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 | ||||||||||
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| Additional Information: | © 1997 Springer-Verlag Berlin Heidelberg. | ||||||||||
| DOI: | 10.1007/978-3-540-49709-7_43 | ||||||||||
| 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: | 15 Nov 2021 16:34 |
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