Science Case

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JWST key science The End of the Dark Ages: First Light and Reionization Assembly of Galaxies ➱ suite of optical/NIR sensitive multi-object spectrographs The Birth of Stars and Protoplanetary Systems Planetary Systems and the Origins of Life ➱ METIS: mid-IR instrument (high spatial/spectral resolution at 3-15 μm) ➱ EPICS: planet-finder (incl. low-resolution spectroscopy and polarimetry) Markus Kissler-Patig - ELT Science Case
ALMA key science Detect spectral line emission from CO or CII in a normal galaxy like the Milky Way at a redshift of z = 3, in less than 24 hours of observation. ➱ NIR sensitive integral spectrograph and imager Image the gas kinematics in protostars and in protoplanetary disks around young Sun-like stars at a distance of the nearest star-forming clouds. ➱ NIR and mid-IR high-spectral resolution instruments Provide precise images at an angular resolution of 0.1 arcsec. Markus Kissler-Patig - ELT Science Case
Page 1 and 2: European Extremely Large Telescope
Page 3: E-ELT Overview
Page 6 and 7: The E-ELT Dome
Page 8 and 9: $ N?G7J8$:$$$.A6OD>I$$6=;>%L?AGJAO6
Page 10 and 11: Adaptive Optics • The Telescope d
Page 12 and 13: Instrument Suite
Page 14 and 15: Foreseen first generation of instru
Page 16 and 17: Markus Kissler-Patig E-ELT Status G
Page 18 and 19: TEST INSTRUMENT DISTRIBUTION (NASMY
Page 20 and 21: PRELIMINARY NIRSpec E-ELT Instrumen
Page 22 and 23: PRELIMINARY WF, visual-red camera o
Page 24 and 25: The Science Case for Giant Telescop
Page 26 and 27: Markus Kissler-Patig - ELT Science
Page 28 and 29: Synergy with Large Facilities Marku
Page 32 and 33: Contemporary Science The Design Ref
Page 34 and 35: Planets & Stars Markus Kissler-Pati
Page 36 and 37: Planets & Stars Stars & Galaxies Ma
Page 38 and 39: Planets & Stars Stars & Galaxies Ga
Page 40 and 41: From giant to terrestrial exo-plane
Page 42 and 43: Today, we can detect Jupiter-mass p
Page 46 and 47: Circumstellar disks are the birthpl
Page 50 and 51: Derived key requirements: • “wi
Page 52 and 53: Imaging and spectroscopy of resolve
Page 54 and 55: Understanding the formation and evo
Page 56 and 57: Imaging and spectroscopy of resolve
Page 58 and 59: Derived key requirements: • high
Page 60 and 61: The physics of high-redshift galaxi
Page 62 and 63: What did galaxies look like 10 bill
Page 64 and 65: The physics of high-redshift galaxi
Page 66 and 67: Derived key requirements: • high
Page 68 and 69: For the very first time, a direct m
Page 70: Thank You

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