arxiv: 1807.10003 · v1 · submitted 2018-07-26 · 🌌 astro-ph.IM
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The MICADO first light imager for the ELT: overview, operation, simulation
Richard Davies
,
Jo\~ao Alves
,
Yann Cl\'enet
,
Florian Lang-Bardl
,
Harald Nicklas
,
J\"org-Uwe Pott
,
Roberto Ragazzoni
,
Eline Tolstoy
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Paola Amico
Heiko Anwand-Heerwart
Santiago Barboza
Lothar Barl
Pierre Baudoz
Ralf Bender
Naidu Bezawada
Peter Bizenberger
Wilfried Boland
Piercarlo Bonifacio
Bruno Borgo
Tristan Buey
Fr\'ed\'eric Chapron
Fanny Chemla
Mathieu Cohen
Oliver Czoske
Vincent Deo
Karen Disseau
Stefan Dreizler
Olivier Dupuis
Maximilian Fabricius
Renato Falomo
Pierre Fedou
Natascha Foerster Schreiber
Vincent Garrel
Norbert Geis
Hans Gemperlein
Eric Gendron
Reinhard Genzel
Stefan Gillessen
Martin Gl\"uck
Frank Grupp
Michael Hartl
Marco H\"auser
Hans-Joachim Hess
Ralf Hofferbert
Ulrich Hopp
Veronika H\"ormann
Zoltan Hubert
Elsa huby
Jean-Michel Huet
Victoria Hutterer
Derek Ives
Annemieke Janssen
Willem Jellema
Wolfgang Kausch
Florian Kerber
Helmut Kravcar
Bertrand Le Ruyet
Kieran Leschinski
Christopher Mandla
Markus Manhart
Davide Massari
Simona Mei
Fr\'ed\'eric Merlin
Lars Mohr
Anna Monna
Norbert Muench
Friedrich Mueller
Gert Musters
Ramon Navarro
Udo Neumann
Nadine Neumayer
Jenny Niebsch
Markus Plattner
Norbert Przybilla
Sebastian Rabien
Ronny Ramlau
Jos\'e Ramos
Suzanne Ramsay
Petra Rhode
Amon Richter
Josef Richter
Hans-Walter Rix
Gabriele Rodeghiero
Ralf-Rainer Rohloff
Matthias Rosensteiner
G\'erard Rousset
J\"org Schlichter
Josef Schubert
Arnaud Sevin
Remko Stuik
Eckhard Sturm
Jens Thomas
Niels Tromp
Gijs Verdoes Kleijn
Fabrice Vidal
Roland Wagner
Michael Wegner
Werner Zeilinger
Julian Ziegleder
Bodo Ziegler
G\'erard Zins
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classification
🌌 astro-ph.IM
keywords
instrumentfirstlightmicadosimulationachieveastrometriccapabilities
read the original abstract
MICADO will enable the ELT to perform diffraction limited near-infrared observations at first light. The instrument's capabilities focus on imaging (including astrometric and high contrast) as well as single object spectroscopy. This contribution looks at how requirements from the observing modes have driven the instrument design and functionality. Using examples from specific science cases, and making use of the data simulation tool, an outline is presented of what we can expect the instrument to achieve.
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