Science Case

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PRELIMINARY WF, visual-red camera or spectrograph with GLAO E-ELT Instrumentation Project Office PIXEL SAMPLING, EE within 2x2 spaxels of Wide Field E-ELT INSTRUMENTS EE 0 100 Pixel size (mas) EE 30% at I 5’ EAGLE, NIR MIFU with MOAO
<strong>Science</strong> <strong>Case</strong>
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 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 30 and 31: JWST key science The End of the Dar
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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