activity
20152020
most citedMolecular and atomic gas along and across the main sequence of star-forming galaxies

267 citations · 490 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2020★ 51 cited

JINGLE -- IV. Dust, HI gas and metal scaling laws in the local Universe

I. De Looze, I. Lamperti, A. Saintonge +29

Scaling laws of dust, HI gas and metal mass with stellar mass, specific star formation rate and metallicity are crucial to our understanding of the buildup of galaxies through thei…

astro-ph.GA2019★ 27 cited

JINGLE V: Dust properties of nearby galaxies derived from hierarchical Bayesian SED fitting

Isabella Lamperti, Amélie Saintonge, Ilse De Looze +18

We study the dust properties of 192 nearby galaxies from the JINGLE survey using photometric data in the 22-850micron range. We derive the total dust mass, temperature T and emissi…

astro-ph.GA2019★ 19 cited

JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: II. SCUBA-2 850 μm data reduction and dust flux density catalogues

Matthew W. L. Smith, Christopher J. R. Clark, Ilse De Looze +33

We present the SCUBA-2 850 component of JINGLE, the new JCMT large survey for dust and gas in nearby galaxies, which with 193 galaxies is the largest targeted survey of nearby…

astro-ph.GA2018★ 46 cited

JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: I. Survey overview and first results

Amelie Saintonge, Christine D. Wilson, Ting Xiao +88

JINGLE is a new JCMT legacy survey designed to systematically study the cold interstellar medium of galaxies in the local Universe. As part of the survey we perform 850um continuum…

astro-ph.GA2016★ 267 cited

Molecular and atomic gas along and across the main sequence of star-forming galaxies

A. Saintonge, B. Catinella, L. Cortese +10

We use spectra from the ALFALFA, GASS and COLD GASS surveys to quantify variations in the mean atomic and molecular gas mass fractions throughout the SFR-M* plane and along the mai…

astro-ph.GA2016★ 40 cited

Radiative transfer meets Bayesian statistics: where does a galaxy's [CII] emission come from?

Gioacchino Accurso, Amélie Saintonge, Thomas. G. Bisbas +1

The [CII] 158m emission line can arise in all phases of the ISM, therefore being able to disentangle the different contributions is an important yet unresolved problem when unde…