Stellar-to-halo mass relation of cluster galaxies

Stellar-to-halo mass relation of cluster galaxies

In the formation of galaxy groups and clusters, the dark matter haloes containing satellite galaxies are expected to be tidally stripped in gravitational interactions with the host. We use galaxy-galaxy weak lensing to measure the average mass of dark matter haloes of satellite galaxies as a functio...

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Bibliographic Details
Main Authors: Niemiec, Anna, Jullo, Eric, Limousin, Marceau, Giocoli, Carlo, Erben, Thomas, Hildebrant, Hendrik, Kneib, Jean-Paul, Leauthaud, Alexie, Makler, Martin, Moraes, Bruno, Pereira, Maria E. S., Shan, Huanyuan, Rozo, Eduardo, Rykoff, Eli, Van Waerbeke, Ludovic
Other Authors: Univ Arizona, Dept Phys
Language:en
Published: OXFORD UNIV PRESS 2017
Subjects:
gravitational lensing: weak
galaxies: clusters: general
Online Access:http://hdl.handle.net/10150/625737
http://arizona.openrepository.com/arizona/handle/10150/625737

Internet

http://hdl.handle.net/10150/625737
http://arizona.openrepository.com/arizona/handle/10150/625737

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