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The X-ray luminous galaxy cluster population at 0.9 < z less than or similar to 1.6 as revealed by the XMM-Newton distant cluster project

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons18622

Fassbender,  R.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4835

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons26359

Nastasi,  A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons22333

Suhada,  R.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4875

Mühlegger,  M.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons4872

Mohr,  J. J.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Citation

Fassbender, R., Böhringer, H., Nastasi, A., Suhada, R., Mühlegger, M., de Hoon, A., et al. (2011). The X-ray luminous galaxy cluster population at 0.9 < z less than or similar to 1.6 as revealed by the XMM-Newton distant cluster project. New Journal of Physics, 13(12): 125014, pp. 1-53. doi:10.1088/1367-2630/13/12/125014.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000F-4297-F
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