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pro vyhledávání: '"Stephenson, Harry"'
We use a sample of 11 $z\approx0.2-0.5$ ($z_{\text{med.}} = 0.36$) galaxy clusters from the Cluster Lensing And Supernovae survey with Hubble (CLASH) to analyse the angular dependence of satellite galaxy colour $(B-R)$ and passive galaxy fractions ($
Externí odkaz:
http://arxiv.org/abs/2412.07834
Autor:
Stephenson, Harry R.
Publikováno v:
JAMA: Journal of the American Medical Association; September 1960, Vol. 174 Issue: 3 p287-292, 6p
Publikováno v:
Applied Spectroscopy; August 1957, Vol. 11 Issue: 3 p131-136, 6p