Abstract
In this paper, we follow up on our previous detection of nuclear ionized outflows in the most massive (log(M*/M☉)≥10.9) z∼1-3 star-forming galaxies (SFGs) by increasing the sample size by a factor of six (to 44 galaxies above log(M*/M☉)≥10.9) from a combination of the SINS/zC-SINF, LUCI, GNIRS, and KMOS3D spectroscopic surveys.
For the analysis in this paper, we included a total of 110 SFGs at z∼1-3 with near-IR integral field or slit spectroscopy covering the Hα+[NII] line emission from surveys carried out with SINFONI, KMOS, LUCI, and GNIRS. The targets for these surveys were originally drawn from rest-frame optical, UV, and near-IR selected samples in broadband imaging surveys with optical spectroscopic redshifts, and from stellar mass-selected samples with near-IR or optical spectroscopic redshifts. Show more
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CDS Centré de Données astronomiques des StrasbourgSubject
Galaxies: IR; Redshifts; Spectra, infrared; Galaxies: evolution; Galaxies: high-redshift; Galaxies: kinematics and dynamics; Infrared: galaxiesOrganisational unit
03612 - Carollo, Marcella (ehemalig) / Carollo, Marcella (former)
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Is supplement to: http://hdl.handle.net/20.500.11850/93258
Notes
VizieR Online Data Catalog: J/ApJ/796/7More
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