Coupled blind signal separation and spectroscopic database fitting of the mid-infrared PAH features (Corrigendum)

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This article is an erratum for: [this article]

Issue		A&A Volume 537, January 2012


Article Number		C5
Number of page(s)		2
Section		Interstellar and circumstellar matter
DOI		http://dx.doi.org/10.1051/0004-6361/201016340e
Published online		25 January 2012

A&A 537, C5 (2012)

Coupled blind signal separation and spectroscopic database fitting of the mid-infrared PAH features (Corrigendum)^⋆

M. J. F. Rosenberg¹^,2, O. Berné¹, C. Boersma³, L. J. Allamandola³ and A. G. G. M. Tielens¹

¹ Sterrewacht Leiden, Universiteit Leiden, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands
e-mail: rosenberg@strw.leidenuniv.nl
² The International Space University, Parc d’Innovation, 1 rue Jean Dominique Cassini, 67400 Illkirch Graffenstaden, France
³ NASA Ames Research Center, Space Science Division, Mail Stop 245-6, Moffett Field, CA 94035, USA
e-mail: Louis.J.Allamandola@nasa.gov; Christiaan.Boersma@nasa.gov

This article has no abstract.

Key words: astrochemistry / infrared: ISM / ISM: lines and bands / photon-dominated region (PDR) / Errata, addenda

^⋆

This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA.

Erratum of: A&A 532, A128 (2011), DOI: 10.1051/0004-6361/201016340

© ESO, 2012

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Coupled blind signal separation and spectroscopic database fitting of the mid-infrared PAH features (Corrigendum)⋆

Coupled blind signal separation and spectroscopic database fitting of the mid-infrared PAH features (Corrigendum)^⋆