J
Jean-Paul Baluteau
Researcher at Centre national de la recherche scientifique
Publications - 69
Citations - 8203
Jean-Paul Baluteau is an academic researcher from Centre national de la recherche scientifique. The author has contributed to research in topics: Spectrometer & Spire. The author has an hindex of 27, co-authored 68 publications receiving 7845 citations. Previous affiliations of Jean-Paul Baluteau include University of Provence & Aix-Marseille University.
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Journal ArticleDOI
The Herschel-SPIRE instrument and its in-flight performance
Matthew Joseph Griffin,Alain Abergel,A. Abreu,Peter A. R. Ade,Philippe André,J.-L. Augueres,Tom Babbedge,Y. Bae,T. Baillie,Jean-Paul Baluteau,M. J. Barlow,George J. Bendo,Dominique Benielli,James J. Bock,P. Bonhomme,Drew Brisbin,C. Brockley-Blatt,Martin E. Caldwell,C. Cara,N. Castro-Rodriguez,R. Cerulli,Pierre Chanial,Pierre Chanial,Sina Chen,Eric M. Clark,David L. Clements,L. Clerc,J. Coker,D. Communal,Luca Conversi,Peter Timothy Cox,D. Crumb,C. R. Cunningham,F. Daly,Gary R. Davis,P. De Antoni,J. Delderfield,N. Devin,A. M. di Giorgio,Iris Didschuns,Kjetil Dohlen,M. Donati,A. Dowell,C. D. Dowell,L. Duband,Luc Dumaye,R. J. Emery,Marc Ferlet,D. Ferrand,Jean Fontignie,M. Fox,Alberto Franceschini,Margaret A. Frerking,Trevor Fulton,J. Garcia,R. Gastaud,Walter Kieran Gear,Jason Glenn,A-S Goizel,Douglas Griffin,T. Grundy,S. Guest,L. Guillemet,Peter Charles Hargrave,Martin Harwit,P. Hastings,Evanthia Hatziminaoglou,Evanthia Hatziminaoglou,M. Herman,B. Hinde,Viktor Hristov,Maohai Huang,P. Imhof,Kate Gudrun Isaak,Kate Gudrun Isaak,Ulf E. Israelsson,Rob Ivison,D. E. Jennings,Brian John Kiernan,K. J. King,Andrew E. Lange,William B. Latter,Glenn Laurent,Philippe Laurent,S. J. Leeks,Emmanuel Lellouch,Louis Levenson,Bo Li,Jin-Zeng Li,J. Lilienthal,T. L. Lim,S. J. Liu,N. Lu,Suzanne C. Madden,G. Mainetti,P. Marliani,D. J. McKay,K. Mercier,Sergio Molinari,Huw R. Morris,H. Moseley,Jerry Mulder,M. Mur,David A. Naylor,Hien Nguyen,B. O'Halloran,Seb Oliver,G. Olofsson,Hans Olofsson,R. Orfei,Mat Page,I. Pain,P. Panuzzo,Andreas Papageorgiou,G. Parks,P. Parr-Burman,Alan Pearce,C. P. Pearson,C. P. Pearson,Ismael Perez-Fournon,F. Pinsard,Giampaolo Pisano,Giampaolo Pisano,J. Podosek,Michael Pohlen,Edward Polehampton,Edward Polehampton,D. Pouliquen,D. Rigopoulou,D. Rizzo,Isaac Roseboom,Helene Roussel,Michael Rowan-Robinson,B. K. Rownd,P. Saraceno,Marc Sauvage,Richard S. Savage,Giorgio Savini,Giorgio Savini,Eric Sawyer,Carsten Scharmberg,D. Schmitt,D. Schmitt,Nicola Schneider,Benjamin L. Schulz,Arnold A. Schwartz,Rick Shafer,David L. Shupe,B. Sibthorpe,Sunil Sidher,Alan Smith,Anthony J. Smith,David J. Smith,Locke D. Spencer,Locke D. Spencer,Brian Stobie,Rashmikant V. Sudiwala,K. Sukhatme,Christian Surace,Jamie Stevens,B. M. Swinyard,Markos Trichas,T. Tourette,H. Triou,S. Tseng,Carole Tucker,A. D. Turner,Mattia Vaccari,Ivan Valtchanov,L. Vigroux,L. Vigroux,E. Virique,George M. Voellmer,H. J. Walker,Robyn L. Ward,Timothy James Waskett,M. Weilert,Roger Wesson,Glenn J. White,Glenn J. White,Nicola Jane Whitehouse,Christine D. Wilson,Berend Winter,Adam Woodcraft,Gillian S. Wright,C. K. Xu,Annie Zavagno,Michael Zemcov,L. Zhang,E. Zonca +189 more
TL;DR: The Spectral and Photometric Imaging REceiver (SPIRE) is the Herschel Space Observatory's sub-millimetre camera and spectrometer as discussed by the authors, which is used for image and spectroscopic data acquisition.
Journal ArticleDOI
The Herschel-SPIRE instrument and its in-flight performance
Matthew Joseph Griffin,A. Abergel,A. Abreu,Peter A. R. Ade,Pascale Andre,J.-L. Augueres,Tom Babbedge,Y. Bae,T. Baillie,Jean-Paul Baluteau,M. J. Barlow,George J. Bendo,D. Benielli,James J. Bock,P. Bonhomme,D. Brisbin,C. Brockley-Blatt,Martin E. Caldwell,Christophe Cara,N. Castro-Rodriguez,R. Cerulli,P. Chanial,Sina Chen,Eric M. Clark,David L. Clements,L. Clerc,J. Coker,D. Communal,Luca Conversi,Peter Timothy Cox,D. Crumb,Colin Cunningham,F. Daly,Gary R. Davis,P. De Antoni,J. Delderfield,N. Devin,A. M. di Giorgio,Iris Didschuns,Kjetil Dohlen,M. Donati,A. Dowell,C. D. Dowell,L. Duband,Luc Dumaye,R. J. Emery,Marc Ferlet,D. Ferrand,Jean Fontignie,M. Fox,Alberto Franceschini,Margaret A. Frerking,Trevor Fulton,J. Garcia,R. Gastaud,Walter Kieran Gear,Jason Glenn,A-S Goizel,Douglas Griffin,T. Grundy,S. Guest,L. Guillemet,Peter Charles Hargrave,Martin Harwit,P. Hastings,Evanthia Hatziminaoglou,M. Herman,B. Hinde,V. V. Hristov,Maohai Huang,P. Imhof,K. J. Isaak,Ulf E. Israelsson,Rob Ivison,D. E. Jennings,Brian John Kiernan,K. J. King,Andrew E. Lange,William B. Latter,Glenn Laurent,Philippe Laurent,Sarah Leeks,E. Lellouch,Louis Levenson,Bo Li,Jin-Zeng Li,J. Lilienthal,T. L. Lim,J. Liu,N. Lu,S. C. Madden,G. Mainetti,P. Marliani,D. J. McKay,K. Mercier,Sergio Molinari,Huw R. Morris,H. Moseley,Jerry Mulder,M. Mur +99 more
TL;DR: The Spectral and Photometric Imaging Receiver (SPIRE) as discussed by the authors is the Herschel Space Observatory's submillimetre camera and spectrometer, which is used for scan-mapping, whereby the field of view is scanned across the sky to achieve full spatial sampling and to cover large areas.
Journal ArticleDOI
Clouds, filaments and protostars: the Herschel Hi-GAL Milky Way
Sergio Molinari,B. Swinyard,John Bally,M. J. Barlow,J.-P. Bernard,Paul Martin,Toby J. T. Moore,Alberto Noriega-Crespo,Rene Plume,Leonardo Testi,Annie Zavagno,A. Abergel,Babar Ali,L. D. Anderson,Pascal André,Jean-Paul Baluteau,Cara Battersby,M. T. Beltrán,M. Benedettini,N. Billot,J. A. D. L. Blommaert,Sylvain Bontemps,F. Boulanger,Jan Brand,Christopher M. Brunt,Michael G. Burton,Luca Calzoletti,Sean Carey,Paola Caselli,Riccardo Cesaroni,José Cernicharo,Sukanya Chakrabarti,Antonio Chrysostomou,Martin Cohen,Mathieu Compiegne,P. de Bernardis,G. de Gasperis,A. M. di Giorgio,Davide Elia,F. Faustini,Nicolas Flagey,Yasuo Fukui,Gary A. Fuller,K. Ganga,Pedro García-Lario,Jason Glenn,Paul F. Goldsmith,Matthew Joseph Griffin,Melvin Hoare,Maohai Huang,D. Ikhenaode,C. Joblin,G. Joncas,Mika Juvela,Jason M. Kirk,Guilaine Lagache,Jin-Zeng Li,T. L. Lim,S. D. Lord,Massimo Marengo,D. J. Marshall,Silvia Masi,Fabrizio Massi,Mikako Matsuura,Vincent Minier,Marc-Antoine Miville-Deschenes,L. Montier,L. K. Morgan,Frédérique Motte,Joseph C. Mottram,T. Mueller,Paolo Natoli,J. Neves,Luca Olmi,R. Paladini,D. Paradis,Harriet Parsons,Nicolas Peretto,M. R. Pestalozzi,Stefano Pezzuto,F. Piacentini,Lorenzo Piazzo,D. Polychroni,M. Pomarès,Cristina Popescu,William T. Reach,Isabelle Ristorcelli,Jean-François Robitaille,Thomas P. Robitaille,J. A. Rodón,A. Roy,Pierre Royer,D. Russeil,P. Saraceno,Marc Sauvage,Peter Schilke,Eugenio Schisano,Nicola Schneider,Frederic Schuller,Benjamin L. Schulz,B. Sibthorpe,Howard A. Smith,Michael D. Smith,L. Spinoglio,Dimitrios Stamatellos,Francesco Strafella,Guy S. Stringfellow,E. Sturm,Russell H. Taylor,Maggie A. Thompson,Alessio Traficante,Richard J. Tuffs,Grazia Umana,Luca Valenziano,R. Vavrek,M. Veneziani,Serena Viti,C. Waelkens,Derek Ward-Thompson,Glenn J. White,L. A. Wilcock,Friedrich Wyrowski,H. W. Yorke,Qizhou Zhang +123 more
TL;DR: In this paper, the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key-project that will map the inner Galactic Plane of the Milky Way in 5 bands are presented.
Journal ArticleDOI
Hi-GAL: The Herschel Infrared Galactic Plane Survey
Sergio Molinari,B. Swinyard,John Bally,M. J. Barlow,J.-P. Bernard,Pierrick Martin,Toby J. T. Moore,Alberto Noriega-Crespo,Rene Plume,Leonardo Testi,Annie Zavagno,A. Abergel,Babar Ali,Pascal André,Jean-Paul Baluteau,M. Benedettini,Olivier Berné,N. Billot,J. A. D. L. Blommaert,Sylvain Bontemps,F. Boulanger,Jan Brand,Christopher M. Brunt,Michael G. Burton,L. Campeggio,Sean Carey,Paola Caselli,Riccardo Cesaroni,José Cernicharo,Sukanya Chakrabarti,Antonio Chrysostomou,C. Codella,Martin Cohen,Mathieu Compiegne,C. J. Davis,P. de Bernardis,G. de Gasperis,J. Di Francesco,A. M. di Giorgio,Davide Elia,F. Faustini,J. Fischera,Yasuo Fukui,Gary A. Fuller,K. Ganga,Pedro García-Lario,M. Giard,Giovanna Giardino,Jason Glenn,Paul F. Goldsmith,Matthew Joseph Griffin,Melvin Hoare,Maohai Huang,Biwei Jiang,C. Joblin,G. Joncas,Mika Juvela,Jason M. Kirk,Guilaine Lagache,Jin-Zeng Li,T. L. Lim,S. D. Lord,Philip W. Lucas,B. Maiolo,Massimo Marengo,D. J. Marshall,Silvia Masi,Fabrizio Massi,Mikako Matsuura,C. Meny,Vincent Minier,Marc-Antoine Miville-Deschenes,L. Montier,Frédérique Motte,Thomas G. Müller,Paolo Natoli,J. Neves,Luca Olmi,R. Paladini,D. Paradis,M. R. Pestalozzi,Stefano Pezzuto,F. Piacentini,M. Pomarès,Cristina Popescu,William T. Reach,John Richer,Isabelle Ristorcelli,A. Roy,Pierre Royer,D. Russeil,Paolo Saraceno,Marc Sauvage,Peter Schilke,N. Schneider-Bontemps,Frederic Schuller,B. Schultz,D. S. Shepherd,B. Sibthorpe,Howard A. Smith,Michael D. Smith,L. Spinoglio,Dimitrios Stamatellos,Francesco Strafella,Guy S. Stringfellow,E. Sturm,Russell H. Taylor,Maggie A. Thompson,Richard J. Tuffs,Grazia Umana,Luca Valenziano,R. Vavrek,Serena Viti,C. Waelkens,Derek Ward-Thompson,Glenn J. White,Friedrich Wyrowski,H. W. Yorke,Qizhou Zhang +118 more
TL;DR: Hi-GAL as mentioned in this paper is an open-time key project of the Herschel Space Observatory, which aims to detect the earliest phases of the formation of molecular clouds and high-mass stars.
Journal ArticleDOI
Herschel and SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy at z = 2.3
Rob Ivison,Rob Ivison,A. M. Swinbank,B. Swinyard,Ian Smail,Chris Pearson,Chris Pearson,Dimitra Rigopoulou,Dimitra Rigopoulou,Edward Polehampton,Edward Polehampton,Jean-Paul Baluteau,M. J. Barlow,Andrew Blain,J. J. Bock,J. J. Bock,David L. Clements,Kristen Coppin,Asantha Cooray,A. L. R. Danielson,Eli Dwek,Alastair C. Edge,Alberto Franceschini,Trevor Fulton,Jason Glenn,Matthew Joseph Griffin,Kate Gudrun Isaak,S. J. Leeks,T. L. Lim,David A. Naylor,S. J. Oliver,Mat Page,I. Perez Fournon,I. Perez Fournon,Michael Rowan-Robinson,Giorgio Savini,Douglas Scott,Locke D. Spencer,Ivan Valtchanov,L. Vigroux,Gillian S. Wright +40 more
TL;DR: In this article, a detailed analysis of the far-infrared properties of the bright, lensed, z = 2.3, sub-millimetre-selected galaxy (SMG), SMM 2135-0102 (hereafter SMM J2135), using new observations with Herschel, SCUBA-2 and the Very Large Array (VLA).