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Structure and dynamics of high-z galaxies

HST and integral-field spectroscopic observations of star-forming galaxies at cosmic noon provide a view on the spatial distribution of stars, gas and dust, and probe gaseous motions revealing the central gravitational...

Structure and dynamics of high-z galaxies

HST and integral-field spectroscopic observations of star-forming galaxies at cosmic noon provide a view on the spatial distribution of stars, gas and dust, and probe gaseous motions revealing the central gravitational...

Resolved views on early galaxy evolution
Resolved observations of star-forming galaxies at cosmic noon with the Hubble Space Telescope and large ground-based facilities provide a view on the spatial distribution of stars, gas and dust, and probe gaseous motions...
Resolved views on early galaxy evolution
Resolved observations of star-forming galaxies at cosmic noon with the Hubble Space Telescope and large ground-based facilities provide a view on the spatial distribution of stars, gas and dust, and probe gaseous motions...
Cool outflows in MaNGA
This paper investigates the neutral gas phase of galactic winds via the Na I Dλλ5890, 5895Å feature within z ∼ 0.04 MaNGA galaxies and directly compares their incidence and strength to the ionized winds detected within the same...
Incidence, scaling relations and physical conditions of ionized gas outflows in MaNGA
In this work, we investigate the strength and impact of ionized gas outflows within z ∼ 0.04 MaNGA galaxies. We find evidence for outflows in 322 galaxies (⁠12 per cent of the analysed line-emitting sample), 185 of which show...
Incidence, scaling relations and physical conditions of ionized gas outflows in MaNGA
In this work, we investigate the strength and impact of ionized gas outflows within z ∼ 0.04 MaNGA galaxies. We find evidence for outflows in 322 galaxies (⁠12 per cent of the analysed line-emitting sample), 185 of which show...
Cool outflows in MaNGA
This paper investigates the neutral gas phase of galactic winds via the Na I Dλλ5890, 5895Å feature within z ∼ 0.04 MaNGA galaxies and directly compares their incidence and strength to the ionized winds detected within the same...
Galaxy kinematics and mass estimates at z ∼ 1 from ionised gas and stars
We compare ionised gas and stellar kinematics of 16 star-forming galaxies (log (M⋆/M⊙) = 9.7 − 11.2, SFR =6 − 86M⊙/yr) at z ∼ 1 using near-infrared integral field spectroscopy (IFS) of Hα emission from the KMOS3D survey and...
Galaxy kinematics and mass estimates at z ∼ 1 from ionised gas and stars
We compare ionised gas and stellar kinematics of 16 star-forming galaxies (log (M⋆/M⊙) = 9.7 − 11.2, SFR =6 − 86M⊙/yr) at z ∼ 1 using near-infrared integral field spectroscopy (IFS) of Hα emission from the KMOS3D survey and...
Cross-calibration of CO- versus dust-based gas masses and assessment of the <i>dynamical </i>mass budget in <i>Herschel</i>-SDSS Stripe82 galaxies
We present a cross-calibration of CO- and dust-based molecular gas masses at z ≤ 0.2. Our results are based on a survey with the IRAM 30-m telescope collecting CO(1–0) measurements of 78 massive (logM⋆/M⊙> 10) galaxies with...
Cross-calibration of CO- versus dust-based gas masses and assessment of the <i>dynamical </i>mass budget in <i>Herschel</i>-SDSS Stripe82 galaxies
We present a cross-calibration of CO- and dust-based molecular gas masses at z ≤ 0.2. Our results are based on a survey with the IRAM 30-m telescope collecting CO(1–0) measurements of 78 massive (logM⋆/M⊙> 10) galaxies with...
Star-Forming Galaxies at Cosmic Noon
Ever deeper and wider lookback surveys have led to a fairly robust outline of the cosmic star formation history, which culminated around z~2 -- a period often nicknamed "cosmic noon." Our knowledge about star-forming galaxies at...
Star-Forming Galaxies at Cosmic Noon
Ever deeper and wider lookback surveys have led to a fairly robust outline of the cosmic star formation history, which culminated around z~2 -- a period often nicknamed "cosmic noon." Our knowledge about star-forming galaxies at...
First Results from the VIRIAL Survey
We investigate the stellar populations of 25 massive galaxies (${\rm log} [{{M}_{*}}/{{M}_{\odot }}]\geqslant 10.9$) at $1.5\lt z\lt 2$ using data obtained with the K-band Multi-Object Spectrograph (KMOS) on the ESO VLT. Targets...
The Kinematics of Massive Quiescent Galaxies at 1.4 &lt; z &lt;2.1

We study the dynamical properties of massive quiescent galaxies at 1.4 < z < 2.1 using deep Hubble Space Telescope WFC3/F160W imaging and a combination of literature stellar velocity dispersion measurements and new...

First Results from the VIRIAL Survey
We investigate the stellar populations of 25 massive galaxies (${\rm log} [{{M}_{*}}/{{M}_{\odot }}]\geqslant 10.9$) at $1.5\lt z\lt 2$ using data obtained with the K-band Multi-Object Spectrograph (KMOS) on the ESO VLT. Targets...
Millimeter Mapping at z ∼ 1

A randomly chosen star in today's universe is most likely to live in a galaxy with stellar mass between the Milky Way and Andromeda. It remains uncertain, however, how the structural evolution of these bulge-disk systems...

Millimeter Mapping at z ∼ 1

A randomly chosen star in today's universe is most likely to live in a galaxy with stellar mass between the Milky Way and Andromeda. It remains uncertain, however, how the structural evolution of these bulge-disk systems...

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