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NASA Technical Reports Server (NTRS) 20100033351: [CII] At 1 < z < 2: Observing Star Formation in the Early Universe with Zeus (1 and 2) PDF

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Preview NASA Technical Reports Server (NTRS) 20100033351: [CII] At 1 < z < 2: Observing Star Formation in the Early Universe with Zeus (1 and 2)

[CII] At 1<z<2: Observing Star Formation In The Early Universe With Zeus(I Page I of 2 7Z,010_ (b 1 Sign on ly k., SAO/NASA ADS Astronomy Abstract Service • Find Similar Abstracts (with d-- e—tf a -s-u-e-l- -t-t--i--n---g s bdqw) • Also-Read Articles (Reads History) • T- r- —a —n -s - late This PaW ------------- I---,--- Title: [CII] At I<z<2: Observing Star Formation In The Early Universe With Zeus (1 &2). Authors: Ferk-inhoff, Carl; Hailey-Dunsheath, S.; Nikola. T.; Oberst, T.; Parshley, S.; Stacey, G,; Benford D.; Staguhn, Affiliation: AA(Cornell University), AB(Max-Planck-Institut ffir extraterrestrische Physik, Germany), AC(Cornell University), AD(Westminster College), AE(Cornell University), AF(Comell University), AG(Goddard Space Flight Center), AH (Goddard Space Flight Center) Publication: American Astronomical Society, AAS Meeting #215, #387.08; Bulletin of the American Astronomical Society, Vol, 42, p.603 Publication Date: 0112010 Origin: AAS Bibliographic Code: 20 1 OAAS .. 21538708F Abstract We report the detection of the [CII] 158 micron fine structure line from six submillimeter galaxies with redshifts between 1.12 and 1.73. This more than doubles the total number of [CII] 158 micron detections reported from high redshift sources. These observations were made with the Redshift(z) and Early Universe Spectrometer(ZEUS) at the Caltech Submillimeter Observatory on Mauna Kea, Hawaii between December 2006 and March 2009. ZEUS is a background limited submm echelle grating spectrometer (Hailey-Dunsheath 2009). Currently we are constructing ZEUS-2. This new instrument will utilize the same grating but will feature a two dimensional transition-edge sensed bolometer array with SQUID multiplexing readout system enabling simultaneous background limited observations in the 200, 340,450 and 650 micron telluric windows. ZEUS-2 will allow for long slit imaging spectroscopy in nearby galaxies and a [CII] survey from z 0.25 to 2.5. Bibtex entry for this abstract Preferred format for this abstract (see Preferences) Add this article to private iibrary Remove this article from private library. Find Similar Abstracts: http://adsabs.harvard.edu/abs/201 OAAS ... 21538708F 812712010

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