The quasar MBH-Mhost relation through cosmic time - I. Data set and black hole masses

Bibcode
2010MNRAS.402.2441D
DOI
10.1111/j.1365-2966.2009.16048.x
Decarli, R.; Falomo, R.; Treves, A.; Kotilainen, J. K.; Labita, M.; Scarpa, R.
Referencia bibliográfica

Monthly Notices of the Royal Astronomical Society, Volume 402, Issue 4, pp. 2441-2452.

Fecha de publicación:
3
2010
Revista
Monthly Notices of the Royal Astronomical Society
Número de autores
6
Número de autores del IAC
1
Número de citas
37
Número de citas referidas
33
Descripción
We study the relation as a function of cosmic time in a sample of 96 quasars from z = 3 to the present epoch. In this paper, we describe the sample, the data sources and the new spectroscopic observations. We then illustrate how we derive from single-epoch spectra, pointing out the uncertainties in the procedure. In a companion paper, we address the dependence of the ratio between the black hole mass and the host-galaxy luminosity and mass on cosmic time.
Proyectos relacionados
Imagen del Proyecto
Astrofísica Relativista y Teórica
El estudio de las lentes gravitatorias proporciona poderosas herramientas en Astrofísica y Cosmología. Las principales aplicaciones de las lentes gravitatorias en las que se centra este proyecto son las siguientes: (i) estudiar la presencia de subestructura de materia obscura en las galaxias lente a partir de las anomalías en la magnificación de
Evencio
Mediavilla Gradolph
En ejecución
Tipo
Con árbitro
Cosmología y Astropartículas (CYA)
Galaxias
Cuásares

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