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20152025
most citedKiloparsec-scale gaseous clumps and star formation at

157 citations · 362 across the 7 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2023

Identification and Characterization of Six Spectroscopically Confirmed Massive Protostructures at

Ekta A. Shah, Brian Lemaux, Benjamin Forrest +22

We present six spectroscopically confirmed massive protostructures, spanning a redshift range of in the Extended Chandra Deep Field South (ECDFS) field discovered as pa…

astro-ph.GA2017★ 157 cited

Kiloparsec-scale gaseous clumps and star formation at

S. Carniani, R. Maiolino, R. Amorin +13

We investigate the morphology of the [CII] emission in a sample of "normal" star-forming galaxies at in relation to their UV (rest-frame) counterpart. We use new ALMA obs…

astro-ph.GA2017★ 96 cited

The Lyman Continuum escape fraction of faint galaxies at z~3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC

A. Grazian, E. Giallongo, D. Paris +41

The reionization of the Universe is one of the most important topics of present day astrophysical research. The most plausible candidates for the reionization process are star-form…

astro-ph.GA2016★ 57 cited

New constraints on the average escape fraction of Lyman continuum radiation in z~4 galaxies from the VIMOS Ultra Deep Survey (VUDS)

F. Marchi, L. Pentericci, L. Guaita +20

Determining the average fraction of Lyman continuum (LyC) photons escaping high redshift galaxies is essential for understanding how reionization proceeded in the z>6 Universe. We…

astro-ph.GA2015

Limits on Lyman Continuum escape from z=2.2 H-alpha emitting galaxies

A. Sandberg, G. Östlin, J. Melinder +2

The leakage of Lyman continuum photons from star forming galaxies is an elusive parameter. When observed, it provides a wealth of information on star formation in galaxies and the…

astro-ph.GA2015★ 48 cited

The Lyman alpha reference sample: IV. Morphology at low and high redshift

L. Guaita, J. Melinder, M. Hayes +3

We measured the sizes and morphological parameters of LARS galaxies in the continuum, Lya, and Ha images. We studied morphology by using the Gini coefficient vs M20 and asymmetry v…