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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

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.

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 Creators:
Fassbender, R.1, Author           
Böhringer, H.1, Author           
Nastasi, A.1, Author           
Suhada, R.1, Author           
Mühlegger, M.1, Author           
de Hoon, A, Author
Kohnert, J, Author
Lamer, G, Author
Mohr, J. J.2, Author           
Pierini, D, Author
Pratt, G W, Author
Quintana, H, Author
Rosati, P, Author
Santos, J S, Author
Schwope, A D, Author
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              
2Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159895              

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Language(s): eng - English
 Dates: 2011-12-19
 Publication Status: Published online
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1088/1367-2630/13/12/125014
Other: LOCALID: 1362565
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Title: New Journal of Physics
  Abbreviation : New J. Phys.
Source Genre: Journal
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Pages: - Volume / Issue: 13 (12) Sequence Number: 125014 Start / End Page: 1 - 53 Identifier: ISSN: 1367-2630