First on-sky results of ERIS at VLT

Kateryna Kravchenko, Yigit Dallilar, Olivier Absil, Alex Agudo Berbel, Andrea Baruffolo, Markus Bonse, Alexander Buron, Yixian Cao, Angela Cortes, Felix Dannert, Richard Davies, Robert J. De Rosa, Matthias Deysenroth, David S. Doelman, Frank Eisenhauer, Simone Esposito, Helmut Feuchtgruber, Natascha Förster Schreiber, Xiaofeng Gao, Hans GemperleinReinhard Genzel, Stefan Gillessen, Christian Ginski, Adrian Glauser, Andreas Glindemann, Paolo Grani, Pierre Haguenauer, Johannes Hartwig, Jean Hayoz, Marianne Heida, Matthew Kenworthy, Johann Kolb, Harald Kuntschner, Dieter Lutz, Daizhong Liu, Mike MacIntosh, Michael Marsset, Gilles Orban de Xivry, Hakan Özdemir, Alfio Puglisi, Sascha Quanz, Christian Rau, Armando Riccardi, Daniel Schuppe, Frans Snik, Eckhard Sturm, Linda Tacconi, William D. Taylor, Erich Wiezorrek

Research output: Chapter in Book or Conference Publication/ProceedingConference Publication

3 Citations (Scopus)

Abstract

ERIS (Enhanced Resolution Imager and Spectrograph) is a new adaptive optics instrument installed at the Cassegrain focus of the VLT-UT4 telescope at the Paranal Observatory in Chile. ERIS consists of two near infrared instruments: SPIFFIER, an integral field unit (IFU) spectrograph covering J to K bands, and NIX, an imager covering J to M bands. ERIS has an adaptive optics system able to work with both LGS and NGS. The Assembly Integration Verification (AIV) phase of ERIS at the Paranal Observatory was carried out starting in December 2021, followed by several commissioning runs in 2022. This contribution will describe the first preliminary results of the on-sky performance of ERIS during its commissioning and the future perspectives based on the preliminary scientific results....
Original languageEnglish
Title of host publicationGround-based and Airborne Instrumentation for Astronomy IX
DOIs
Publication statusPublished - Aug 2022

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