De re metallica: the cosmic chemical evolution of galaxies
The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …
abundances, their spatial distribution, and how these scale with various galactic properties …
Understanding galaxy evolution through emission lines
LJ Kewley, DC Nicholls… - Annual Review of …, 2019 - annualreviews.org
We review the use of emission lines for understanding galaxy evolution, focusing on
excitation source, metallicity, ionization parameter, ISM pressure, and electron density. We …
excitation source, metallicity, ionization parameter, ISM pressure, and electron density. We …
Host galaxy properties and offset distributions of fast radio bursts: implications for their progenitors
We present observations and detailed characterizations of five new host galaxies of fast
radio bursts (FRBs) discovered with the Australian Square Kilometre Array Pathfinder …
radio bursts (FRBs) discovered with the Australian Square Kilometre Array Pathfinder …
Nebular continuum and line emission in stellar population synthesis models
Accounting for nebular emission when modeling galaxy spectral energy distributions (SEDs)
is important, as both line and continuum emissions can contribute significantly to the total …
is important, as both line and continuum emissions can contribute significantly to the total …
SDSS IV MaNGA–spatially resolved diagnostic diagrams: a proof that many galaxies are LIERs
We study the spatially resolved excitation properties of the ionized gas in a sample of 646
galaxies using integral field spectroscopy data from the Sloan Digital Sky Survey IV Map** …
galaxies using integral field spectroscopy data from the Sloan Digital Sky Survey IV Map** …
SDSS-IV MaNGA IFS galaxy survey—Survey design, execution, and initial data quality
ABSTRACT The MaNGA Survey (Map** Nearby Galaxies at Apache Point Observatory) is
one of three core programs in the Sloan Digital Sky Survey IV. It is obtaining integral field …
one of three core programs in the Sloan Digital Sky Survey IV. It is obtaining integral field …
A characteristic oxygen abundance gradient in galaxy disks unveiled with CALIFA
We present the largest and most homogeneous catalog of H ii regions and associations
compiled so far. The catalog comprises more than 7000 ionized regions, extracted from 306 …
compiled so far. The catalog comprises more than 7000 ionized regions, extracted from 306 …
A tale of two DIGs: The relative role of H II regions and low-mass hot evolved stars in powering the diffuse ionised gas (DIG) in PHANGS–MUSE galaxies
F Belfiore, F Santoro, B Groves, E Schinnerer… - Astronomy & …, 2022 - aanda.org
We use integral field spectroscopy from the PHANGS–MUSE survey, which resolves the
ionised interstellar medium structure at∼ 50 pc resolution in 19 nearby spiral galaxies, to …
ionised interstellar medium structure at∼ 50 pc resolution in 19 nearby spiral galaxies, to …
Black hole variability and the star formation–active galactic nucleus connection: do all star-forming galaxies host an active galactic nucleus?
We investigate the effect of active galactic nucleus (AGN) variability on the observed
connection between star formation and black hole accretion in extragalactic surveys. Recent …
connection between star formation and black hole accretion in extragalactic surveys. Recent …
CALIFA, the Calar Alto Legacy Integral Field Area survey-IV. Third public data release
This paper describes the third public data release (DR3) of the Calar Alto Legacy Integral
Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public …
Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public …