NASA Jet Propulsion Laboratory California Institute of Technology Follow this link to skip to the main content

BEACON eSpace at Jet Propulsion Laboratory >
JPL Technical Report Server >
JPL TRS 1992+ >

Please use this identifier to cite or link to this item: http://hdl.handle.net/2014/40878

Title: Rest-frame mid-infrared detection of an extremely luminous lyman break galaxy with the Spitzer Infrared Spectrograph (IRS)
Authors: Teplitz, H. I.
Charmandaris, V.
Armus, L.
Appleton, P. N.
Houck, J. R.
Soifer, B. T.
Weedman, D.
Brandl, B. R.
van Cleve, J.
Grillmair, C.
Uchid, K. I.
Keywords: cosmology
galaxies
high redshift
Issue Date: Sep-2004
Publisher: American Astronomical Society
Citation: The Astrophysical Journal Supplement Series, 154:103–106, 2004 September doi.org/10.1086/423134
Abstract: We present the first rest-frame ~4 μm detection of a Lyman break galaxy. The data were obtained using the 16 μm imaging capability of the Spitzer Infrared Spectrograph. The target object, J134026.44+634433.2, is an extremely luminous Lyman break galaxy at z = 2:79, first identified in Sloan Digital Sky Survey (SDSS) spectra (as reported by Bentz et al.). The source is strongly detected with a flux of 0:94 ± 0:02 mJy. Combining Spitzer and SDSS photometry with supporting ground-based J- and K-band data, we show that the spectral energy distribution is consistent with an actively star-forming galaxy. We also detect other objects in the Spitzer field of view, including a very red mid-infrared source. We find no evidence of a strong lens among the mid-infrared sources.
URI: http://hdl.handle.net/2014/40878
Appears in Collections:JPL TRS 1992+

Files in This Item:

File Description SizeFormat
04-1139.pdf174.5 kBAdobe PDFView/Open

Items in DSpace are protected by copyright, but are furnished with U.S. government purpose use rights.

 

Privacy/Copyright Image Policy Beacon Home Contact Us
NASA Home Page + Div 27
+ JPL Space
Site last updated on November 15, 2012.
If you have any comments or suggestions for this web site, please e-mail Alexander Smith or call 4-4202.