Mass distribution in the most X-ray-luminous galaxy cluster RX J1347.5-1145 studied with XMM-Newton

M. Gitti¹ - R. Piffaretti² - S. Schindler³

1 - INAF - Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy
2 - SISSA/ISAS, via Beirut 4, 34014 Trieste, Italy
3 - Institut für Astro- und Teilchen Physik, Leopold-Franzens Universität Innsbruck, Technikerstraße 25, 6020 Innsbruck, Austria

A&A 472, 383-394 (2007), DOI: 10.1051/0004-6361:20077580

Key words: galaxies: clusters: individual: RX J1347.5-1145 - X-rays: galaxies: clusters - galaxies: intergalactic medium - galaxies: cooling flows - cosmology: dark matter - cosmology: observations - errata, addenda

A wrong ``Note added in proofs'' has been inserted during the production process. The text of the current note added in proofs reads as follows:

Note added in proofs

As a private communication after this work was accepted for publication, Marusa Bradac pointed out that the lensing masses reconstructed outside $\sim$ 510 kpc are not very reliable because of the large error bars, and also very small radii have a significant error. This, however, does not change the main conclusion derived from the comparison with X-ray masses, since a general large discrepancy is found at all radii.