350 micron SHARC-II Imaging of Luminous High-z Radio Galaxies

Details 350 micron SHARC-II Imaging of Luminous High-z Radio Galaxies 350 micron SHARC-II Imaging of Luminous High-z Radio Galaxies

2005-09-14

arxiv.org/abs/astro-ph/0509364v1

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, "Granada Workshop on High Redshift Radio Galaxies"

Scientific paper

10.1002/asna.200510508

Using the filled bolometer array SHARC-II on the Caltech Submillimeter Observatory (CSO), we have obtained deep (rms ~ 15mJy/beam), high-quality 350 micron maps of five of the most luminous high-z radio galaxies known. In all cases the central radio galaxy is detected at the >3sigma level, and in some cases the high resolution of SHARC-II (FWHM ~ 9") allows us to confirm the spatially extended nature of the dust emission. In PKS1138-262 (z=2.156), 8C1909+722 (z=3.538) and 4C41.17 (z=3.792), additional sources -- first discovered by SCUBA at 850 micron and believed to be dusty, merging systems associated with the central radio galaxy -- are detected at 350 micron. Furthermore, in PKS1138 and 4C41.17 additional SHARC-II sources are seen which were not detected at 850 micron, although the reality of these sources will have to be confirmed by independent submm observations. Thus, our observations seem to support the notion of extended star formation taking place in radio galaxies at high redshifts, and that these systems sit at the centers of overdense regions harbouring a complexity of dusty and vigorously star forming systems. At the redshift of the radio galaxies, the 350 micron observations sample very close to the rest-frame dust peak (typically at ~100 micron), and they therefore contribute a particularly important point to the spectral energy distributions of these sources, which we use this in conjunction with existing (sub)millimeter data to derive FIR luminosities, dust temperatures and spectral emissivities of the central radio galaxies.

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