Authors

Guillermo Barro, University of California - Santa Cruz
Jonathan R. Trump, Pennsylvania State University
David C. Koo, University of California - Santa Cruz
Avishai Dekel, Hebrew University, Israel
Susan A. Kassin, Space Telescope Science Institute
Dale D. Kocevski, University of KentuckyFollow
Sandra M. Faber, University of California - Santa Cruz
Arjen van der Wel, Max-Planck-Institut für Astronomie, Germany
Yicheng Guo, University of California - Santa Cruz
Pablo G. Pérez-González, Universidad Complutense de Madrid, Spain
Elisa Toloba, University of California - Santa Cruz
Jerome J. Fang, University of California - Santa Cruz
Camilla Pacifici, Yonsei University, Korea
Raymond Simons, Johns Hopkins University
Randy D. Campbell, California Association for Research in Astronomy
Daniel Ceverino, Universidad Autonoma de Madrid, Spain
Steven L. Finkelstein, University of Texas at Austin
Bob Goodrich, California Association for Research in Astronomy
Marc Kassis, California Association for Research in Astronomy
Anton M. Koekemoer, Space Telescope Science Institute
Nicholas P. Konidaris, California Institute of Technology
Rachel C. Livermore, University of Texas at Austin
James E. Lyke, California Association for Research in Astronomy
Bahram Mobasher, University of California - Riverside
Hooshang Nayyeri, University of California - Riverside
Michael Peth, Johns Hopkins University
Joel R. Primack, University of California - Santa Cruz
Luca Rizzi, California Association for Research in Astronomy
Rachel S. Somerville, Rutgers University
Gregory D. Wirth, California Association for Research in Astronomy
Adi Zolotov, Hebrew University, Israel

Abstract

We present Keck-I MOSFIRE near-infrared spectroscopy for a sample of 13 compact star-forming galaxies (SFGs) at redshift 2 ≤ z ≤ 2.5 with star formation rates of SFR ~ 100 M yr–1 and masses of log(M/M ) ~10.8. . . .

For the remainder of the abstract, please visit:

http://dx.doi.org/10.1088/0004-637X/795/2/145

Document Type

Article

Publication Date

10-23-2014

Notes/Citation Information

Published in The Astrophysical Journal, v. 795, no. 2, article 145, p. 1-12.

© 2014. The American Astronomical Society. All rights reserved.

Reproduced by permission of the AAS.

Digital Object Identifier (DOI)

http://dx.doi.org/10.1088/0004-637X/795/2/145

Funding Information

Support for program number HST-GO-12060 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. G.B. acknowledges support from NSF grant AST-08-08133. P.G.P.-G. acknowledges support from grant AYA2012-31277-E. This work has made use of the Rainbow Cosmological Surveys Database, which is operated by the Universidad Complutense de Madrid (UCM), partnered with the University of California Observatories at Santa Cruz (UCO/Lick, UCSC). C.P. is supported by the KASI–Yonsei Joint Research Program (2014) for the Frontiers of Astronomy and Space Science funded by the Korea Astronomy and Space Science Institute. The authors recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.

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