VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno (Corrigendum)

M. Viikinkoski; M. Kaasalainen; J. Ďurech; B. Carry; M. Marsset; T. Fusco; C. Dumas; W. J. Merline; B. Yang; J. Berthier; P. Kervella; P. Vernazza

doi:10.1051/0004-6361/201526626e

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201526626]

Issue		A&A Volume 582, October 2015


Article Number		C1
Number of page(s)		1
Section		Letters
DOI		https://doi.org/10.1051/0004-6361/201526626e
Published online		05 October 2015

A&A 582, C1 (2015)

VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno (Corrigendum)

M. Viikinkoski¹, M. Kaasalainen¹, J. Ďurech², B. Carry³^,4, M. Marsset⁵^,6, T. Fusco⁶^,7, C. Dumas⁵, W. J. Merline⁸, B. Yang⁵, J. Berthier³, P. Kervella⁹^,10 and P. Vernazza⁶

¹ Department of MathematicsTampere University of Technology, PO Box 553, 33101 Tampere, Finland
e-mail: matti.viikinkoski@tut.fi
² Astronomical Institute, Faculty of Mathematics and Physics, Charles University in Prague, V Holešovičkách 2, 18000 Prague, Czech Republic
³ ACME, IMCCE, UMR 8028 du CNRS, UPMC, Université de Lille 1, 77 Av. Denfert-Rochereau, 75014 Paris, France
⁴ Laboratoire Lagrange, UMR 7293 CNRS, UNS, Observatoire de la Côte d’Azur, 06304 Nice, France
⁵ European Southern Observatory (ESO), Alonso de Còrdova 3107, 1900 Casilla Vitacura, Santiago, Chile
⁶ Aix-Marseille University, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388 Marseille, France
⁷ ONERA − Optics Department, 29 avenue de la Division Leclerc, 92322 Chatillon Cedex, France
⁸ Southwest Research Institute, 1050 Walnut St., #300 Boulder, CO 80302, USA
⁹ Unidad Mixta Internacional FCA (UMI 3386), CNRS/INSU & Universidad de Chile, Las Condes, Santiago, Chile
¹⁰ LESIA (UMR 8109), Observatoire de Paris, CNRS, UPMC, Univ. Paris-Diderot, PSL, 5 place Jules Janssen, 92195 Meudon, France

Key words: instrumentation: interferometers / instrumentation: adaptive optics / minor planets, asteroids: individual: (3) Juno / methods: numerical / errata, addenda

Erratum for: A&A 581, L3 (2015), DOI: 10.1051/0004-6361/201526626

Fig. 4

Adaptive-optics images used for reconstruction (top) and corresponding model views (bottom). See Table 1 for observing conditions and instruments. The scattering law used for the shading exaggerates surface features.

© ESO, 2015

All Figures

	Fig. 4 Adaptive-optics images used for reconstruction (top) and corresponding model views (bottom). See Table 1 for observing conditions and instruments. The scattering law used for the shading exaggerates surface features.
In the text

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