papers

Publications (18)

astro-ph.GA2022

Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z>6.5 Universe

R. J. Bouwens, R. Smit, S. Schouws +28

The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA Large Program (LP) that is identifying and performing a first characterization of many of the most lumin…

astro-ph2006

Galaxies Under the Cosmic Microscope: Resolved Spectroscopy and New Constraints on the z=1 Tully-Fisher relation

M. Swinbank, R. Bower, G. P. Smith +5

We exploit the gravitational potential of massive cluster lenses to probe the emission line properties of six z=1 galaxies which appear as highly magnified luminous arcs. Using the…

astro-ph.GA2018

The VANDELS ESO public spectroscopic survey: observations and first data release

L. Pentericci, R. J. McLure B. Garilli, O. Cucciati +93

This paper describes the observations and the first data release (DR1) of the ESO public spectroscopic survey "VANDELS, a deep VIMOS survey of the CANDELS CDFS and UDS fields". VAN…

astro-ph.GA2022

The REBELS ALMA Survey: cosmic dust temperature evolution out to z 7

L. Sommovigo, A. Ferrara, A. Pallottini +27

ALMA observations have revealed the presence of dust in the first generations of galaxies in the Universe. However, the dust temperature remains mostly unconstrained due to t…

astro-ph2004

Spitzer and Hubble Constraints on the Physical Properties of the z~7 Galaxy Strongly Lensed by Abell 2218

E. Egami, J. -P. Kneib, G. H. Rieke +10

We report the detection of a z~7 galaxy strongly lensed by the massive galaxy cluster Abell 2218 (z=0.175) at 3.6 and 4.5 um using the Spitzer Observatory and at 1.1 um using the H…

astro-ph.GA2013

A molecular line scan in the Hubble Deep Field North

R. Decarli, F. Walter, C. Carilli +20

We present a molecular line scan in the Hubble Deep Field North (HDF-N) that covers the entire 3mm window (79-115 GHz) using the IRAM Plateau de Bure Interferometer. Our CO redshif…

astro-ph.CO2012

The Intense Starburst HDF850.1 in a Galaxy Overdensity at z=5.2 in the Hubble Deep Field

Fabian Walter, R. Decarli, C. Carilli +24

The Hubble Deep Field (HDF) is a region in the sky that provides one of the deepest multi-wavelength views of the distant universe and has led to the detection of thousands of gala…

physics.plasm-ph2020

Birefringence in thermally anisotropic relativistic plasmas and its impact on laser-plasma interactions

A. Arefiev, D. Stark, T. Toncian +1

One of the paradigm-shifting phenomena triggered in laser-plasma interactions at relativistic intensities is the so-called relativistic transparency. As the electrons become heated…

cond-mat.mes-hall2018

Room temperature operation of n-type Ge/SiGe terahertz quantum cascade lasers predicted by non-equilibrium Green's functions

T. Grange, D. Stark, G. Scalari +9

n-type Ge/SiGe terahertz quantum cascade laser are investigated using non-equilibrium Green's functions calculations. We compare the temperature dependence of the terahertz gain pr…

astro-ph2005

Evidence for a Massive Post-Starburst Galaxy at z ~ 6.5

B. Mobasher, M. Dickinson, H. C. Ferguson +26

We present results from a search for high-redshift J--band ``dropout'' galaxies in the portion of the GOODS southern field that is covered by extremely deep imaging from the Hubble…

astro-ph.GA2022

The ALMA REBELS Survey: the dust content of Lyman Break Galaxies

P. Dayal, A. Ferrara, L. Sommovigo +22

We include a fully coupled treatment of metal and dust enrichment into the Delphi semi-analytic model of galaxy formation to explain the dust content of 13 Lyman Break Galaxies (LB…

astro-ph.GA2021

Normal, Dust-Obscured Galaxies in the Epoch of Reionization

Y. Fudamoto, P. A. Oesch, S. Schouws +26

Over the past decades, rest-frame ultraviolet (UV) observations have provided large samples of UV luminous galaxies at redshift (z) greater than 6, during the so-called epoch of re…

astro-ph.GA2022

The ALMA REBELS Survey: Average [CII] sizes of Star-Forming Galaxies from to

Y. Fudamoto, R. Smit, R. A. A. Bowler +36

We present the average [CII] emission line sizes of UV-bright star-forming galaxies at . Our results are derived from a stacking analysis of [CII] $158\,\rm…

astro-ph.GA2021

The VANDELS ESO public spectroscopic survey: final Data Release of 2087 spectra and spectroscopic measurements

B. Garilli, R. McLure, L. Pentericci +94

VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we prese…

astro-ph.CO2013

A Molecular Line Scan in the Hubble Deep Field North: Constraints on the CO Luminosity Function and the Cosmic H2 Density

F. Walter, R. Decarli, M. Sargent +19

We present direct constraints on the CO luminosity function at high redshift and the resulting cosmic evolution of the molecular gas density, (z), based on a blind mol…

astro-ph2006

A very bright, highly magnified Lyman-break galaxy at z=3.07

Ian Smail, A. M. Swinbank, J. Richard +8

We report the discovery using Hubble Space Telescope imaging and Keck spectroscopy of a very bright, highly magnified (~30*) Lyman Break Galaxy (LBG) at z=3.07 in the field of the…

astro-ph.GA2015

Mean Halpha+[NII]+[SII] EW Inferred for Star-Forming Galaxies at z=5.1-5.4 Using High-Quality Spitzer/IRAC Photometry

N. Rasappu, R. Smit, I. Labbe +4

Recent Spitzer/InfraRed Array Camera (IRAC) photometric observations have revealed that rest-frame optical emission lines contribute signficantly to the broadband fluxes of high-re…

astro-ph.GA2022

The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at

A. Ferrara, L. Sommovigo, P. Dayal +27

We analyse FIR dust continuum measurements for 14 galaxies () in the ALMA REBELS LP to derive their physical properties. Our model uses three input data: (a) the UV spe…