed from adequate orbit l…

astro-ph2003

Globular Clusters in Early-Type Galaxies with GMOS

Terry Bridges, Mike Beasley, Favio Faifer +6

We present recent results from our long-term Gemini/GMOS study of globular clusters in early-type galaxies. To date, we have obtained photometry and spectroscopy for clusters in NG…

astro-ph2003

Influence of Black Holes on Stellar Orbits

Karl Gebhardt

We review the current state of dynamical modeling for galaxies in terms of being able to measure both the central black hole mass and stellar orbital structure. Both of these must…

astro-ph2001

Spectroscopy of Globular Clusters in NGC 1399 - A Progress Report

T. Richtler, B. Dirsch, D. Geisler +9

We performed spectroscopy of globular clusters associated with NGC 1399 and measured radial velocities of more than 400 clusters, the largest sample ever obtained for dynamical stu…

astro-ph1999

Obtaining Galaxy Masses Using Stellar Absorption and [O II] Emission-Line Diagnostics in Late-Type Galaxies

Chip Kobulnicky, Karl Gebhardt

The [O II] lambda3727 emission lines and absorption features from stellar Balmer and Ca H&K lines are the most accessible kinematic diagnotics in galaxies at z~1. We investigate th…

astro-ph1996

The Quadruple Gravitational Lens PG1115+080: Time Delays and Models

P. L. Schechter, C. D. Bailyn, R. Barr +24

Optical photometry is presented for the quadruple gravitational lens PG1115+080. A preliminary reduction of data taken from November 1995 to June 1996 gives component ``C'' leading…