... more independent parameters are required to account for the line strength variations in the distant cluster data than in the Coma data, and second, line strengths which are not correlated in the distant cluster data are strongly coupled in the Coma data ...
... Diffuse Emission in/around the Coma Cluster: Beyond Simple Accretion . ... RESEARCH . CV . Publications . Coma . Relics . ... Coma . Relics . Here is a full resolution pdf of our recent Coma Cluster paper. ...
... Coma cluster paper accepted to MNRAS . ... RESEARCH . CV . Publications . Coma . Relics . ... clear cases of partial shock illumination (like Coma and Abell 548, but much more ...
... in each principal component for the clean Coma, noisy Coma, and high redshift data ... represent the clean Coma data, filled squares represent the noisy Coma data, and ...
... Coma, and noisy Coma samples indepentdently, producing three sets of new axes, or ... artificially dominated by the Coma spectra due to the larger number of Coma galaxies ...
... Comparison of Line Strength Variations in Coma and Cluster Galaxies at z 0.3 ... The Coma cluster data have been published by Caldwell et al. (1993) and Caldwell ... All of the Coma spectra are cluster members. ...
... CSIROpedia . A Statistical Comparison of Line Strength Variations in Coma and Cluster Galaxies at z 0.3 . ... thank Jim Rose and Nelson Caldwell for providing the Coma spectra and Charley Lineweaver, Simon Driver, and Michael Drinkwater ...
... CSIROpedia . A Statistical Comparison of Line Strength Variations in Coma and Cluster Galaxies at z 0.3 . ... High- z . Percentage chance that correlation could result from a random distribution ...Coma . Same as for High- z ...KS . ...