Frédéric Galliano
Commissariat à l'énergie atomique et aux énergies alternatives
38 Papers
839 Citations
Frédéric Galliano is an academic researcher from Commissariat à l'énergie atomique et aux énergies alternatives. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 21, co-authored 38 publications. Previous affiliations of Frédéric Galliano include DSM.
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Papers
MIPS 24-160 micron photometry for the Herschel-SPIRE Local Galaxies Guaranteed Time Programs
TL;DR: In this article, an overview of ancillary 24, 70, and 160 micron data from the Multiband Imaging Photometer for Spitzer (MIPS) that are intended to complement the 70-500 micron Herschel Space Observatory photometry data for nearby galaxies obtained by the SPIRE Local Galaxies Guaranteed Time Programs and the Herschel Virgo Cluster Survey is provided.
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The nature of the interstellar medium of the starburst low-metallicity galaxy Haro11: a multi-phase model of the infrared emission
Diane Cormier,V. Lebouteiller,S. C. Madden,N. P. Abel,S. Hony,Frédéric Galliano,Maarten Baes,M. J. Barlow,Asantha Cooray,I. De Looze,Maud Galametz,O. L. Karczewski,T. J. Parkin,Aurelie Remy,Marc Sauvage,Luigi Spinoglio,Christine D. Wilson,Ronin Wu +17 more
TL;DR: In this article, a multi-phase ISM of the IR bright low-metallicity galaxy Haro 11 is described by dissecting the photoionised and photodissociated gas components.
The SAGE-Spec Spitzer Legacy programme: the life-cycle of dust and gas in the Large Magellanic Cloud - Point source classification I: SAGE-Spec - Point source classification I
Paul M. Woods,Joana M. Oliveira,Francisca Kemper,J. Th. van Loon,B. A. Sargent,Mikako Matsuura,Ryszard Szczerba,Kevin Volk,Albert A. Zijlstra,Greg Sloan,Eric Lagadec,Iain McDonald,Olivia Jones,Varoujan Gorjian,Kathleen E. Kraemer,Clio Gielen,Margaret Meixner,Robert Blum,Marta Sewilo,D. Riebel,Bernie Shiao,C.-H. R. Chen,Martha L. Boyer,Remy Indebetouw,Vallia Antoniou,J.-P. Bernard,Martin Cohen,C. Dijkstra,Maud Galametz,Frédéric Galliano,Karl D. Gordon,J. Harris,S. Hony,Joseph L. Hora,Akiko Kawamura,Brandon Lawton,Jarron Leisenring,S. C. Madden,Massimo Marengo,C. McGuire,A. J. Mulia,B. O'Halloran,K. A. G. Olsen,R. Paladini,D. Paradis,William T. Reach,D. Rubin,Karin Sandstrom,Igor Soszyński,Angela Speck,Sundar Srinivasan,Alexander G. G. M. Tielens,E. van Aarle,S. D. Van Dyk,H. Van Winckel,Uma P. Vijh,B. A. Whitney,A. N. Wilkins +57 more
Physical conditions in the gas phases of the giant HII region LMC-N11 unveiled by Herschel - I. Diffuse [CII] and [OIII] emission in LMC-N11B
V. Lebouteiller,Diane Cormier,S. C. Madden,Frédéric Galliano,Remy Indebetouw,N. P. Abel,Marc Sauvage,S. Hony,A. Contursi,Albrecht Poglitsch,Aurelie Remy,Eckhard Sturm,Ronin Wu +12 more
TL;DR: In this paper, the distribution and properties of the ionized gas in the Magellanic clouds were investigated using the Herschel/PACS maps in several tracers, [CII], [OI]63um, 145um, [NII]122um, NII]57um, and [OIII]88um in the HII region N11B in the Large Magellan Cloud.
SPIRE imaging of M82: cool dust in the wind and tidal streams
H. Roussel,Christine D. Wilson,L. Vigroux,K. G. Isaak,Marc Sauvage,S. C. Madden,Robbie Richard Auld,Maarten Baes,M. J. Barlow,G. J. Bendo,J. J. Bock,A. Boselli,M. Bradford,V. Buat,N. Castro-Rodriguez,P. Chanial,Stéphane Charlot,Laure Ciesla,D. L. Clements,Asantha Cooray,Diane Cormier,Luca Cortese,Jonathan Ivor Davies,E. Dwek,Steve Eales,D. Elbaz,M. Galametz,Frédéric Galliano,Walter Kieran Gear,Jason Glenn,Haley Louise Gomez,Matthew Joseph Griffin,S. Hony,Louis Levenson,Nanyao Y. Lu,B. O'Halloran,K. Okumura,Seb Oliver,M. J. Page,P. Panuzzo,Andreas Papageorgiou,T. J. Parkin,I. Perez-Fournon,M. Pohlen,N. Rangwala,E. E. Rigby,A. Rykala,N. Sacchi,Benjamin L. Schulz,Maximilien R. P. Schirm,M. W. L. Smith,Luigi Spinoglio,Jamie Stevens,Sundar Srinivasan,M. Symeonidis,M. Trichas,Mattia Vaccari,Herve Wozniak,Gillian S. Wright,Werner W. Zeilinger +59 more
TL;DR: In this paper, the far-infrared emission of the starburst and underlying disk from the SPIRE maps was derived, and spatially-resolved farinfrared colors for the wind and halo were derived in terms of dust mass, dust temperature and global physical conditions.