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The high mass end of the stellar mass function: Dependence on stellar population models and agreement between fits to the light profile (2017)

First Author: Bernardi M

Attributed to: Astrophysics at Southampton funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stx176

Publication URI: http://dx.doi.org/10.1093/mnras/stx176

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society