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  Predicting quiescence: the dependence of specific star formation rate on galaxy size and central density at 0.5 < z < 2.5

Whitaker, K. E., Bezanson, R., van Dokkum, P. G., Franx, M., van der Wel, A., Brammer, G., et al. (2017). Predicting quiescence: the dependence of specific star formation rate on galaxy size and central density at 0.5 < z < 2.5. The Astrophysical Journal, 838(1): 19, pp. 1-19. doi:10.3847/1538-4357/aa6258.

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 Creators:
Whitaker, Katherine E., Author
Bezanson, Rachel, Author
van Dokkum, Pieter G., Author
Franx, Marijn, Author
van der Wel, Arjen, Author
Brammer, Gabriel, Author
Förster-Schreiber, Natascha M.1, Author           
Giavalisco, Mauro, Author
Labbé, Ivo, Author
Momcheva, Ivelina G., Author
Nelson, Erica J.1, Author           
Skelton, Rosalind, Author
Affiliations:
1Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159889              

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Language(s): eng - English
 Dates: 2017-03-20
 Publication Status: Published online
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.3847/1538-4357/aa6258
Other: LOCALID: 2457200
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Title: The Astrophysical Journal
  Abbreviation : Astrophys. J.
Source Genre: Journal
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Pages: - Volume / Issue: 838 (1) Sequence Number: 19 Start / End Page: 1 - 19 Identifier: ISSN: 0004-637X
ISSN: 1538-4357