Radio Observations of the Subaru/XMM-Newton Deep Survey Field.

Autor: Renzini, Alvio, Bender, Ralf, Simpson, Chris, Rawlings, Steve, Ivison, Rob
Zdroj: Multiwavelength Mapping of Galaxy Formation & Evolution; 2005, p461-462, 2p
Abstrakt: The Subaru/XMM-Newton Deep Survey[1] (SXDS) comprises deep optical and X-ray observations of an area of sky larger than a square degree. With a transverse size of 100 Mpc at z = 1.5, the SXDS can detect and measure large-scale structure which will strongly affect the global results from smaller surveys. This region of sky is also home to a 0.8-deg2 ultra-deep near-infrared imaging survey [2], a 0.25-deg2 submillimetre survey [3], and also lies within the XMM-LSS region which will be observed by SIRTF as part of the SWIRE Legacy Program [4], and by GALEX as part of its Deep Imaging Survey and Medium-Deep Spectroscopic Survey. Extragalactic radio sources are able to probe large-scale structure and inform on the accretion and star formation histories of the Universe, and we have therefore undertaken deep radio observations to complete an unparalleled multi-wavelength dataset. This paper introduces the radio data in this field. [ABSTRACT FROM AUTHOR]
Databáze: Supplemental Index