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E. Giovannoli

Researcher at Aix-Marseille University

Publications -  20
Citations -  3629

E. Giovannoli is an academic researcher from Aix-Marseille University. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 12, co-authored 20 publications receiving 3291 citations.

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The Herschel Multi-tiered Extragalactic Survey: HerMES

Seb Oliver, +120 more
TL;DR: The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy program designed to map a set of nested fields totalling ∼380deg^2 as mentioned in this paper.
Journal ArticleDOI

Analysis of galaxy spectral energy distributions from far-UV to far-IR with CIGALE: studying a SINGS test sample

TL;DR: In this paper, a code CIGALE (Code Investigating GALaxy Emission) that uses model spectra composed of the Maraston (or PEGASE) stellar population models, synthetic attenuation functions based on a modified Calzetti law, spectral line templates, the Dale & Helou dust emission models, and optional spectral templates of obscured AGN is presented.
Journal ArticleDOI

The Herschel Multi-tiered Extragalactic Survey: HerMES

Seb Oliver, +118 more
TL;DR: The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy program designed to map a set of nested fields totalling ~380 deg^2 as mentioned in this paper.
Journal ArticleDOI

Analysis of galaxy SEDs from far-UV to far-IR with CIGALE: Studying a SINGS test sample

TL;DR: In this article, a code CIGALE (Code Investigating GALaxy Emission) that uses model spectra composed of the Maraston (or PEGASE) stellar population models, synthetic attenuation functions based on a modified Calzetti law, spectral line templates, the Dale & Helou dust emission models, and optional spectral templates of obscured AGN.
Journal ArticleDOI

CIGALEMC: Galaxy Parameter Estimation Using a Markov Chain Monte Carlo Approach with CIGALE

TL;DR: A fast Markov Chain Monte Carlo (MCMC) exploration of the astrophysical parameter space using a modified version of the publicly available code CIGALE, which fits to photometric fluxes from Ultraviolet to Infrared to put contraints on parameters related to both formation and evolution of galaxies.