HARMONI at ELT: overview of the capabilities and expected performance of the ELT's first light, adaptive optics assisted integral field spectrograph.

Niranjan . Thatte,Dave Melotte,Benoit Neichel,David Le Mignant,Ian Bryson,Fraser Clarke,Vanessa Ferraro-Wood,Thierry Fusco,Oscar Gonzalez,Hermine Schnetler,Matthias Tecza, Sandi Wilson, Alonso Álvarez Urueña, Heribert A. Vilaseca,Santiago Arribas Mocoroa, Gonzalo José Carracedo Carballale,Alejandro Crespo, Alberto Estrada Piqueras, Miriam García García,Cecilia Martínez Martín,Miguel Pereira Santaella,Michele Perna,Javier Piqueras López,Niolas Bouché, Didier Boudon, Eric Daguisé,Karen Disseau,Jérémy J. Fensch,Adrien Girardot,Matthieu Guibert,Aurélien Jarno,Alexandre Jeanneau,Jens-Kristian Krogager,Florence Laurent, Magali Loupias, Jean-Emmanuel Migniau,Laure Piqueras, Alban Remillieux, Johan Richard,Arlette Pecontal,Lisa F. Bardou,David Barr,Sylvain Cetre,Rishi Deshmukh,Sofia Dimoudi,Marc Dubbledam,Andrew Dunn,Dimitra Gadotti, Joss J. Guy,David L. King, David J. Little,Anna McLeod,Simon Morris,Tim Morris,Kieran S. O'Brien, Emily Ronson,Russell Smith,Lazar Staykov,Mark Swinbank,Matthew Townson,Matteo Accardo,Domingo Alvarez Mendez,Elizabeth George,Joshua Hopgood,Derek Ives,Leander Mehrgan,Eric Mueller, Javier Reyes-Moreno,Ralf Conzelmann,Pablo Gutierrez Cheetham,Ángel Alonso-Sánchez,Giuseppina Battaglia,Miguel Angel Cagigas Garcia,Haresh M. Chulani, Graciela C. Delgado García, Patricia Fernández-Izquierdo, Ana Belén Fragoso López,Begoña García-Lorenzo, Alberto Hernández González, Elvio Hernández Suárez, Jose Miguel Herreros Linares,Enrique Joven,Roberto López López, Alejandro Antonio Lujan Gonzalez,Yolanda Martín,Evencio Mediavilla,Saúl Menéndez Mendoza, Luz Maria Montoya Martínez,José Peñate Castro, Álvaro Pérez,José Luis Rasilla, Rafael Rebolo-López,Luis Fernando Rodríguez-Ramos,Afrodisio Vega Moreno,Teodora Viera-Curbelo,Natacha Zanon Dametto,Alexis Carlotti,Jean-Jacques Correia, Stéphane Curaba,Alain Delboulbé,Sylvain Guieu, Adrien Hours,Zoltan Hubert,Laurent Jocou,Yves Magnard,Thibaut Moulin,Fabrice Pancher,Patrick Rabou,Eric Stadler, Maxime Vérove,Thierry Contini, Marie Larrieu, Olivier Boebion, Yan Fantéï-Caujolle, Daniel Lecron,Sylvain Rousseau,Philippe Amram,Olivier Beltramo-Martin, William Bon,Anne Bonnefoi, William Ceria,Zalpha Challita, Yannick Charles,Elodie Choquet,Carlos Correia,Anne Costille,Kjetil Dohlen, Franck Ducret,Kacem El Hadi,Jean-Luc Gach,Jean-Luc Gimenez,Olivier Groussin,Marc Jaquet,Pierre Jouve,Fabrice Madec,Felipe Pedreros Bustos,Edgard Renault,Patrice Sanchez,Arthur Vigan,Pascal Vola, Annie Zavago,Romain Fétick,Caroline Lim,Cyril Petit,Jean-Francois Sauvage,Nicolas Védrenne,Fehim Taha Bagci,Martin E. Caldwell,Ellis Elliott,Peter Hiscock,Emma Johnson,Murali Nalagatla, Aristea Seitis,Mark Wells,Martin Black,Charlotte Z. Bond, Saskia Brierley, Kenneth Campbell,Neil Campbell, James Carruthers,William Cochrane,Chris Evans,Joel Harman,William Humphreys,Thomas Louth,Chris Miller,David Montgomery,Meenu Murali,John Murray, Norman O'Malley,Ruben Sanchez-Janssen,Noah Schwartz,Patrick Smith, Jonathan Strachan,Stephen Todd,Stuart Watt,Martyn Wells,Asim Yaqoob,Eric Bell,Oleg O. Gnedin,Kayhan Gultekin,Mario Mateo, Michael Meyer,Munadi Ahmad,Jayne Birkby,Michael Booth,Michele Cappellari,Edgar Castillo Dominguez, Jorge Chao Ortiz,David Gooding,Kearn Grisdale,Andrea Hidalgo Valadez,Laurence Hogan,James Kariuki,Ian Lewis,Adam Lowe,Zeynep Ozer,Laurence Routledge,Dimitra Rigopoulou,Alec York

Ground-based and Airborne Instrumentation for Astronomy IX(2022)

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摘要
HARMONI is the first light, adaptive optics assisted, integral field spectrograph for the European Southern Observatory’s Extremely Large Telescope (ELT). A work-horse instrument, it provides the ELT’s diffraction limited spectroscopic capability across the near-infrared wavelength range. HARMONI will exploit the ELT’s unique combination of exquisite spatial resolution and enormous collecting area, enabling transformational science. The design of the instrument is being finalized, and the plans for assembly, integration and testing are being detailed. We present an overview of the instrument’s capabilities from a user perspective, and provide a summary of the instrument’s design. We also include recent changes to the project, both technical and programmatic, that have resulted from red-flag actions. Finally, we outline some of the simulated HARMONI observations currently being analyzed.
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