Probing the physical properties of z = 4.5 Lyα emitters with spitzer

Keely D. Finkelstein, Steven L. Finkelstein, Vithal Tilvi, Sangeeta Malhotra, James E. Rhoads, Norman A. Grogin, Norbert Pirzkal, Arjun Dey, Buell Tomasson Jannuzi, Bahram Mobasher, Sabrina Pakzad, Brett Salmon, Junxian Wang

Research output: Contribution to journalArticle

10 Citations (Scopus)

Abstract

We present the results from a stellar population modeling analysis of a sample of 162 z = 4.5 and 14 z = 5.7 Ly emitting galaxies (LAEs) in the Boötes field, using deep Spitzer/IRAC data at 3.6 and 4.5 μm from the Spitzer Ly Survey, along with Hubble Space Telescope NICMOS and WFC3 imaging at 1.1 and 1.6 μm for a subset of the LAEs. This represents one of the largest samples of high-redshift LAEs imaged with Spitzer IRAC. We find that 30/162 (19%) of the z = 4.5 LAEs and 9/14 (64%) of the z = 5.7 LAEs are detected at ≥3σ in at least one IRAC band. Individual z = 4.5 IRAC-detected LAEs have a large range of stellar mass, from 5 × 108-1011 . One-third of the IRAC-detected LAEs have older stellar population ages of 100 Myr-1 Gyr, while the remainder have ages 8 ) and young (64-570 Myr). We find a correlation between stellar mass and the dust-corrected ultraviolet-based star formation rate (SFR) similar to that at lower redshifts, in that higher mass galaxies exhibit higher SFRs. However, the z = 4.5 LAE correlation is elevated 4-5 times in SFR compared to continuum-selected galaxies at similar redshifts. The exception is the most massive LAEs which have SFRs similar to galaxies at lower redshifts suggesting that they may represent a different population of galaxies than the traditional lower-mass LAEs, perhaps with a different mechanism promoting Ly photon escape.

Original languageEnglish (US)
Article number78
JournalAstrophysical Journal
Volume813
Issue number1
DOIs
StatePublished - Nov 1 2015

Fingerprint

emitters
physical property
physical properties
galaxies
star formation rate
stellar mass
population modeling
Hubble Space Telescope
set theory
escape
dust
continuums
photons
rate

Keywords

  • galaxies: evolution
  • galaxies: high-redshift
  • galaxies: stellar content

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Finkelstein, K. D., Finkelstein, S. L., Tilvi, V., Malhotra, S., Rhoads, J. E., Grogin, N. A., ... Wang, J. (2015). Probing the physical properties of z = 4.5 Lyα emitters with spitzer. Astrophysical Journal, 813(1), [78]. https://doi.org/10.1088/0004-637X/813/1/78

Probing the physical properties of z = 4.5 Lyα emitters with spitzer. / Finkelstein, Keely D.; Finkelstein, Steven L.; Tilvi, Vithal; Malhotra, Sangeeta; Rhoads, James E.; Grogin, Norman A.; Pirzkal, Norbert; Dey, Arjun; Jannuzi, Buell Tomasson; Mobasher, Bahram; Pakzad, Sabrina; Salmon, Brett; Wang, Junxian.

In: Astrophysical Journal, Vol. 813, No. 1, 78, 01.11.2015.

Research output: Contribution to journalArticle

Finkelstein, KD, Finkelstein, SL, Tilvi, V, Malhotra, S, Rhoads, JE, Grogin, NA, Pirzkal, N, Dey, A, Jannuzi, BT, Mobasher, B, Pakzad, S, Salmon, B & Wang, J 2015, 'Probing the physical properties of z = 4.5 Lyα emitters with spitzer', Astrophysical Journal, vol. 813, no. 1, 78. https://doi.org/10.1088/0004-637X/813/1/78
Finkelstein KD, Finkelstein SL, Tilvi V, Malhotra S, Rhoads JE, Grogin NA et al. Probing the physical properties of z = 4.5 Lyα emitters with spitzer. Astrophysical Journal. 2015 Nov 1;813(1). 78. https://doi.org/10.1088/0004-637X/813/1/78
Finkelstein, Keely D. ; Finkelstein, Steven L. ; Tilvi, Vithal ; Malhotra, Sangeeta ; Rhoads, James E. ; Grogin, Norman A. ; Pirzkal, Norbert ; Dey, Arjun ; Jannuzi, Buell Tomasson ; Mobasher, Bahram ; Pakzad, Sabrina ; Salmon, Brett ; Wang, Junxian. / Probing the physical properties of z = 4.5 Lyα emitters with spitzer. In: Astrophysical Journal. 2015 ; Vol. 813, No. 1.
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