SIMBAD references

2007ApJS..172..523M - Astrophys. J., Suppl. Ser., 172, 523-544 (2007/September-0)

Lyα emitters at redshift 5.7 in the COSMOS field.

MURAYAMA T., TANIGUCHI Y., SCOVILLE N.Z., AJIKI M., SANDERS D.B., MOBASHER B., AUSSEL H., CAPAK P., KOEKEMOER A., SHIOYA Y., NAGAO T., CARILLI C., ELLIS R.S., GARILLI B., GIAVALISCO M., KITZBICHLER M.G., LE FEVRE O., MACCAGNI D., SCHINNERER E., SMOLCIC V., TRIBIANO S., CIMATTI A., KOMIYAMA Y., MIYAZAKI S., SASAKI S.S., KODA J. and KAROJI H.

Abstract (from CDS):

We present results from a narrowband optical survey of a contiguous area of 1.95 deg2, covered by the Cosmic Evolution Survey (COSMOS). Both optical narrowband (λc=8150 Å and Δλ=120 Å) and broadband (B, V, g', r', i', and z') imaging observations were performed with the Subaru prime-focus camera, Suprime-Cam on the Subaru Telescope. We provide the largest contiguous narrowband survey, targeting Lyα emitters (LAEs) at z~5.7. We find a total of 119 LAE candidates at z∼5.7. Over the wide-area covered by this survey, we find no strong evidence for large-scale clustering of LAEs. We estimate a star formation rate (SFR) density of ∼7x10–4 M/yr/Mpc3 for LAEs at z~5.7 and compare it with previous measurements.

Abstract Copyright:

Journal keyword(s): Cosmology: Observations - Cosmology: Early Universe - Galaxies: Evolution - Galaxies: Formation

VizieR on-line data: <Available at CDS (J/ApJS/172/523): table1.dat table2.dat>

Nomenclature: Fig.2, Table 1: [MTS2007] NNN (Nos 1-119).

Simbad objects: 121

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2020.08.12-17:47:50

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