The SAMI Galaxy Survey: Mass as the Driver of the Kinematic Morphology–Density Relation in Clusters-Reference-Cited by-同舟云学术

The SAMI Galaxy Survey: Mass as the Driver of the Kinematic Morphology–Density Relation in Clusters

Published:2017-07-21 Issue:1 Volume:844 Page:59
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Brough Sarah,van de Sande Jesse,Owers Matt S.,d’Eugenio Francesco,Sharp Rob,Cortese Luca^ORCID,Scott Nicholas^ORCID,Croom Scott M.,Bassett Rob,Bekki Kenji^ORCID,Bland-Hawthorn Joss^ORCID,Bryant Julia J.,Davies Roger,Drinkwater Michael J.^ORCID,Driver Simon P.^ORCID,Foster Caroline^ORCID,Goldstein Gregory,López-Sánchez Á. R.,Medling Anne M.^ORCID,Sweet Sarah M.^ORCID,Taranu Dan S.^ORCID,Tonini Chiara,Yi Sukyoung K.^ORCID,Goodwin Michael,Lawrence J. S.,Richards Samuel N.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/844/i=1/a=59/pdf

Reference67 articles.

1. The SAMI Galaxy Survey: Early Data Release

2. Galaxy Zoo: the dependence of morphology and colour on environment

3. SExtractor: Software for source extraction

4. Hexabundles: imaging fiber arrays for low-light astronomical applications

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