The high mass end of the stellar mass function: Dependence on stellar population models and agreement between fits to the light profile-Reference-Cited by-同舟云学术

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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

Published:2017-01-23 Issue: Volume: Page:stx176
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Bernardi M.,Meert A.,Sheth R. K.,Fischer J.-L.,Huertas-Company M.,Maraston C.,Shankar F.,Vikram V.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/467/2/2217/10874268/stx176.pdf

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