Greifswald 2024 – scientific programme
Parts | Days | Selection | Search | Updates | Downloads | Help
EP: Fachverband Extraterrestrische Physik
EP 2: Planets in their Environment
EP 2.9: Talk
Tuesday, February 27, 2024, 17:30–17:45, ELP 1: HS 1.22
ANDES - The high resolution spectrograph for the ELT and its calibration unit(s): Current baseline Design — •Philipp Huke1, Ansgar Reiners2, Michael Debus2, Sebastian Schäfer2, Richard McCracken3, Derryck Reid3, Yuk Shan Cheng3, Kamalesh Dadi3, Mirsad Sarjlic4, Christopher Broeg4, Omar Gabella5, Michael Lehmitz6, Wolfgang Gaessler6, Driss Kouach7, Jörg Knoche8, Lea Bonhomme9, Piotr Maslowski10, and Alessio Zanutta11 — 1Institute for Laser and Optics, University of applied Sciences Emden /Leer — 2Institute for Astrophysics and Geophysics, Georg-August-University Göttingen — 3Institute of Photonics and Quantum Sciences, Herriot-Watt-University Edinburgh — 4Center for Space and Habitability, University of Bern — 5Laboratoire Univers et Particul de Montpellier — 6Max-Planck Institut für Astronomie, Heidelberg — 7Observatoire Midi-Pyrénées, Université de Toulouse — 8University of Hamburg — 9Observatoire Midi-Pyrénées — 10Nicolaus-Copernicus University — 11Osservatorio Astronomico die Trieste
The ANDES-project entered phase B in January 2022. Among its main scientific goals are the detection of atmospheres of exoplanets and the determination of fundamental physical constants. For this, high radial velocity precision and accuracy are required. Even though the ANDES-spectrograph is designed for maximum intrinsic stability, calibration is mandatory. This talk provides and update of the current baseline design of the spectrograph with special emphasis on the calibration unit(s).
Keywords: Spectrograph; ANDES; ELT; Cosmology; Exoplanets