M
Matteo Accardo
Researcher at European Southern Observatory
Publications - 49
Citations - 1827
Matteo Accardo is an academic researcher from European Southern Observatory. The author has contributed to research in topics: Spectrograph & Telescope. The author has an hindex of 13, co-authored 44 publications receiving 1457 citations. Previous affiliations of Matteo Accardo include Max Planck Society.
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Proceedings ArticleDOI
The MUSE second-generation VLT instrument
Roland Bacon,Matteo Accardo,L. Adjali,H. Anwand,Svend-Marian Bauer,I. Biswas,Jeremy Blaizot,D. Boudon,S. Brau-Nogué,Jarle Brinchmann,P. Caillier,L. Capoani,C. M. Carollo,T. Contini,P. Couderc,E. Daguisé,S. Deiries,B. Delabre,Stefan Dreizler,Jean-Pierre Dubois,M. Dupieux,Christophe Dupuy,Eric Emsellem,Eric Emsellem,T. Fechner,A. Fleischmann,Marc François,G. Gallou,T. Gharsa,Andreas Glindemann,D. Gojak,B. Guiderdoni,G. Hansali,T. Hahn,Aurélien Jarno,Andreas Kelz,C. Koehler,Johan Kosmalski,F. Laurent,M. Le Floc'h,Simon J. Lilly,J.-L. Lizon,M. Loupias,Antonio Manescau,Christian Monstein,Harald Nicklas,J.-C. Olaya,L. Parès,Luca Pasquini,Arlette Pécontal-Rousset,Roser Pello,C. Petit,E. Popow,Roland Reiss,A. Remillieux,E. Renault,Martin Roth,Gero Rupprecht,Denis Serre,Joop Schaye,G. Soucail,Matthias Steinmetz,Ole Streicher,Remko Stuik,Valentin H,Joel Vernet,Peter M. Weilbacher,Lutz Wisotzki,N. Yerle +68 more
TL;DR: The Multi Unit Spectroscopic Explorer (MUSE) as mentioned in this paper is a second-generation VLT panoramic integral-field spectrograph currently in manufacturing, assembly and integration phase.
Journal ArticleDOI
First Light for GRAVITY: Phase Referencing Optical Interferometry for the Very Large Telescope Interferometer
R. Abuter,Matteo Accardo,António Amorim,Narsireddy Anugu,G. Avila,N. Azouaoui,Myriam Benisty,Jean-Philippe Berger,Nicolas Blind,H. Bonnet,Pierre Bourget,Wolfgang Brandner,R. Brast,A. Buron,Leonard Burtscher,Frédéric Cassaing,F. Chapron,Elodie Choquet,Y. Clénet,C. Collin,V. Coudé du Foresto,W. J. de Wit,P. T. de Zeeuw,Casey Deen,F. Delplancke-Ströbele,Roderick Dembet,Frederic Derie,Jason Dexter,Gilles Duvert,M. Ebert,Andreas Eckart,Frank Eisenhauer,Michael Esselborn,P. Fédou,G. Finger,Paulo J. V. Garcia,C. E. Garcia Dabo,R. J. García López,Eric Gendron,R. Genzel,Stefan Gillessen,Frédéric Gonté,Paulo Gordo,M. Grould,Ulrich Grözinger,S. Guieu,P. Haguenauer,O. Hans,Xavier Haubois,M. Haug,F. Haussmann,Th. Henning,Stefan Hippler,Matthew Horrobin,Armin Huber,Z. Hubert,N. Hubin,Christian A. Hummel,Gerd Jakob,A. Janssen,Lieselotte Jochum,Laurent Jocou,Andreas Kaufer,S. Kellner,L. Kern,Pierre Kervella,Mario Kiekebusch,Ralf Klein,Yitping Kok,Johann Kolb,Martin Kulas,Sylvestre Lacour,Vincent Lapeyrere,B. Lazareff,J.-B. Le Bouquin,Pierre Léna,Rainer Lenzen,Samuel Lévêque,Magdalena Lippa,Yves Magnard,Leander Mehrgan,M. Mellein,Antoine Mérand,J. Moreno-Ventas,Thibaut Moulin,Ewald Müller,F. Müller,Udo Neumann,S. Oberti,T. Ott,L. Pallanca,Johana Panduro,Luca Pasquini,T. Paumard,Isabelle Percheron,K. Perraut,Guy Perrin,A. Pflüger,O. Pfuhl,T. Phan Duc,P. M. Plewa,Dan Popovic,Sebastian Rabien,A. Ramirez,Juan-Luis Ramos,C. Rau,M. Riquelme,R.-R. Rohloff,G. Rousset,J. Sanchez-Bermudez,Silvia Scheithauer,Markus Schöller,Nicolas Schuhler,Jason Spyromilio,Christian Straubmeier,Eckhard Sturm,Marcos Suarez,Konrad R. W. Tristram,N. Ventura,F. H. Vincent,Idel Waisberg,Imke Wank,J. Weber,Ekkehard Wieprecht,M. Wiest,Erich Wiezorrek,Markus Wittkowski,Julien Woillez,Burkhard Wolff,Senol Yazici,D. Ziegler,Gérard Zins +131 more
TL;DR: GRAVITY as mentioned in this paper is a new instrument to coherently combine the light of the European Southern Observatory Very Large Telescope Interferometer to form a telescope with an equivalent 130 m diameter angular resolution and a collecting area of 200 m$^2$.
Journal ArticleDOI
First light for GRAVITY: Phase referencing optical interferometry for the Very Large Telescope Interferometer
Roberto Abuter,Matteo Accardo,António Amorim,Narsireddy Anugu,G. Avila,N. Azouaoui,Myriam Benisty,Jean-Philippe Berger,Nicolas Blind,H. Bonnet,Pierre Bourget,Wolfgang Brandner,R. Brast,A. Buron,Leonard Burtscher,Frédéric Cassaing,F. Chapron,Elodie Choquet,Yann Clénet,C. Collin,V. Coudé du Foresto,W. J. de Wit,P. T. de Zeeuw,P. T. de Zeeuw,Casey Deen,F. Delplancke-Ströbele,R. Dembet,Frederic Derie,Jason Dexter,Gilles Duvert,M. Ebert,Andreas Eckart,Andreas Eckart,Frank Eisenhauer,Michael Esselborn,P. Fédou,Gert Finger,Paulo J. V. Garcia,C. E. Garcia Dabo,R. Garcia Lopez,Eric Gendron,R. Genzel,Stefan Gillessen,Frédéric Gonté,Paulo Gordo,M. Grould,Ulrich Grözinger,S. Guieu,S. Guieu,Pierre Haguenauer,O. Hans,Xavier Haubois,Marcus Haug,F. Haussmann,Th. Henning,Stefan Hippler,Matthew Horrobin,Armin Huber,Z. Hubert,Norbert Hubin,Christian A. Hummel,Gerd Jakob,A. Janssen,Lieselotte Jochum,Laurent Jocou,Andreas Kaufer,S. Kellner,Sarah Kendrew,Sarah Kendrew,L. Kern,Pierre Kervella,Pierre Kervella,Mario Kiekebusch,Ralf Klein,Yitping Kok,Johann Kolb,Martin Kulas,Sylvestre Lacour,V. Lapeyrère,Bernard Lazareff,J.-B. Le Bouquin,Pierre Léna,Rainer Lenzen,Samuel Lévêque,Magdalena Lippa,Yves Magnard,Leander Mehrgan,M. Mellein,Antoine Mérand,J. Moreno-Ventas,Thibaut Moulin,Ewald Müller,Ewald Müller,F. Müller,Udo Neumann,Sylvain Oberti,T. Ott,Laurent Pallanca,Johana Panduro,Luca Pasquini,Thibaut Paumard,Isabelle Percheron,Karine Perraut,Guy Perrin,A. Pflüger,Oliver Pfuhl,T. Phan Duc,P. M. Plewa,Dan Popovic,Sebastian Rabien,A. Ramirez,Joany Andreina Manjarres Ramos,C. Rau,M. Riquelme,R.-R. Rohloff,Gérard Rousset,J. Sanchez-Bermudez,Silvia Scheithauer,Markus Schöller,Nicolas Schuhler,Jason Spyromilio,Christian Straubmeier,Eckhard Sturm,Marcos Suarez,Konrad R. W. Tristram,N. Ventura,Frederic H. Vincent,Idel Waisberg,Imke Wank,J. Weber,Ekkehard Wieprecht,M. Wiest,Erich Wiezorrek,Markus Wittkowski,Julien Woillez,Burkhard Wolff,Senol Yazici,D. Ziegler,Gérard Zins +138 more
TL;DR: GRAVITY as discussed by the authors is a new instrument to coherently combine the light of the European Southern Observatory Very Large Telescope Interferometer to form a telescope with an equivalent 130 m diameter angular resolution and a collecting area of 200 m2.
Journal ArticleDOI
Direct constraint on the distance of y2 Velorum from AMBER/VLTI observations
Florentin Millour,Romain Petrov,Olivier Chesneau,D. Bonneau,Luc Dessart,C. Bechet,Isabelle Tallon-Bosc,Michel Tallon,Eric Thiébaut,Farrokh Vakili,Fabien Malbet,Denis Mourard,G. Zins,Alain Roussel,S. Robbe-Dubois,Pascal Puget,Karine Perraut,Franco Lisi,E. Le Coarer,Stephane Lagarde,P. Kern,L. Glück,Gilles Duvert,Alain Chelli,Yves Bresson,Uwe Beckmann,P. Antonelli,Gerd Weigelt,N. Ventura,Martin Vannier,J.-C. Valtier,Leonardo Testi,E. Tatulli,D. Tasso,P. Stefanini,Philippe Stee,W. Solscheid,Dieter Schertl,Piero Salinari,M. Sacchettini,Andrea Richichi,François Reynaud,S. Rebattu,Yves Rabbia,Thomas Preibisch,C. Perrier,F. Pacini,Keiichi Ohnaka,E. Nussbaum,D. Mouillet,J. L. Monin,P. Mège,Philippe Mathias,G. Martinot-Lagarde,G. Mars,Alessandro Marconi,Y. Magnard,Bruno Lopez,D. Le Contel,J. M. Le Contel,Stefan Kraus,D. Kamm,Karl-Heinz Hofmann,O. Hernandez Utrera,M. Heininger,M. Heiden,C. Gil,Elisabetta Giani,A. Glentzlin,Sandro Gennari,A. Gallardo,Didier Fraix-Burnet,Renaud Foy,Eric Fossat,T. Forveille,D. Ferruzzi,P. Feautrier,M. Dugué,Thomas Driebe,A. Domiciano de Souza,A. Delboulbé,C. Connot,J. Colin,Jean-Michel Clausse,Frédéric Cassaing,S. Busoni,S. Bonhomme,T. Blöcker,J. Behrend,Carlo Baffa,Eric Aristidi,B. Arezki,K. Agabi,Bram Acke,Matteo Accardo,Mario Kiekebusch,F. Rantakyrö,Markus Schoeller +97 more
TL;DR: The first AMBER observations of the Wolf-Rayet and O (WR+O) star binary system y2 Velorum were presented in this article, with a resolution R = 1500 in the spectral band 1.95-2.17 micron.
Journal ArticleDOI
The PRIMA fringe sensor unit
Johannes Sahlmann,Serge Menardi,Roberto Abuter,Matteo Accardo,S. Mottini,Francoise Delplancke +5 more
TL;DR: The fringe sensor unit (FSU) as mentioned in this paper is the central element of the phase referenced imaging and micro-arcsecond astrometry (PRIMA) dual-feed facility and provides fringe sensing for all observation modes, comprising off-axis fringe tracking, phase-reference imaging, and high-accuracy narrow-angle astrometric.