• C. De Boni, K. Dolag, S. Ettori, L. Moscardini, V. Pettorino, and C. Baccigalupi. Hydrodynamical simulations of galaxy clusters in dark energy cosmologies - I. General properties. mnras , 415:2758-2772, aug 2011.

  • J. P. Henry and K. A. Arnaud. A measurement of the mass fluctuation spectrum from the cluster X-ray temperature function. apj , 372:410-418, May 1991.

  • J. P. Henry. A Measurement of the Density Parameter Derived from the Evolution of Cluster X-Ray Temperatures. apjl , 489:L1, November 1997.

  • J. P. Henry. Measuring Cosmological Parameters from the Evolution of Cluster X-Ray Temperatures. apj , 534:565-580, May 2000.

  • J. P. Henry. X-Ray Temperatures for the Extended Medium-Sensitivity Survey High-Redshift Cluster Sample: Constraints on Cosmology and the Dark Energy Equation of State. apj , 609:603-616, July 2004.

  • G. Yepes, R. Sevilla, S. Gottlöber, and J. Silk. Is WMAP3 Normalization Compatible with the X-Ray Cluster Abundance?. apjl , 666:L61-L64, sep 2007.