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Planck intermediate results - III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal

MPS-Authors
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Böhringer,  H.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Chon,  G.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Dolag,  K.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Enßlin,  T. A.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Hernández-Monteagudo,  C.
High Energy Astrophysics, MPI for Astrophysics, Max Planck Society;

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Knoche,  J.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Matthai,  F.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Rachen,  J. P.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Reinecke,  M.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Sunyaev,  R.
High Energy Astrophysics, MPI for Astrophysics, Max Planck Society;

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White,  S. D. M.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Planck Collaboration, Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Atrio-Barandela, F., et al. (2013). Planck intermediate results - III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal. Astronomy & Astrophysics, 550: A129, pp. 1-20. doi:10.1051/0004-6361/201219398.


Cite as: https://hdl.handle.net/11858/00-001M-0000-000E-EC96-D
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