activity
20112024
most citedDust in the reionization era: ALMA observations of a =8.38 Galaxy

324 citations · 2.5k across the 61 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.GA2021★ 45 cited

The Prevalence of Galaxy Overdensities Around UV-Luminous Lyman Emitters in the Epoch of Reionization

E. Leonova, P. A. Oesch, Y. Qin +19

Before the end of the epoch of reionization, the Hydrogen in the Universe was predominantly neutral. This leads to a strong attenuation of Ly lines of galaxies in th…

astro-ph.GA2021★ 43 cited

Assessing the sources of reionisation: a spectroscopic case study of a 30 lensed galaxy at with Lyα, CIV, MgII, and [NeIII]

Joris Witstok, Renske Smit, Roberto Maiolino +5

We present a detailed spectroscopic analysis of a galaxy at that is, by chance, magnified by gravitational lensing. Only three sources at $z \gtrsi…

astro-ph.GA2021★ 9 cited

ALMA Lensing Cluster Survey: A spectral stacking analysis of [CII] in lensed galaxies

Jean-Baptiste Jolly, Kirsten Knudsen, Nicolas Laporte +14

The properties of galaxies at redshift hold the key to our understanding of the early stages of galaxy evolution and can potentially identify the sources of the ultraviolet r…

astro-ph.GA2021★ 81 cited

Probing Cosmic Dawn : Ages and Star Formation Histories of Candidate 9 Galaxies

N. Laporte, R. A. Meyer, R. S. Ellis +3

We discuss the spectral energy distributions and physical properties of six galaxies whose photometric redshifts suggest they lie beyond a redshift 9. Each was selected on…

astro-ph.GA2021★ 59 cited

ALMA Lensing Cluster Survey: Bright [CII] 158 m Lines from a Multiply Imaged Sub- Galaxy at

Seiji Fujimoto, Masamune Oguri, Gabriel Brammer +31

We present bright [CII] 158 m line detections from a strongly magnified and multiply-imaged () sub- ( = ) Lyman-break gal…

astro-ph.GA2021★ 30 cited

ALMA Lensing Cluster Survey: a strongly lensed multiply imaged dusty system at 6

N. Laporte, A. Zitrin, R. S. Ellis +20

We report the discovery of an intrinsically faint, quintuply-imaged, dusty galaxy MACS0600-z6 at a redshift 6.07 viewed through the cluster MACSJ0600.1-2008 (=0.46). A $\sim…