Galaxy halo truncation and giant arc surface brightness reconstruction in the cluster MACSJ1206.2-0847

In this work we analyze the mass distribution of MACSJ1206.2-0847, especially focusing on the halo properties of its cluster members. The cluster appears relaxed in its X-ray emission, but has significant amounts of intracluster light which is not centrally concentrated, suggesting that galaxy-scale...

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Bibliographic Details
Main Authors: Eichner, Thomas (Author) , Zitrin, Adi (Author) , Bartelmann, Matthias (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: 21 Jun 2013
In: Arxiv

Online Access:Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1306.5240
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Author Notes:Thomas Eichner, Stella Seitz, Sherry H. Suyu, Aleksi Halkola, Keiichi Umetsu, Adi Zitrin, Dan Coe, Anna Monna, Piero Rosati, Claudio Grillo, Italo Balestra, Marc Postman, Anton Koekemoer, Wei Zheng, Ole Høst, Doron Lemze, Tom Broadhurst, Leonidas Moustakas, Larry Bradley, Alberto Molino, Mario Nonino, Amata Mercurio, Marco Scodeggio, Matthias Bartelmann, Narciso Benitez, Rychard Bouwens, Megan Donahue, Leopoldo Infante, Stephanie Jouvel, Daniel Kelson, Ofer Lahav, Elinor Medezinski, Peter Melchior, Julian Merten, Adam Riess
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Galaxy halo truncation and giant arc surface brightness reconstruction in the cluster MACSJ1206.2-0847 by Eichner, Thomas (Author) , Zitrin, Adi (Author) , Bartelmann, Matthias (Author) ,


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