Results 21 to 30 of about 262,930 (273)

Characterizing Extreme Emission Line Galaxies. II. A Self-consistent Model of Their Ionizing Spectrum [PDF]

open access: yesAstrophysical Journal, 2021
Observations of high-redshift galaxies (z > 5) have shown that these galaxies have extreme emission lines with equivalent widths much larger than their local star-forming counterparts.
G. Olivier   +5 more
semanticscholar   +1 more source

A 16 deg2 survey of emission-line galaxies at z < 1.6 from HSC-SSP PDR2 and CHORUS [PDF]

open access: bronze, 2020
We have conducted a comprehensive survey of emission-line galaxies at $z\lesssim1.6$ based on narrowband (NB) imaging data taken with Hyper Suprime-Cam (HSC) on the Subaru telescope.
Masao Hayashi   +9 more
openalex   +3 more sources

The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: exploring the halo occupation distribution model for emission line galaxies [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2020
We study the modelling of the halo occupation distribution (HOD) for the eBOSS DR16 emission line galaxies (ELGs). Motivated by previous theoretical and observational studies, we consider different physical effects that can change how ELGs populate ...
S. Ávila   +27 more
semanticscholar   +1 more source

The galaxy–halo connection of emission-line galaxies in IllustrisTNG [PDF]

open access: yes, 2020
We employ the hydrodynamical simulation IllustrisTNG-300-1 to explore the halo occupation distribution (HOD) and environmental dependence of luminous star-forming emission-line galaxies (ELGs) at $z \sim 1$.
B. Hadzhiyska   +3 more
semanticscholar   +1 more source

Do model emission line galaxies live in filaments at z ∼ 1? [PDF]

open access: yes, 2020
Current and future cosmological surveys are targeting star-forming galaxies at $z\sim 1$ with nebular emission lines. We use a state-of-the-art semi-analytical model of galaxy formation and evolution to explore the large scale environment of star-forming
V. Gonzalez-Perez   +10 more
semanticscholar   +1 more source

OMEGA: OSIRIS Mapping of Emission-Line Galaxies in A901/2 [PDF]

open access: greenProceedings of the International Astronomical Union, 2014
This work presents the first results from an ESO Large Programme carried out using the OSIRIS instrument on the 10m GTC telescope (La Palma). We have observed a large sample of galaxies in the region of the Abell 901/902 system (z∼0.165) which has been ...
Bruno Rodríguez Del Pino   +4 more
openalex   +2 more sources

The chemical composition of metal-poor emission-line galaxies in the Data Release 3 of the Sloan Digital Sky Survey [PDF]

open access: bronze, 2006
We have re-evaluated empirical expressions for the abundance determination of N, O, Ne, S, Cl, Ar and Fe taking into account the latest atomic data and constructing an appropriate grid of photoionization models with state-of-the art model atmospheres ...
Y. I. Izotov   +8 more
openalex   +3 more sources

The Circumgalactic Medium of eBOSS Emission Line Galaxies: Signatures of Galactic Outflows in Gas Distribution and Kinematics [PDF]

open access: yesAstrophysical Journal, 2018
We study the distribution and kinematics of the cool circumgalactic medium (CGM) of emission line galaxies (ELGs) traced by metal absorption lines. Using about 200,000 ELGs from SDSS-IV eBOSS and half a million background quasars from SDSS, we measure ...
Ting-Wen Lan, H. Mo
semanticscholar   +1 more source

Extreme emission line galaxies detected in JADES JWST/NIRSpec I: inferred galaxy properties [PDF]

open access: yesMonthly notices of the Royal Astronomical Society
Extreme emission line galaxies (EELGs) exhibit large equivalent widths (EW) in their rest-optical emission lines ([OIII]λ5007 or Hα rest-frame EW>750Å) which can be tied to a recent upturn in star formation rate (SFR), due to the sensitivity of the ...
K. Boyett   +35 more
semanticscholar   +1 more source

Machine-learning Classifiers for Intermediate Redshift Emission-line Galaxies [PDF]

open access: yesAstrophysical Journal, 2019
Classification of intermediate redshift (z = 0.3–0.8) emission line galaxies as star-forming galaxies, composite galaxies, active galactic nuclei (AGNs), or low-ionization nuclear emission regions (LINERs) using optical spectra alone was impossible ...
Kai Zhang   +7 more
semanticscholar   +1 more source

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