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THE DEAD SEQUENCE: A CLEAR BIMODALITY IN GALAXY COLORS FROM z = 0 to z = 2.5

Journal Article · · Astrophysical Journal (Online)
; ; ; ; ;  [1];  [2]; ;  [3];  [4];  [5];  [6]
  1. Department of Astronomy, Yale University, New Haven, CT 06520 (United States)
  2. Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)
  3. Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA, Leiden (Netherlands)
  4. Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)
  5. UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States)
  6. University of Kansas, Department of Physics and Astronomy, Malott room 1082, 1251 Wescoe Hall Drive, Lawrence, KS 66045 (United States)

We select 25,000 galaxies from the NEWFIRM Medium Band Survey (NMBS) to study the rest-frame U - V color distribution of galaxies at 0 < z approx< 2.5. The five unique NIR filters of the NMBS enable the precise measurement of photometric redshifts and rest-frame colors for 9900 galaxies at 1 < z < 2.5. The rest-frame U - V color distribution at all z approx< 2.5 is bimodal, with a red peak, a blue peak, and a population of galaxies in between (the green valley). Model fits to the optical-NIR spectral energy distributions and the distribution of MIPS-detected galaxies indicate that the colors of galaxies in the green valley are determined largely by the amount of reddening by dust. This result does not support the simplest interpretation of green valley objects as a transition from blue star forming to red quiescent galaxies. We show that correcting the rest-frame colors for dust reddening allows a remarkably clean separation between the red and blue sequences up to z approx 2.5. Our study confirms that dusty-starburst galaxies can contribute a significant fraction to red-sequence samples selected on the basis of a single rest-frame color (i.e., U - V), so extra care must be taken if samples of truly 'red and dead' galaxies are desired. Interestingly, of galaxies detected at 24 mum, 14% remain on the red sequence after applying the reddening correction.

OSTI ID:
21378147
Journal Information:
Astrophysical Journal (Online), Journal Name: Astrophysical Journal (Online) Journal Issue: 1 Vol. 706; ISSN 1538-4357
Country of Publication:
United States
Language:
English