Results 41 to 50 of about 266,062 (301)

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

Finding Peas in the Early Universe with JWST

open access: yesThe Astrophysical Journal Letters, 2023
The Early Release Observations (EROs) of JWST beautifully demonstrate the promise of JWST in characterizing the universe at Cosmic Dawn. We analyze the Near Infrared Spectrograph ERO spectra of three z ∼ 8 galaxies to determine their metallicities, gas ...
James E. Rhoads   +8 more
doaj   +1 more source

Understanding Galaxy Evolution Through Emission Lines [PDF]

open access: yesAnnual Review of Astronomy and Astrophysics, 2019
We review the use of emission lines for understanding galaxy evolution, focusing on excitation source, metallicity, ionization parameter, ISM pressure, and electron density. We discuss the physics, benefits, and caveats of emission line diagnostics, including the effects of theoretical model uncertainties, diffuse ionized gas, and sample selection ...
Kewley, Lisa   +2 more
openaire   +3 more sources

Ionized-gas Metallicity of the Strong [O iii]λ5007 Emission-line Compact Galaxies in the LAMOST Survey

open access: yesThe Astrophysical Journal Supplement Series, 2023
This article reports a sample of 1830 strong [O iii ] λ 5007 emission-line compact galaxies discovered with the LAMOST spectroscopic survey and the photometric catalog of the Sloan Digital Sky Survey.
Siqi Liu   +6 more
doaj   +1 more source

X-ray emission of galaxies with emission lines [PDF]

open access: yesAstronomical School’s Report, 2011
We built new sample of 315 SDSS galaxies which were detected as X-ray sources in 2XMM catalog. On the basis of distribution of relative intensities of emission lines NII [6583] and OIII [5007] we divided objects of the sample into starburst galaxies and galaxies with active nuclei. Also we found distributions of X-ray luminosities of these galaxies.
A. V. Tugay, A. A. Vasylenko
openaire   +4 more sources

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

Beyond BPT: A New Multidimensional Diagnostic Diagram for Classifying Power Sources Tested Using the SAMI Galaxy Survey

open access: yesThe Astrophysical Journal, 2023
Current methods of identifying the ionizing source of nebular emission in galaxies are well defined for the era of single-fiber spectroscopy, but still struggle to differentiate the complex and overlapping ionization sources in some galaxies.
Victor D. Johnston   +13 more
doaj   +1 more source

CLEAR: Spatially Resolved Emission Lines and Active Galactic Nuclei at 0.6 < z < 1.3

open access: yesThe Astrophysical Journal, 2023
We investigate spatially resolved emission-line ratios in a sample of 219 galaxies (0.6 < z < 1.3) detected using the G102 grism on the Hubble Space Telescope Wide Field Camera 3 taken as part of the CANDELS Ly α Emission at Reionization survey to ...
Bren E. Backhaus   +10 more
doaj   +1 more source

Predicting Hα emission-line galaxy counts for future galaxy redshift surveys [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2017
Knowledge of the number density of H$ $ emitting galaxies is vital for assessing the scientific impact of the Euclid and WFIRST missions. In this work we present predictions from a galaxy formation model, Galacticus, for the cumulative number counts of H$ $-emitting galaxies.
A. Merson   +6 more
openalex   +5 more sources

Simulations of High-redshift [O iii] Emitters: Chemical Evolution and Multiline Diagnostics

open access: yesThe Astrophysical Journal, 2023
Recent observations by the James Webb Space Telescope discovered a number of high-redshift galaxies with strong emission lines from doubly ionized oxygen.
Yurina Nakazato   +2 more
doaj   +1 more source

Home - About - Disclaimer - Privacy