activity
20142018
most citedThe evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point

446 citations · 1.2k across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2018★ 18 cited

Probing the High-Redshift Universe with SPICA: Toward the Epoch of Reionization and Beyond

E. Egami, S. Gallerani, R. Schneider +36

With the recent discovery of a dozen dusty star-forming galaxies and around 30 quasars at z>5 that are hyper-luminous in the infrared ( L, where $μ…

astro-ph.GA2017★ 312 cited

The global dust modelling framework THEMIS (The Heterogeneous dust Evolution Model for Interstellar Solids)

A. P. Jones, M. Koehler, N. Ysard +2

Here we introduce the interstellar dust modelling framework THEMIS (The Heterogeneous dust Evolution Model for Interstellar Solids), which takes a global view of dust and its evolu…

astro-ph.GA2016★ 44 cited

Modeling dust emission in the Magellanic Clouds with Spitzer and Herschel

Jeremy Chastenet, Caroline Bot, Karl D. Gordon +4

Dust modeling is crucial to infer dust properties and budget for galaxy studies. However, there are systematic disparities between dust grain models that result in corresponding sy…

astro-ph.GA2016★ 138 cited

DustPedia - A Definitive Study of Cosmic Dust in the Local Universe

J. I. Davies, M. Baes, S. Bianchi +20

The European Space Agency has invested heavily in two cornerstones missions; Herschel and Planck. The legacy data from these missions provides us with an unprecedented opportunity…

astro-ph.GA2016★ 32 cited

The Herschel Virgo Cluster Survey. XX. Dust and gas in the foreground Galactic cirrus

S. Bianchi, C. Giovanardi, M. W. L. Smith +22

We study the correlation between far-infared/submm dust emission and atomic gas column density in order to derive the properties of the high Galactic latitude, low density, Milky W…

astro-ph.IM2016★ 90 cited

Convolution kernels for multi-wavelength imaging

Alexandre Boucaud, Marco Bocchio, Alain Abergel +3

Astrophysical images issued from different instruments and/or spectral bands often require to be processed together, either for fitting or comparison purposes. However each image i…

astro-ph.GA2015★ 59 cited

The metal and dust yields of the first massive stars

S. Marassi, R. Schneider, M. Limongi +3

We quantify the role of Population (Pop) III core-collapse supernovae (SNe) as the first cosmic dust polluters. Starting from a homogeneous set of stellar progenitors with masses i…

astro-ph.GA2014★ 446 cited

The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point

A. P. Jones, L. Fanciullo, M. Koehler +4

Context. The evolution of amorphous hydrocarbon materials, a-C(:H), principally resulting from ultraviolet (UV) photon absorption- induced processing, are likely at the heart of th…

astro-ph.GA2014★ 54 cited

The cycling of carbon into and out of dust

Anthony P. Jones, Nathalie Ysard, Melanie Koehler +5

Observational evidence seems to indicate that the depletion of interstellar carbon into dust shows rather wide variations and that carbon undergoes rather rapid recycling in the in…

astro-ph.GA2014★ 14 cited

The Herschel Fornax Cluster Survey II: FIR properties of optically-selected Fornax cluster galaxies

C. Fuller, J. I. Davies, R. Auld +13

The Fornax Cluster Survey (HeFoCS) is a deep, far-infrared (FIR) survey of the Fornax cluster. The survey is in 5 bands (100 - 500 m) and covers an area of…