H
Heike Rauer
Researcher at Technical University of Berlin
Publications - 517
Citations - 19822
Heike Rauer is an academic researcher from Technical University of Berlin. The author has contributed to research in topics: Planet & Exoplanet. The author has an hindex of 64, co-authored 476 publications receiving 17741 citations. Previous affiliations of Heike Rauer include German Aerospace Center & Max Planck Society.
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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.
Journal ArticleDOI
Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius
A. Léger,Daniel Rouan,Jean Schneider,Pierre Barge,M. Fridlund,B. Samuel,Marc Ollivier,Eike W. Guenther,Magali Deleuil,Hans J. Deeg,M. Auvergne,Roi Alonso,Suzanne Aigrain,A. Alapini,J. M. Almenara,Annie Baglin,M. Barbieri,H. Bruntt,Pascal Bordé,François Bouchy,J. Cabrera,C. Catala,Ludmila Carone,S. Carpano,Sz. Csizmadia,Rudolf Dvorak,Anders Erikson,Sylvio Ferraz-Mello,Bernard Foing,Francois Fressin,Davide Gandolfi,Michaël Gillon,P. Gondoin,Olivier Grasset,Tristan Guillot,A. P. Hatzes,Guillaume Hébrard,Laurent Jorda,Helmut Lammer,Antoine Llebaria,B. Loeillet,B. Loeillet,Michel Mayor,Tsevi Mazeh,C. Moutou,Martin Pätzold,Frederic Pont,Didier Queloz,Heike Rauer,S. Renner,R. Samadi,Avi Shporer,C. Sotin,Brandon Tingley,Günther Wuchterl,M. Adda,P. Agogu,Thierry Appourchaux,H. Ballans,Philippe Baron,T. Beaufort,R. Bellenger,R. Berlin,P. Bernardi,D. Blouin,Frédéric Baudin,P. Bodin,L. Boisnard,L. Boit,F. Bonneau,S. Borzeix,R. Briet,Jean-Tristan Buey,B. Butler,D. Cailleau,R. Cautain,P.-Y. Chabaud,S. Chaintreuil,F. Chiavassa,V. Costes,V. Cuna Parrho,F. De Oliveira Fialho,M. Decaudin,J.-M. Defise,S. Djalal,G. Epstein,G.-E. Exil,C. Fauré,T. Fenouillet,A. Gaboriaud,A. Gallic,P. Gamet,P. Gavalda,E. Grolleau,R. Gruneisen,L. Guéguen,V. Guis,V. Guivarc'h,P. Guterman,D. Hallouard,J. Hasiba,F. Heuripeau,G. Huntzinger,H. Hustaix,C. Imad,C. Imbert,B. Johlander,M. Jouret,P. Journoud,F. Karioty,L. Kerjean,V. Lafaille,L. Lafond,T. Lam-Trong,P. Landiech,V. Lapeyrère,T. Larqué,T. Larqué,P. Laudet,N. Lautier,H. Lecann,Laure Lefèvre,B. Leruyet,P. Levacher,A. Magnan,E. Mazy,Florent Mertens,J.-M. Mesnager,J. C. Meunier,J.-P. Michel,W. Monjoin,D. Naudet,K. Nguyen-Kim,J.-L. Orcesi,H. Ottacher,R. Perez,Gisbert Peter,P. Plasson,J.-Y. Plesseria,B. Pontet,A. Pradines,Céline Quentin,J.-L. Reynaud,G. Rolland,F. Rollenhagen,R. Romagnan,N. Russ,R. Schmidt,N. Schwartz,I. Sebbag,G. Sedes,H. Smit,M. Steller,W. Sunter,Christian Surace,M. Tello,D. Tiphène,P. Toulouse,B. Ulmer,O. Vandermarcq,E. Vergnault,A. Vuillemin,P. Zanatta +162 more
TL;DR: In this paper, the authors reported the discovery of very shallow (ΔF/F ≈ 3.4× 10 −4 ) periodic dips in the light curve of an active V = 11.7 G9V star observed by the CoRoT satellite, which they interpret as caused by a transiting companion.
Journal ArticleDOI
Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius
A. Léger,Daniel Rouan,Jean Schneider,Pierre Barge,M. Fridlund,B. Samuel,Marc Ollivier,Eike W. Guenther,Magali Deleuil,Hans J. Deeg,M. Auvergne,Roi Alonso,Suzanne Aigrain,A. Alapini,J. M. Almenara,A. Baglin,M. Barbieri,H. Bruntt,Pascal Bordé,François Bouchy,J. Cabrera,C. Catala,L. Carone,Stefania Carpano,Sz. Csizmadia,Rudolf Dvorak,Anders Erikson,Sylvio Ferraz-Mello,Bernard Foing,Francois Fressin,Davide Gandolfi,Michaël Gillon,P. Gondoin,Olivier Grasset,Tristan Guillot,A. P. Hatzes,G. Hebrard,Laurent Jorda,Helmut Lammer,Antoine Llebaria,B. Loeillet,M. Mayor,Tsevi Mazeh,C. Moutou,Martin Paetzold,Frederic Pont,Didier Queloz,Heike Rauer,S. Renner,R. Samadi,Avi Shporer,C. Sotin,Brandon Tingley,Günther Wuchterl +53 more
TL;DR: In this paper, the authors reported the discovery of very shallow (DF/F = 3.4 10-4), periodic dips in the light curve of an active V = 11.7 G9V star observed by the CoRoT satellite, which they interpret as due to the presence of a transiting companion.