Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

Detection of far-infrared and polycyclic aromatic hydrocarbon emission from the cosmic eye : probing the dust and star formation of Lyman Break galaxies.

Siana, B. and Smail, I. and Swinbank, A.M. and Richard, J. and Teplitz, H.I. and Coppin, K.E.K. and Ellis, R.S. and Stark, D.P. and Kneib, J.-P. and Edge, A.C. (2009) 'Detection of far-infrared and polycyclic aromatic hydrocarbon emission from the cosmic eye : probing the dust and star formation of Lyman Break galaxies.', Astrophysical journal., 698 (2). pp. 1273-1281.

Abstract

We report the results of a Spitzer infrared (IR) study of the Cosmic Eye, a strongly lensed, L*UV Lyman break galaxy (LBG) at z = 3.074. We obtained Spitzer mid-IR spectroscopy as well as MIPS 24 and 70 μm photometry. The Eye is detected with high significance at both 24 and 70 μm and, when including a flux limit at 3.5 mm, we estimate an IR luminosity of L IR = 8.3+4.7 –4.4 × 1011 L ☉ assuming a magnification of 28± 3. This L IR is eight times lower than that predicted from the rest-frame ultraviolet properties assuming a Calzetti reddening law. This has also been observed in other young LBGs, and indicates that the dust reddening law may be steeper in these galaxies. The mid-IR spectrum shows strong polycyclic aromatic hydrocarbon (PAH) emission at 6.2 and 7.7 μm, with equivalent widths near the maximum values observed in star-forming galaxies at any redshift. The L PAH-to-L IR ratio lies close to the relation measured in local starbursts. Therefore, L PAH or L MIR may be used to estimate L IR, and thus star formation rate, of LBGs, whose fluxes at longer wavelengths are typically below current confusion limits. We also report the highest redshift detection of the 3.3 μm PAH emission feature. The PAH ratio, L 6.2/L 3.3 = 5.1 ± 2.7, and the PAH-to-LIR ratio, L 3.3/L IR = 8.5 ± 4.7 × 10–4, are both in agreement with measurements in local starbursts and ultraluminous infrared galaxies (ULIRGs), suggesting that this line may serve as a good proxy for L PAH or L IR at z > 3 with the James Webb Space Telescope.

Item Type:Article
Keywords:Galaxies, High-redshift, Individual (J213512.73 – 010143, Cosmic Eye), Infrared.
Full text:(VoR) Version of Record
Download PDF
(313Kb)
Status:Peer-reviewed
Publisher Web site:http://dx.doi.org/10.1088/0004-637X/698/2/1273
Publisher statement:© 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
Date accepted:No date available
Date deposited:04 September 2013
Date of first online publication:June 2009
Date first made open access:No date available

Save or Share this output

Export:
Export
Look up in GoogleScholar