P
Pau Amaro-Seoane
Researcher at Institut de Ciències de l'Espai
Publications - 180
Citations - 12341
Pau Amaro-Seoane is an academic researcher from Institut de Ciències de l'Espai. The author has contributed to research in topics: Gravitational wave & Black hole. The author has an hindex of 47, co-authored 174 publications receiving 10011 citations. Previous affiliations of Pau Amaro-Seoane include Chinese Academy of Sciences & Technical University of Berlin.
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Journal ArticleDOI
The PLATO 2.0 Mission
Heike Rauer,C. Catala,Conny Aerts,T. Appourchaux,Willy Benz,Alexis Brandeker,Jørgen Christensen-Dalsgaard,Magali Deleuil,Laurent Gizon,M. J. Goupil,Manuel Güdel,Eduardo Janot-Pacheco,M. Mas-Hesse,I. Pagano,Giampaolo Piotto,Don Pollacco,Nuno C. Santos,Amanda J. Smith,Suárez,Róbert Szabó,Stéphane Udry,V. Adibekyan,Yann Alibert,J. M. Almenara,Pau Amaro-Seoane,M. Ammler-von Eiff,Martin Asplund,Elio Antonello,Warrick H. Ball,Sydney A. Barnes,F. Baudin,Kevin Belkacem,Maria Bergemann,G. Bihain,Aaron C. Birch,Xavier Bonfils,Isabelle Boisse,Aldo S. Bonomo,Francesco Borsa,I. M. Brandão,Enzo Brocato,S. Brun,Matthew R. Burleigh,R. Burston,Juan Cabrera,Santi Cassisi,William J. Chaplin,Stéphane Charpinet,Cristina Chiappini,Ross P. Church,Sz. Csizmadia,Margarida S. Cunha,Mario Damasso,Melvyn B. Davies,Hans J. Deeg,Rodrigo F. Díaz,S. Dreizler,C. Dreyer,P. Eggenberger,David Ehrenreich,Philipp Eigmüller,Anders Erikson,Robert Farmer,Sofia Feltzing,F. De Oliveira Fialho,P. Figueira,T. Forveille,M. Fridlund,Rafael A. García,Paolo Giommi,G. Giuffrida,M Godolt,J. Gomes da Silva,T. Granzer,John Lee Grenfell,A. Grotsch-Noels,E. Günther,Carole A. Haswell,A. P. Hatzes,G. Hebrard,Saskia Hekker,Ravit Helled,Kevin Heng,Jon M. Jenkins,Anders Johansen,Maxim L. Khodachenko,Kristina G. Kislyakova,Wilhelm Kley,Ulrich Kolb,Natalie A. Krivova,Friedrich Kupka,Helmut Lammer,Antonino F. Lanza,Yveline Lebreton,Demetrio Magrin,P. Marcos-Arenal,P. M. Marrese,J. P. Marques,J. H. C. Martins,Stéphane Mathis,Savita Mathur,S. Messina,Andrea Miglio,Josefina Montalbán,M. Montalto,Mário J. P. F. G. Monteiro,Hamed Moradi,Ehsan Moravveji,Christoph Mordasini,Thierry Morel,Annelies Mortier,Valerio Nascimbeni,Richard P. Nelson,Martin Bo Nielsen,Lena Noack,Andrew Norton,Aviv Ofir,Mahmoudreza Oshagh,R. M. Ouazzani,Péter Pápics,V. C. Parro,Pascal Petit,Bertrand Plez,E. Poretti,A. Quirrenbach,Roberto Ragazzoni,Gabriella Raimondo,Monica Rainer,Daniel R. Reese,Ronald Redmer,Sabine Reffert,Bárbara Rojas-Ayala,Ian W. Roxburgh,S. Salmon,Alexandre Santerne,Jean Schneider,Jesper Schou,Sonja Schuh,Hannah Schunker,A. Silva-Valio,Roberto Silvotti,I. Skillen,Ignas Snellen,Frank Sohl,S. G. Sousa,Alessandro Sozzetti,Dennis Stello,Klaus G. Strassmeier,Michal Švanda,Gy. M. Szabó,Andrew Tkachenko,Diana Valencia,Valérie Van Grootel,Sylvie Vauclair,Paolo Ventura,F. W. Wagner,N. A. Walton,J. Weingrill,Stephanie C. Werner,Peter J. Wheatley,Konstanze Zwintz +160 more
TL;DR: The PLATO 2.0 instrument consists of 34 small aperture telescopes (32 with 25 sec readout cadence and 2 with 2.5 sec candence) providing a wide field-of-view (2232 deg2) and a large photometric magnitude range (4-16 mag) as discussed by the authors.
Journal ArticleDOI
The PLATO 2.0 mission
Heike Rauer,Heike Rauer,C. Catala,Conny Aerts,Thierry Appourchaux,Willy Benz,Alexis Brandeker,Jørgen Christensen-Dalsgaard,Magali Deleuil,Laurent Gizon,Laurent Gizon,M. J. Goupil,Manuel Güdel,Eduardo Janot-Pacheco,M. Mas-Hesse,Isabella Pagano,Giampaolo Piotto,Don Pollacco,Ċ. Santos,Andrew Smith,Juan Carlos Suárez,Róbert Szabó,Stéphane Udry,V. Adibekyan,Yann Alibert,J. M. Almenara,Pau Amaro-Seoane,M. Ammler-von Eiff,Martin Asplund,E. Antonello,Sydney A. Barnes,Frédéric Baudin,K. Belkacem,Maria Bergemann,G. Bihain,Aaron C. Birch,Xavier Bonfils,Isabelle Boisse,Aldo S. Bonomo,Francesco Borsa,I. M. Brandão,Enzo Brocato,S. Brun,Matthew R. Burleigh,R. Burston,Juan Cabrera,Santi Cassisi,William J. Chaplin,Stéphane Charpinet,Cristina Chiappini,Ross P. Church,Sz. Csizmadia,Margarida S. Cunha,Mario Damasso,Mario Damasso,Melvyn B. Davies,Hans J. Deeg,Rodrigo F. Díaz,Stefan Dreizler,C. Dreyer,C. Dreyer,P. Eggenberger,David Ehrenreich,Philipp Eigmüller,Anders Erikson,Robert Farmer,Sofia Feltzing,F. De Oliveira Fialho,Pedro Figueira,T. Forveille,Malcolm Fridlund,Rafael A. García,Paolo Giommi,G. Giuffrida,G. Giuffrida,M. Godolt,J. Gomes da Silva,T. Granzer,John Lee Grenfell,A. Grotsch-Noels,E. Günther,Carole A. Haswell,A. P. Hatzes,Guillaume Hébrard,Saskia Hekker,Saskia Hekker,Ravit Helled,Kevin Heng,Jon M. Jenkins,Anders Johansen,Maxim L. Khodachenko,Kristina G. Kislyakova,Wilhelm Kley,Ulrich Kolb,Natalie A. Krivova,Friedrich Kupka,Helmut Lammer,Antonino F. Lanza,Yveline Lebreton,Demetrio Magrin,P. Marcos-Arenal,P. M. Marrese,P. M. Marrese,J. P. Marques,J. H. C. Martins,S. Mathis,Savita Mathur,S. Messina,Andrea Miglio,Josefina Montalbán,M. Montalto,Mário J. P. F. G. Monteiro,Hamed Moradi,Ehsan Moravveji,Christoph Mordasini,Thierry Morel,Annelies Mortier,Valerio Nascimbeni,Richard P. Nelson,Martin Bo Nielsen,Lena Noack,Andrew Norton,Aviv Ofir,Mahmoudreza Oshagh,R.-M. Ouazzani,Péter Pápics,V. C. Parro,Pascal Petit,Bertrand Plez,Ennio Poretti,Andreas Quirrenbach,Roberto Ragazzoni,Giuliano Raimondo,Monica Rainer,Daniel R. Reese,Ronald Redmer,Sabine Reffert,Bárbara Rojas-Ayala,Ian W. Roxburgh,Stéphanie Salmon,Alexandre Santerne,Jean Schneider,Jesper Schou,Sonja Schuh,Hannah Schunker,A. Silva-Valio,Roberto Silvotti,I. Skillen,Ignas Snellen,Frank Sohl,S. G. Sousa,Alessandro Sozzetti,Dennis Stello,Klaus G. Strassmeier,Michal Švanda,Gy. M. Szabó,Gy. M. Szabó,Andrew Tkachenko,Diana Valencia,Valérie Van Grootel,Sylvie Vauclair,Paolo Ventura,F. W. Wagner,N. A. Walton,Joerg Weingrill,Stephanie C. Werner,Peter J. Wheatley,Konstanze Zwintz +167 more
TL;DR: The PLATO 2.0 mission as discussed by the authors has been selected for ESA's M3 launch opportunity (2022/24) to provide accurate key planet parameters (radius, mass, density and age) in statistical numbers.
Laser Interferometer Space Antenna
Pau Amaro-Seoane,Heather Audley,Stanislav Babak,John M. Baker,Enrico Barausse,Peter L. Bender,Emanuele Berti,Pierre Binétruy,M. Born,Daniele Bortoluzzi,Jordan Camp,Chiara Caprini,Vitor Cardoso,Monica Colpi,John Conklin,Neil J. Cornish,Curt Cutler,Karsten Danzmann,Rita Dolesi,Luigi Ferraioli,Valerio Ferroni,Ewan Fitzsimons,Jonathan R. Gair,Lluis Gesa Bote,Domenico Giardini,Ferran Gibert,Catia Grimani,Hubert Halloin,Gerhard Heinzel,Thomas Hertog,Martin Hewitson,Kelly Holley-Bockelmann,Daniel Hollington,Mauro Hueller,Henri Inchauspe,Philippe Jetzer,N. Karnesis,Christian J. Killow,Antoine Klein,Bill Klipstein,N. Korsakova,Shane L. Larson,Jeffrey Livas,Ivan Lloro,Nary Man,Davor Mance,J. Martino,Ignacio Mateos,Kirk McKenzie,Sean T. McWilliams,Cole Miller,Guido Mueller,Germano Nardini,Gijs Nelemans,Miquel Nofrarías,Antoine Petiteau,P. Pivato,Eric Plagnol,Ed Porter,J. Reiche,David J. Robertson,N. A. Robertson,Elena M. Rossi,G. Russano,Bernard F. Schutz,Alberto Sesana,David H. Shoemaker,Jacob Slutsky,Carlos F. Sopuerta,T. J. Sumner,Nicola Tamanini,Ira Thorpe,Michael Troebs,Michele Vallisneri,Alberto Vecchio,Daniele Vetrugno,Stefano Vitale,Marta Volonteri,Gudrun Wanner,H. Ward,Peter Wass,W. J. Weber,John Ziemer,Peter Zweifel +83 more
TL;DR: The LISA Consortium as mentioned in this paper proposed a 4-year mission in response to ESA's call for missions for L3, which is an all-sky monitor and will offer a wide view of a dynamic cosmos using Gravitational Waves as new and unique messengers to unveil The Gravitational Universe.
Journal ArticleDOI
Sensitivity studies for third-generation gravitational wave observatories
Stefan Hild,M. R. Abernathy,Fausto Acernese,Pau Amaro-Seoane,Nils Andersson,K. G. Arun,Fabrizio Barone,B. Barr,M. Barsuglia,Mark Beker,N. Beveridge,S. Birindelli,Suvadeep Bose,L. Bosi,S. Braccini,C. Bradaschia,Tomasz Bulik,Enrico Calloni,Giancarlo Cella,E. Chassande Mottin,S. Chelkowski,Andrea Chincarini,James S. Clark,E. Coccia,C. Colacino,J. Colas,A. Cumming,L. Cunningham,E. Cuoco,S. L. Danilishin,Karsten Danzmann,R. De Salvo,T. Dent,R. De Rosa,L. Di Fiore,A. Di Virgilio,M. Doets,V. Fafone,Paolo Falferi,R. Flaminio,J. Franc,F. Frasconi,Andreas Freise,D. Friedrich,Paul Fulda,Jonathan R. Gair,Gianluca Gemme,E. Genin,A. Gennai,A. Giazotto,Kostas Glampedakis,Christian Gräf,M. Granata,Hartmut Grote,G. M. Guidi,A. Gurkovsky,G. D. Hammond,Mark Hannam,Jan Harms,D. Heinert,Martin Hendry,Ik Siong Heng,E. Hennes,J. H. Hough,Sascha Husa,S. H. Huttner,G. T. Jones,F. Y. Khalili,Keiko Kokeyama,Kostas D. Kokkotas,Badri Krishnan,Tjonnie G. F. Li,M. Lorenzini,H. Lück,Ettore Majorana,Ilya Mandel,Vuk Mandic,M. Mantovani,I. W. Martin,Christine Michel,Y. Minenkov,N. Morgado,S. Mosca,B. Mours,Helge Müller-Ebhardt,P. G. Murray,Ronny Nawrodt,Ronny Nawrodt,John Nelson,Richard O'Shaughnessy,Christian D. Ott,C. Palomba,Angela Delli Paoli,G. Parguez,A. Pasqualetti,R. Passaquieti,R. Passaquieti,D. Passuello,Laurent Pinard,Wolfango Plastino,Rosa Poggiani,Rosa Poggiani,P. Popolizio,Mirko Prato,M. Punturo,P. Puppo,D. S. Rabeling,P. Rapagnani,Jocelyn Read,Tania Regimbau,H. Rehbein,S. Reid,F. Ricci,F. Richard,A. Rocchi,Sheila Rowan,A. Rüdiger,Lucía Santamaría,Benoit Sassolas,Bangalore Suryanarayana Sathyaprakash,Roman Schnabel,C. Schwarz,Paul Seidel,Alicia M. Sintes,Kentaro Somiya,Fiona C. Speirits,Kenneth A. Strain,S. E. Strigin,P. J. Sutton,S. P. Tarabrin,Andre Thüring,J. F. J. van den Brand,M. van Veggel,C. Van Den Broeck,Alberto Vecchio,John Veitch,F. Vetrano,A. Viceré,S. P. Vyatchanin,Benno Willke,Graham Woan,Kazuhiro Yamamoto +141 more
TL;DR: In this article, a special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates, including the most relevant fundamental noise contributions.
Journal ArticleDOI
Low-frequency gravitational-wave science with eLISA/NGO
Pau Amaro-Seoane,Sofiane Aoudia,Stanislav Babak,Pierre Binétruy,Emanuele Berti,Alejandro Bohé,Chiara Caprini,Monica Colpi,Neil J. Cornish,Karsten Danzmann,Jean-François Dufaux,Jonathan R. Gair,Oliver Jennrich,Philippe Jetzer,Antoine Klein,Ryan N. Lang,Alberto Lobo,Tyson Littenberg,Sean T. McWilliams,Gijs Nelemans,Gijs Nelemans,Antoine Petiteau,Edward K. Porter,Bernard F. Schutz,Alberto Sesana,Robin Stebbins,T. J. Sumner,Michele Vallisneri,Stefano Vitale,Marta Volonteri,H. Ward +30 more
TL;DR: The New Gravitational-Wave Observatory (NGO) as discussed by the authors, a mission under study by the European Space Agency for launch in the early 2020s, will survey the low-frequency gravitational wave sky (from 0.1 mHz to 1 Hz), detecting and characterizing a broad variety of systems and events throughout the Universe, including the coalescences of massive black holes brought together by galaxy mergers, the inspirals of stellar-mass black holes and compact stars into central galactic black holes; several millions of ultra-compact binaries, both detached and mass transferring, in