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Millimetre Emission from High Redshift Radioquiet Quasars

Omont, A. and McMahon, R. G. and Bergeron, J. and Cox, P. and Guilloteau, S. and Kreysa, E. and Pajot, F. and Pécontal, E. and Petitjean, P. and Solomon, P. M. and Storrie-Lombardi, L. J. (1997) Millimetre Emission from High Redshift Radioquiet Quasars. In: The Early Universe with the VLT. Springer , Berlin, pp. 357-360. ISBN 978-3-662-22488-5. https://resolver.caltech.edu/CaltechAUTHORS:20170329-111636341

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Abstract

The detection at millimetre wavelengths of continuum radiation emitted by dust in high z quasars is favored by the steepness of the far infrared-submm spectrum in the rest frame. About 10 radioquiet quasars at z > 2, the majority of them at z > 4, have now been detected at 1.25mm with the IRAM 30m telescope, with fluxes in the range 3–15 mJy. Millimeter lines of CO are slightly more difficult to detect, but already within the reach of sensitive interferometers for several of these sources. The J = 5–4 line has recently been detected in BR1202–0725 at redshift 4.69.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1007/978-3-540-49709-7_43DOIArticle
http://link.springer.com/chapter/10.1007%2F978-3-540-49709-7_43PublisherArticle
ORCID:
AuthorORCID
Omont, A.0000-0002-4721-3922
Cox, P.0000-0003-2027-8221
Storrie-Lombardi, L. J.0000-0002-5987-5210
Additional Information:© 1997 Springer-Verlag Berlin Heidelberg.
Record Number:CaltechAUTHORS:20170329-111636341
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170329-111636341
Official Citation:Omont A. et al. (1997) Millimetre Emission from High Redshift Radioquiet Quasars. In: Bergeron J. (eds) The Early Universe with the VLT. ESO Astrophysics Symposia (European Southern Observatory). Springer, Berlin, Heidelberg
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:75511
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:29 Mar 2017 19:05
Last Modified:03 Oct 2019 16:51

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