P
Pierre Royer
Researcher at Katholieke Universiteit Leuven
Publications - 146
Citations - 10750
Pierre Royer is an academic researcher from Katholieke Universiteit Leuven. The author has contributed to research in topics: Stars & Asymptotic giant branch. The author has an hindex of 40, co-authored 144 publications receiving 9873 citations. Previous affiliations of Pierre Royer include University of Liège.
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Journal ArticleDOI
The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory
Albrecht Poglitsch,C. Waelkens,Norbert Geis,Helmut Feuchtgruber,B. Vandenbussche,L. Rodriguez,Oliver Krause,Etienne Renotte,C. Van Hoof,P. Saraceno,J. Cepa,Franz Kerschbaum,P. Agnese,Babar Ali,Bruno Altieri,Paola Andreani,J.-L. Augueres,Zoltan Balog,L. Barl,Otto H. Bauer,N. Belbachir,M. Benedettini,N. Billot,O. Boulade,Horst Bischof,Joris Blommaert,E. Callut,C. Cara,R. Cerulli,D. Cesarsky,Alessandra Contursi,Ybe Creten,W. De Meester,V. Doublier,E. Doumayrou,L. Duband,Katrina Exter,Reinhard Genzel,Jean-Marie Gillis,Ulrich Grözinger,Thomas Henning,J. M. Herreros,Rik Huygen,Massimo Inguscio,Gerhard Jakob,Claude Jamar,C. Jean,J. de Jong,Reinhard O. Katterloher,Csaba Kiss,Ulrich Klaas,Dietrich Lemke,Dieter Lutz,Suzanne C. Madden,Benoit Marquet,J. Martignac,A. Mazy,Patrick Merken,Francis Montfort,L. Morbidelli,Thomas Müller,Markus Nielbock,K. Okumura,R. Orfei,Roland Ottensamer,Roland Ottensamer,Stefano Pezzuto,Paola Popesso,Jan Putzeys,S. Regibo,V. Reveret,Pierre Royer,Marc Sauvage,Jürgen Schreiber,Jutta Stegmaier,D. Schmitt,J. Schubert,E. Sturm,M. Thiel,G. Tofani,R. Vavrek,M. Wetzstein,E. Wieprecht,Erich Wiezorrek +83 more
TL;DR: The Photodetector Array Camera and Spectrometer (PACS) as discussed by the authors is one of the three science instruments on ESA's far infrared and sub-mil- limetre observatory.
Journal ArticleDOI
From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey
Ph. André,Alexander Men'shchikov,Sylvain Bontemps,Vera Könyves,Frédérique Motte,Nicola Schneider,P. Didelon,Vincent Minier,Paolo Saraceno,Derek Ward-Thompson,J. Di Francesco,Glenn J. White,Glenn J. White,Sergio Molinari,Leonardo Testi,Alain Abergel,Matthew Joseph Griffin,Th. Henning,Pierre Royer,Bruno Merín,R. Vavrek,M. Attard,Doris Arzoumanian,C. D. Wilson,Peter A. R. Ade,Herve Aussel,J.-P. Baluteau,Milena Benedettini,J.-Ph. Bernard,Joris Blommaert,L. Cambrésy,Pierre Cox,A. Di Giorgio,Peter Charles Hargrave,Martin Hennemann,Maohai Huang,Jason M. Kirk,Oliver Krause,Ralf Launhardt,S. J. Leeks,J. Le Pennec,Jin-Zeng Li,Peter G. Martin,Anaëlle Maury,Göran Olofsson,Alain Omont,Nicolas Peretto,Stefano Pezzuto,Timo Prusti,Helene Roussel,D. Russeil,Marc Sauvage,Bruce Sibthorpe,Aurora Sicilia-Aguilar,L. Spinoglio,C. Waelkens,Adam Woodcraft,Annie Zavagno +57 more
TL;DR: In this paper, the first results from the Gould Belt survey, obtained toward the Aquila Rift and Polaris Flare regions during the'science demonstration phase' of Herschel, were summarized.
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,Leonardo Testi,Annie Zavagno,Alain Abergel,Babar Ali,L. D. Anderson,Ph. André,J.-P. Baluteau,Cara Battersby,M. T. Beltrán,M. Benedettini,N. Billot,J. A. D. L. Blommaert,Sylvain Bontemps,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,Douglas 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. G. Müller,Paolo Natoli,J. Neves,Luca Olmi,Roberta Paladini,Deborah Paradis,Harriet Parsons,Nicolas Peretto,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,Paolo Saraceno,Marc Sauvage,Peter Schilke,Eugenio Schisano,Nicola Schneider,Frederic Schuller,Benjamin L. Schulz,B. Sibthorpe,Hazel Smith,Michael D. Smith,L. Spinoglio,Dimitrios Stamatellos,Francesco Strafella,Guy S. Stringfellow,E. Sturm,R. Taylor,Mark 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,Harold W. Yorke,Qizhou Zhang +126 more
TL;DR: In this paper, the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key program that will map the inner Galactic plane of the Milky Way in 5 bands, were presented.
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.