Submillimetre photometry of 323 nearby galaxies from the Herschel Reference Survey (Corrigendum)

L. Ciesla; A. Boselli; M. W. L. Smith; G. J. Bendo; L. Cortese; S. Eales; S. Bianchi; M. Boquien; V. Buat; J. Davies; M. Pohlen; S. Zibetti; M. Baes; A. Cooray; I. de Looze; S. di Serego Alighieri; M. Galametz; H. L. Gomez; V. Lebouteiller; S. C. Madden; C. Pappalardo; A. Remy; L. Spinoglio; M. Vaccari; R. Auld; D. L. Clements

doi:10.1051/0004-6361/201219216e

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A&A, 550 (2013) C1

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201219216]

Issue		A&A Volume 550, February 2013


Article Number		C1
Number of page(s)		82
Section		Catalogs and data
DOI		https://doi.org/10.1051/0004-6361/201219216e
Published online		31 January 2013

A&A 550, C1 (2013)

Submillimetre photometry of 323 nearby galaxies from the Herschel Reference Survey^⋆ (Corrigendum)

L. Ciesla¹, A. Boselli¹, M. W. L. Smith², G. J. Bendo³, L. Cortese⁴, S. Eales², S. Bianchi⁵, M. Boquien¹, V. Buat¹, J. Davies², M. Pohlen², S. Zibetti⁵^,6, M. Baes⁷, A. Cooray⁸^,9, I. de Looze⁷, S. di Serego Alighieri⁵, M. Galametz¹⁰, H. L. Gomez², V. Lebouteiller¹¹, S. C. Madden¹¹, C. Pappalardo⁵, A. Remy¹¹, L. Spinoglio¹², M. Vaccari¹³^,14, R. Auld² and D. L. Clements¹⁵

¹ Laboratoire d’Astrophysique de Marseille – LAM, Université d’Aix-Marseille & CNRS, UMR 7326, 38 rue F. Joliot-Curie, 13388 Marseille Cedex 13, France
e-mail: laure.ciesla@oamp.fr
² School of Physics and Astronomy, Cardiff University, Queens Buildings The Parade, Cardiff CF24 3AA, UK
³ UK ALMA Regional Centre Node, Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK
⁴ European Southern Observatory, Karl Schwarzschild Str. 2, 85748 Garching bei Muenchen, Germany
⁵ INAF-Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125 Firenze, Italy
⁶ Dark Cosmology Centre, Niels Bohr Institute University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Denmark
⁷ Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281 S9, 9000 Gent, Belgium
⁸ Department of Physics & Astronomy, University of California, Irvine, CA 92697, USA
⁹ California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125, USA
¹⁰ Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
¹¹ CEA/DSM/IRFU/Service d’Astrophysique, CEA, Saclay, Orme des Merisiers, Bât. 709, 91191 Gif-sur-Yvette, France
¹² Istituto di Fisica dello Spazio Interplanetario, INAF, via Fosso del Cavaliere 100, 00133 Roma, Italy
¹³ Dipartimento di Astronomia, Università di Padova, vicolo Osservatorio 3, 35122 Padova, Italy
¹⁴ Astrophysics Group, Physics Department, University of the Western Cape, Private Bag X17, 7535 Bellville, Cape Town, South Africa
¹⁵ Astrophysics Group, Imperial College, Blackett Laboratory, PrinceConsort Road, London SW7 2AZ, UK

Key words: galaxies: ISM / infrared: galaxies / surveys / catalogs / errata, addenda

^⋆

Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

Erratum for: A&A 543, A161 (2012), DOI: 10.1051/0004-6361/201219216

1. HRS atlas

The 250 μm images of Fig. A.1 in Ciesla et al. (2012) were accidentally replaced by 350 μm images. The new figures with the 250 μm images missing in Ciesla et al. (2012) are available in the electronic version.

References

Ciesla, L., Boselli, A., Smith, M. W. L., et al. 2012, A&A, 543, A161 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

© ESO, 2013

Online material

	Fig. A.1 Images of the HRS galaxies. From left to right: SDSS r′ band image, 250, 350, and 500 μm Herschel images. The aperture used for the photometry is indicated by the solid line and the annulus, where the background is estimated, is indicated in dashed lines.
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All Figures

	Fig. A.1 Images of the HRS galaxies. From left to right: SDSS r′ band image, 250, 350, and 500 μm Herschel images. The aperture used for the photometry is indicated by the solid line and the annulus, where the background is estimated, is indicated in dashed lines.
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[1] Ciesla, L., Boselli, A., Smith, M. W. L., et al. 2012, A&A, 543, A161 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

Submillimetre photometry of 323 nearby galaxies from the Herschel Reference Survey⋆ (Corrigendum)

1. HRS atlas

References

Online material

All Figures

Submillimetre photometry of 323 nearby galaxies from the Herschel Reference Survey^⋆ (Corrigendum)