S
Suzanne C. Madden
Researcher at Paris Diderot University
Publications - 76
Citations - 5952
Suzanne C. Madden is an academic researcher from Paris Diderot University. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 39, co-authored 76 publications receiving 5443 citations. Previous affiliations of Suzanne C. Madden include University of Paris-Sud & University of Paris.
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Journal ArticleDOI
The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types
Ilse De Looze,Diane Cormier,Vianney Lebouteiller,Suzanne C. Madden,Maarten Baes,George J. Bendo,Médéric Boquien,Alessandro Boselli,David L. Clements,Luca Cortese,Luca Cortese,Asantha Cooray,Asantha Cooray,Maud Galametz,Frédéric Galliano,Javier Graciá-Carpio,K. G. Isaak,O. Ł. Karczewski,T. J. Parkin,Eric W. Pellegrini,Aurélie Rémy-Ruyer,Luigi Spinoglio,Matthew Smith,Eckhard Sturm +23 more
TL;DR: In this paper, the authors analyzed the applicability of far-infrared fine-structure lines [Cii] 158μm, [Oi] 63μm and [Oiii] 88μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity dwarf galaxies from the Herschel Dwarf Galaxy Survey and furthermore, extended the analysis to a broad sample of galaxies of various types and metallicities in the literature.
Journal ArticleDOI
OBSERVATIONS OF Arp 220 USING HERSCHEL-SPIRE: AN UNPRECEDENTED VIEW OF THE MOLECULAR GAS IN AN EXTREME STAR FORMATION ENVIRONMENT
Naseem Rangwala,Philip R. Maloney,Jason Glenn,C. D. Wilson,A. Rykala,Kate Gudrun Isaak,Maarten Baes,George J. Bendo,Alessandro Boselli,Charles M. Bradford,David L. Clements,Asantha Cooray,Trevor Fulton,P. Imhof,Julia Kamenetzky,Suzanne C. Madden,Erin Mentuch,N. Sacchi,Marc Sauvage,Maximilien R. P. Schirm,Matthew Smith,Luigi Spinoglio,Mark G. Wolfire +22 more
TL;DR: In this paper, the Herschel Spectral and Photometric Imaging Receiver Fourier Transform Spectrometer (Herschel SPIRE-FTS) observations of Arp 220, a nearby ultra-luminous infrared galaxy, were presented.
Journal ArticleDOI
The Herschel Reference Survey
Alessandro Boselli,Stephen Anthony Eales,Luca Cortese,George J. Bendo,P. Chanial,V. Buat,Jonathan Ivor Davies,Robbie Richard Auld,E. E. Rigby,Maarten Baes,M. J. Barlow,James J. Bock,M. Bradford,N. Castro-Rodriguez,Stephane Charlot,David L. Clements,Diane Cormier,E. Dwek,D. Elbaz,Maud Galametz,Frédéric Galliano,Walter Kieran Gear,Jason Glenn,Haley Louise Gomez,Matthew Joseph Griffin,Sacha Hony,Kate Gudrun Isaak,Louis Levenson,Nanyao Y. Lu,Suzanne C. Madden,B. O'Halloran,K. Okamura,S. J. Oliver,Mat Page,P. Panuzzo,Andreas Papageorgiou,T. J. Parkin,Ismael Perez-Fournon,Michael Pohlen,N. Rangwala,Helene Roussel,A. Rykala,N. Sacchi,Marc Sauvage,Benjamin L. Schulz,Maximilien R. P. Schirm,Matthew Smith,L. Spinoglio,Jamie Stevens,M. Symeonidis,Mattia Vaccari,L. Vigroux,Christine D. Wilson,Herve Wozniak,G. Wright,Werner W. Zeilinger +55 more
TL;DR: The Herschel Reference Survey (HRS) as discussed by the authors is a key project of the Herschel guaranteed time key project and will be a benchmark study of dust in the nearby universe.
Journal ArticleDOI
The Herschel Reference Survey
Alessandro Boselli,Stephen Anthony Eales,Luca Cortese,George J. Bendo,P. Chanial,V. Buat,Jonathan Ivor Davies,Robbie Richard Auld,E. E. Rigby,Maarten Baes,M. J. Barlow,James J. Bock,M. Bradford,N. Castro-Rodriguez,Stephane Charlot,David L. Clements,Diane Cormier,E. Dwek,D. Elbaz,Maud Galametz,Frédéric Galliano,Walter Kieran Gear,Jason Glenn,Haley Louise Gomez,Matthew Joseph Griffin,Sacha Hony,K. G. Isaak,Louis Levenson,Nanyao Y. Lu,Suzanne C. Madden,B. O'Halloran,K. Okumura,S. J. Oliver,Mat Page,P. Panuzzo,Andreas Papageorgiou,T. J. Parkin,Ismael Perez-Fournon,Michael Pohlen,N. Rangwala,Helene Roussel,A. Rykala,N. Sacchi,Marc Sauvage,Benjamin L. Schulz,Maximilien R. P. Schirm,Matthew Smith,L. Spinoglio,Jamie Stevens,M. Symeonidis,Mattia Vaccari,L. Vigroux,Christine D. Wilson,Herve Wozniak,G. Wright,Werner W. Zeilinger +55 more
TL;DR: The Herschel Reference Survey (HRS) as mentioned in this paper is a guaranteed time Herschel key project and will be a benchmark study of dust in the nearby universe and will complement a number of other HRS key projects including large cosmological surveys.
Journal ArticleDOI
The state of the gas and the relation between gas and star formation at low metallicity: the small magellanic cloud
Alberto D. Bolatto,Adam K. Leroy,Katherine Jameson,Eve C. Ostriker,Karl D. Gordon,Brandon Lawton,Snezana Stanimirovic,Frank P. Israel,Suzanne C. Madden,Sacha Hony,Karin Sandstrom,Caroline Bot,Monica Rubio,P. Frank Winkler,Julia Roman-Duval,Jacco Th. van Loon,Joana M. Oliveira,Remy Indebetouw,Remy Indebetouw +18 more
TL;DR: In this article, the authors compare atomic gas, molecular gas, and the recent star formation rate (SFR) inferred from H{alpha} in the Small Magellanic Cloud (SMC) by using infrared dust emission and local dust-to-gas ratios.