activity
20172020
most citedDust Properties of [CII] Detected z 5.5 Galaxies: New HST/WFC3 Near-IR Observations

62 citations · 173 across the 5 of their papers we have counts for

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9 papers · 1 filter

astro-ph.GA2020

The ALMA Spectroscopic Survey in the HUDF: CO Excitation and Atomic Carbon in Star-Forming Galaxies at

Leindert A. Boogaard, Paul van der Werf, Axel Weiß +15

We investigate the CO excitation and interstellar medium (ISM) conditions in a cold gas mass-selected sample of 22 star-forming galaxies at , observed as part of the A…

astro-ph.GA2020

The ALMA Spectroscopic Survey in the HUDF: Constraining the Molecular Content at with CO stacking of MUSE detected Galaxies

Hanae Inami, Roberto Decarli, Fabian Walter +19

We report molecular gas mass estimates obtained from a stacking analysis of CO line emission in the ALMA Spectroscopic Survey (ASPECS) using the spectroscopic redshifts from the op…

astro-ph.GA2020

The ALMA Spectroscopic Survey in the HUDF: Multi-band constraints on line luminosity functions and the cosmic density of molecular gas

Roberto Decarli, Manuel Aravena, Leindert Boogaard +20

We present a CO and atomic fine-structure line luminosity function analysis using the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS). ASPECS consists of two spat…

astro-ph.GA2020

The Ionised- and Cool-Gas Content of The BR1202-0725 System as seen by MUSE and ALMA

A. B. Drake, F. Walter, M. Novak +7

We present MUSE observations of the gas-rich major-merger BR1202-0725 at z~4.7, which constitutes one of the most overdense fields known in the early Universe. We utilise these dat…

astro-ph.GA202012 cited

The Nature of 500 micron Risers I: SMA Observations

J. Greenslade, D. L. Clements, G. Petitpas +4

We present SMA observations at resolutions from 0.35 to 3 arcseconds of a sample of 34 candidate high redshift dusty star forming galaxies (DSFGs). These sources were selected from…

astro-ph.GA2019

Spectral Energy Distributions of Companion Galaxies to z6 Quasars

C. Mazzucchelli, R. Decarli, E. P. Farina +10

Massive, quiescent galaxies are already observed at redshift , i.e. 1.5 Gyr after the Big Bang. Current models predict them to be formed via massive, gas-rich mergers…