Cross-calibrating X-ray detectors with clusters of galaxies: an IACHEC study
暂无分享,去创建一个
[1] M. Markevitch,et al. Chandra Temperature Profiles for a Sample of Nearby Relaxed Galaxy Clusters , 2004, astro-ph/0412306.
[2] P. P. Plucinsky,et al. CHANDRA SPECTRA OF THE SOFT X-RAY DIFFUSE BACKGROUND , 2003 .
[3] C. Sarazin,et al. CHANDRA OBSERVATION OF THE COOLING FLOW CLUSTER ABELL 2052 , 2002, astro-ph/0211027.
[4] C. Sarazin,et al. PROPERTIES OF CLUSTERS OF GALAXIES , 1988 .
[5] XMM-NEWTON OBSERVATIONS OF EVOLUTION OF CLUSTER X-RAY SCALING RELATIONS AT z = 0.4-0.7 , 2005, astro-ph/0504233.
[6] S. L. Snowden,et al. A Catalog of Galaxy Clusters Observed by XMM-Newton , 2007, 0710.2241.
[7] J. Kaastra,et al. Non-Maxwellian electron distributions in clusters of galaxies , 2009, 0905.4802.
[8] Temperature Profiles of Nearby Clusters of Galaxies , 2002 .
[9] D. Liedahl,et al. Collisional Plasma Models with APEC/APED: Emission-Line Diagnostics of Hydrogen-like and Helium-like Ions , 2001, astro-ph/0106478.
[10] C. Jones,et al. ERRATUM: “CHANDRA SAMPLE OF NEARBY RELAXED GALAXY CLUSTERS: MASS, GAS FRACTION, AND MASS–TEMPERATURE RELATION” (2006, ApJ, 640, 691) , 2005, astro-ph/0507092.
[11] N. Grevesse,et al. Abundances of the elements: Meteoritic and solar , 1989 .
[12] T. Akahori,et al. Hydrodynamic Simulations of Merging Galaxy Clusters: Non-Equilibrium Ionization State and Two-Temperature Structure , 2009, 0909.5025.
[13] D. Prokhorov. Non-equilibrium ionization states in galaxy clusters , 2009, 0911.0119.
[14] M. Markevitch,et al. ACCEPTED FOR PUBLICATION IN APJ Preprint typeset using LATEX style emulateapj v. 11/26/04 XMM-NEWTON EPIC BACKGROUND MODELING FOR EXTENDED SOURCES , 2005 .
[15] L. Moscardini,et al. Comparing the temperatures of galaxy clusters from hydrodynamical N-body simulations to Chandra and XMM-Newton observations , 2004, astro-ph/0404425.
[16] F. Durret,et al. An analysis of electron distributions in galaxy clusters by means of the flux ratio of iron lines FeXXV and XXVI , 2008, 0812.1650.
[17] J. Kaastra,et al. The final verdict by XMM-Newton: the X-ray obscured Seyfert galaxy NGC5506 has a broad Fe K-alpha line , 2010 .
[18] D. McCammon,et al. Photoelectric absorption cross sections with variable abundances , 1992 .
[19] P. Schady,et al. EPIC status of calibration and data analysis , 2006 .
[20] Y. Fukazawa,et al. Chandra and ROSAT Observations of NGC 5044: Profile of Dark Halos in Galaxy Groups , 2006 .
[21] K. Lodders. Solar System Abundances and Condensation Temperatures of the Elements , 2003 .