Lista de obras -

A Search for H-Dropout Lyman Break Galaxies at z ∼ 12–16

artículo científico publicado en 2022

ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z = 7.13

artículo científico publicado en 2022

Big Three Dragons: A [N ii] 122 μm Constraint and New Dust-continuum Detection of a z = 7.15 Bright Lyman-break Galaxy with ALMA

artículo científico publicado en 2021

Large Population of ALMA Galaxies at z > 6 with Very High [O iii] 88 μm to [C ii] 158 μm Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?

artículo científico publicado en 2020

MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M UV ∼ −15 ⬇️

scholarly article

Possible Systematic Rotation in the Mature Stellar Population of a z = 9.1 Galaxy

artículo científico publicado en 2022

Radiative equilibrium estimates of dust temperature and mass in high-redshift galaxies

scientific article published in 2020

Recovering the systemic redshift of galaxies from their Lyman alpha line profile

artículo científico publicado en 2018

The MUSE Hubble Ultra Deep Field Survey

The MUSE Hubble Ultra Deep Field Survey VI. The faint-end of the Lyα luminosity function at 2.91 < z < 6.64 and implications for reionisation

scholarly article

The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies

artículo científico publicado en 2017

The MUSE Hubble Ultra Deep Field Survey. X. Ly{alpha} equivalent widths at 2.9 < z < 6.6

artículo científico publicado en 2017

Lista de obras de

A Search for H-Dropout Lyman Break Galaxies at z ∼ 12–16

ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z = 7.13

Big Three Dragons: A [N ii] 122 μm Constraint and New Dust-continuum Detection of a z = 7.15 Bright Lyman-break Galaxy with ALMA

Large Population of ALMA Galaxies at <i>z</i> > 6 with Very High [O iii] 88 <i>μ</i>m to [C ii] 158 <i>μ</i>m Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?

MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M UV ∼ −15 ⬇️

Possible Systematic Rotation in the Mature Stellar Population of a z = 9.1 Galaxy

Radiative equilibrium estimates of dust temperature and mass in high-redshift galaxies

Recovering the systemic redshift of galaxies from their Lyman alpha line profile

The MUSE Hubble Ultra Deep Field Survey

The MUSE Hubble Ultra Deep Field Survey

The MUSE Hubble Ultra Deep Field Survey VI. The faint-end of the Lyα luminosity function at 2.91 < z < 6.64 and implications for reionisation

The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies

The MUSE Hubble Ultra Deep Field Survey. X. Ly{alpha} equivalent widths at 2.9 < z < 6.6

Lista de obras de

A Search for H-Dropout Lyman Break Galaxies at z ∼ 12–16

ALMA Reveals Extended Cool Gas and Hot Ionized Outflows in a Typical Star-forming Galaxy at Z = 7.13

Big Three Dragons: A [N ii] 122 μm Constraint and New Dust-continuum Detection of a z = 7.15 Bright Lyman-break Galaxy with ALMA

Large Population of ALMA Galaxies at <i>z</i> &gt; 6 with Very High [O iii] 88 <i>μ</i>m to [C ii] 158 <i>μ</i>m Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?

MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with M UV ∼ −15 ⬇️

Possible Systematic Rotation in the Mature Stellar Population of a z = 9.1 Galaxy

Radiative equilibrium estimates of dust temperature and mass in high-redshift galaxies

Recovering the systemic redshift of galaxies from their Lyman alpha line profile

The MUSE Hubble Ultra Deep Field Survey

The MUSE Hubble Ultra Deep Field Survey

The MUSE Hubble Ultra Deep Field Survey VI. The faint-end of the Lyα luminosity function at 2.91 < z < 6.64 and implications for reionisation

The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies

The MUSE Hubble Ultra Deep Field Survey. X. Ly{alpha} equivalent widths at 2.9 < z < 6.6

Large Population of ALMA Galaxies at <i>z</i> > 6 with Very High [O iii] 88 <i>μ</i>m to [C ii] 158 <i>μ</i>m Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?