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A weak lensing mass reconstruction of the large-scale filament feeding the massive galaxy cluster MACS J0717.5+3745

Mathilde JauzacAstrophysics and Cosmology Research Unit, School of Mathematical Sciences, University of KwaZulu-Natal, Durban 4041, South AfricaEric JulloJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USAJean‐Paul KneibLaboratoire d’Astrophysique de Marseille - LAM; Université d’Aix-Marseille & CNRS; UMR7326, 38 rue F. Joliot-Curie; 13388; Marseille Cedex 13; FranceH. EbelingInstitute for Astronomy; University of Hawaii; 2680 Woodlawn Drive; Honolulu; HI; 96822; USAAlexie LeauthaudKavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), Todai Institutes for Advanced Study; the University of Tokyo; Kashiwa; 277-8583; JapanCheng-Jiun MaInstitute for Astronomy; University of Hawaii; 2680 Woodlawn Drive; Honolulu; HI; 96822; USAMarceau LimousinDark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen, DenmarkR. MasseyInstitute for Computational Cosmology; Durham University; South Road; Durham; DH1 3LEJohan RichardCRAL, Observatoire de Lyon; Université Lyon 1; 9 Avenue Ch. André; 69561; Saint Genis Laval Cedex; France
2012en
ABI

Аннотация

We report the first weak lensing detection of a large-scale filament funnelling matter on to the core of the massive galaxy cluster MACS J0717.5+3745.

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