Hostname: page-component-76fb5796d-zzh7m Total loading time: 0 Render date: 2024-04-26T20:55:21.330Z Has data issue: false hasContentIssue false
  • English
  • Français

HST, IUE and ROSAT Observations of High Z QSOs

Published online by Cambridge University Press:  19 July 2016

D. L. Band ,
R. D. Cohen ,
P. R. Blanco ,
V. T. Junkkarinen ,
E. M. Burbidge ,
R. E. Rothschild  and
G. A. Reichert
D. L. Band
Affiliation:
CASS, UC San Diego, La Jolla, CA 92093
R. D. Cohen
Affiliation:
CASS, UC San Diego, La Jolla, CA 92093
P. R. Blanco
Affiliation:
CASS, UC San Diego, La Jolla, CA 92093
V. T. Junkkarinen
Affiliation:
CASS, UC San Diego, La Jolla, CA 92093
E. M. Burbidge
Affiliation:
CASS, UC San Diego, La Jolla, CA 92093
R. E. Rothschild
Affiliation:
CASS, UC San Diego, La Jolla, CA 92093
G. A. Reichert
Affiliation:
USRA, NASA-Goddard SFC, Code 668, Greenbelt, MD 20771

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The optical through X-ray spectra of 3 QSOs between z = 1.32 and 3.53 show these objects to be very similar to low z AGN.

Type
Poster Contributions: Continuum studies
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 318
Copyright
Copyright © Kluwer 1994