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Ish: XRISM Constraints on Unidentified X-Ray Emission Lines, Including the 3.5 keV Line, in the Stacked Spectrum of 10 Galaxy Clusters
Parameter estimation in astronomy through application of the likelihood ratio
Maqola197916 iqtibosABI<i>CHANDRA</i>STUDIES OF THE X-RAY GAS PROPERTIES OF GALAXY GROUPS
Ming Sun, G. Mark Voit, Megan Donahue +3
Maqola20098 iqtibosABIAn Accurate Physical Model for Halo Concentrations
Benedikt Diemer, Michael Joyce
Maqola20195 iqtibosABIUPDATED ATOMIC DATA AND CALCULATIONS FOR X-RAY SPECTROSCOPY
Adam Foster, L. Ji, Randall K. Smith +1
Maqola20123 iqtibosABIStatus of x-ray imaging and spectroscopy mission (XRISM)
M. Tashiro, Hironori Maejima, Kenichi Toda +97
Maqola20202 iqtibosABINon-thermal pressure support in X-COP galaxy clusters
D. Eckert, V. Ghirardini, S. Ettori +13
Maqola20182 iqtibosABIHydrostatic mass profiles in X-COP galaxy clusters
S. Ettori, V. Ghirardini, D. Eckert +7
Maqola20182 iqtibosABIThe bulk motion of gas in the core of the Centaurus galaxy cluster
M. Audard, Hisamitsu Awaki, Ralf Ballhausen +97
Maqola20252 iqtibosABIXRISM Forecast for the Coma Cluster: Stormy, with a Steep Power Spectrum
M. Audard, Hisamitsu Awaki, Ralf Ballhausen +97
Maqola20252 iqtibosABI