output
19982025
most citedProbing the Coevolution of Supermassive Black Holes and Galaxies Using Gravitationally Lensed Quasar Hosts

418 citations

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12 papers · 1 filter

astro-ph2006★ 24 cited

The Host Galaxy of the Quasar HE 0450-2958

Minjin Kim, Luis C. Ho, Chien Y. Peng +1

A recent study suggests that the quasar HE 0450-2958 is hosted by a galaxy substantially fainter than that inferred from the correlation between black hole mass and bulge luminosit…

astro-ph2006★ 117 cited

Remarks on statistical errors in equivalent widths

Klaus Vollmann, Thomas Eversberg

Equivalent width measurements for rapid line variability in atomic spectral lines are degraded by increasing error bars with shorter exposure times. We derive an expression for the…

astro-ph2006★ 418 cited

Probing the Coevolution of Supermassive Black Holes and Galaxies Using Gravitationally Lensed Quasar Hosts

C. Y. Peng, C. D. Impey, H. -W. Rix +5

In the present-day universe, supermassive black hole masses (MBH) appear to be strongly correlated with their galaxy's bulge luminosity, among other properties. In this study, we e…

astro-ph2004★ 105 cited

Stellar Population in LLAGN.I: Ground-based observations

Roberto Cid Fernandes, Rosa M. Gonzalez Delgado, Henrique Schmitt +6

(Abridge): We present a spectroscopic study of the stellar populations of Low Luminosity AGN (LLAGN). Our main goal is to determine whether the stars who live in the innermost (100…

astro-ph2004★ 78 cited

Stellar Population in LLAGN.II: STIS observations

Rosa M. Gonzalez Delgado, Roberto Cid Fernandes, Enrique Perez +5

We present a study of the stellar population in Low Luminosity AGN (LLAGN). Our goal is to search for spectroscopic signatures of young and intermediate age stars, and to investiga…

astro-ph2002★ 24 cited

Is a minor-merger driving the nuclear activity in the Seyfert 2 galaxy NGC 2110?

Rosa M. Gonzalez Delgado, Santiago Arribas, Enrique Perez +1

We report on a detailed morphological and kinematic study of the isolated non-barred nearby Seyfert 2 galaxy NGC 2110. We combine Integral Field optical spectroscopy, with long-sli…

astro-ph2000

The Nuclei of Nearby Radio-Loud Ellipticals

G. A. Verdoes Kleijn, P. T. de Zeeuw, S. A. Baum +5

We have observed a complete sample of 21 nearby (D < 70h^{-1} Mpc) Fanaroff & Riley Type I galaxies with HST/WFPC2 and detected dust disks and lanes in 19 of them. The radio jets a…

astro-ph2000★ 203 cited

The Nuclear and Circum-nuclear Stellar Population in Seyfert 2 Galaxies: Implications for the Starburst-AGN Connection

R. M. Gonzalez Delgado, T. Heckman, C. Leitherer

We report the results of a spectroscopic investigation of a sample of 20 of the brightest type 2 Seyfert nuclei. Our goal is to search for the direct spectroscopic signature of mas…

astro-ph1998★ 135 cited

The black hole mass distribution in early-type galaxies: cusps in HST photometry interpreted through adiabatic black hole growth

R. P. van der Marel

The surface brightness profiles of early-type galaxies have central cusps. Two characteristic profile types are observed with HST: `core' profiles have a break at a resolved radius…

astro-ph1998★ 195 cited

Ultraviolet-Optical observations of the Seyfert 2 Galaxies NGC 7130, NGC 5135 and IC 3639: Implications for the Starburst-AGN Connection

Rosa M. Gonzalez Delgado, Timothy Heckman, Claus Leitherer +5

We present and discuss HST (WFPC2 and FOC) images and UV GHRS spectra plus ground-based near UV through to near IR spectra of three Seyfert 2 nuclei (NGC 7130, NGC 5135 and IC 3639…

astro-ph1998★ 1 cited

Astrometric Microlensing of Stars

Martin Dominik, Kailash C. Sahu

Due to dramatic improvements in the precision of astrometric measurements, the observation of light centroid shifts in observed stars due to intervening massive compact objects (`a…

astro-ph1998★ 141 cited

Evidence for a 3 x 10^8 solar mass black hole in NGC 7052 from HST observations of the nuclear gas disk

R. P. van der Marel, F. C. van den Bosch

We present an HST study of the nuclear region of the E4 radio galaxy NGC 7052, which has a nuclear disk of dust and gas. The WFPC2 was used to obtain B, V and I broad-band images a…