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X-Ray and Gamma-Ray Telescopes and Instruments for Astronomy, 2003

DOI: 10.1117/12.461330

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Data analysis method for XMM-Newton observations of extended sources and application to bright massive clusters of galaxies at z=0.2

Proceedings article published in 2003 by Philippe B. Marty, Jean-Paul Kneib ORCID, Rachida Sadat, Harald Ebeling, Ian Smail ORCID
This paper was not found in any repository; the policy of its publisher is unknown or unclear.
This paper was not found in any repository; the policy of its publisher is unknown or unclear.

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