SIMBAD references

2010MNRAS.402.1580O - Mon. Not. R. Astron. Soc., 402, 1580-1598 (2010/March-1)

Stellar populations of Lyα emitters at z = 3-4 based on deep large area surveys in the Subaru-SXDS/UKIDSS-UDS field.

ONO Y., OUCHI M., SHIMASAKU K., AKIYAMA M., DUNLOP J., FARRAH D., LEE J.C., McLURE R., OKAMURA S. and YOSHIDA M.

Abstract (from CDS):

We investigate the stellar populations of Lyα emitters (LAEs) at z = 3.1 and 3.7 in 0.65 deg2 of the Subaru/XMM-Newton Deep Field, based on rest-frame ultraviolet-to-optical photometry obtained from the Subaru/XMM-Newton Deep Survey, the UKIRT Infrared Deep Sky Survey/Ultra Deep Survey (UKIDSS/UDS), and the Spitzer legacy survey of the UKIDSS/UDS. Among a total of 302 LAEs (224 for z = 3.1 and 78 for z = 3.7), only 11 are detected in the K band, i.e. brighter than K(3σ) = 24.1 mag. Eight of the 11 K-detected LAEs are spectroscopically confirmed. In our stellar population analysis, we treat K-detected objects individually, while K-undetected objects are stacked at each redshift. We find that the K-undetected objects, which should closely represent the LAE population as a whole, have low stellar masses of ∼108-108.5M, modest star formation rates (SFRs) of 1-100M/yr, and modest dust extinction of E(B - V)*< 0.2. The K-detected objects are massive, Mstar∼ 109-1010.5M, and have significant dust extinction with a median of E(B - V)*≃ 0.3. Four K-detected objects with the reddest spectral energy distributions, two of which are spectroscopically confirmed, are heavily obscured with E(B - V)*∼ 0.65, and their continua resemble those of some local ultraluminous infrared galaxies (ULIRGs). Interestingly, they have large Lyα equivalent widths ≃70-250 Å. If these four are excluded, our sample has a weak anticorrelation between Lyα equivalent width and Mstar. We compare the stellar masses and the specific SFRs (sSFRs) of LAEs with those of Lyman-break galaxies (LBGs), distant red galaxies, submillimetre galaxies, and I- or K-selected galaxies with photometric redshifts of zphot∼ 3. We find that the LAE population is the least massive among all the galaxy populations in question, but with relatively high sSFRs, while near-infrared (NIR)-detected LAEs have Mstarand sSFR similar to LBGs. Our reddest four LAEs have very high sSFRs in spite of large Mstar, thus occupying a unique region in the Mstar versus sSFR space.

Abstract Copyright: © 2009 The Authors. Journal compilation © 2009 RAS

Journal keyword(s): galaxies: evolution - galaxies: formation - galaxies: high-redshift - galaxies: stellar content - cosmology: observations

Nomenclature: Table 3: [OOS2010] NBNNN-A-NNNNN N=6. Tables 3-4: [OOS2010] RN (Nos R1-R4).

Simbad objects: 35

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2021.06.24-09:16:02

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