'Keck ao' presentation slideshows

Luc Simard AO4ELT3 Conference Firenze, May 27-31, 2013

Exploring the Full Cosmic Timeline with TMT. Luc Simard AO4ELT3 Conference Firenze, May 27-31, 2013. TMT Cosmic Timeline - 13.3 Billion Years. Working at the Diffraction Limit. Seeing-limited observations and observations of resolved sources

646 views • 44 slides

Next Generation Adaptive Optics (NGAO) System Design Phase Update

Next Generation Adaptive Optics (NGAO) System Design Phase Update. Peter Wizinowich, Rich Dekany, Don Gavel, Claire Max Science Case Presenters: Brian Cameron, David Law, Jessica Lu, Phil Marshall, Chuck Steidel, Tommaso Treu Technical Team: Sean Adkins, Brian Bauman, Jim Bell,

539 views • 37 slides

Keck AO the inside story

325 views • 32 slides

Exoplanets : direct detection

426 views • 30 slides

W. M. Keck Observatory: Instrumentation, Adaptive Optics and Scientific Productivity

W. M. Keck Observatory: Instrumentation, Adaptive Optics and Scientific Productivity. Taft Armandroff Director W. M. Keck Observatory. 25 July 2009 La Palma, Canary Islands, Spain. Outline. Recent Science Highlights Current Instrumentation Keck Adaptive Optics

502 views • 30 slides

Strategic Planning for Adaptive Optics at Keck

Strategic Planning for Adaptive Optics at Keck. Claire Max and Mike Liu on behalf of Keck AO Working Group Antonin Bouchez (Caltech), Rich Dekany (Caltech), David Koo (UCSC), Bruce Macintosh (LLNL), Franck Marchis (UCB), Keith Matthews (Caltech). Outline. Role of AO Working Group

270 views • 20 slides

347 views • 19 slides

Science with AO

Science with AO. A. Bouchez for the Keck AO team. Keck AO, K'. Topics. Sample scientific programs. Observing strategies. Technical issues. Sample scientific programs. Program 1: Planetary imaging and spectroscopy.

309 views • 18 slides

AO in AO A daptive O ptics in A stronomical O bservations

811 views • 17 slides

Performance of Adaptive Optics in Large Telescopes:Application to very low-mass objects

Performance of Adaptive Optics in Large Telescopes:Application to very low-mass objects. Eduardo L. Martin Institute for Astronomy University of Hawaii. Operating AO Instruments in Mauna Kea. PUEO: 19 element curvature wavefront sensor at the 3.6-meter CFHT. Open for use since 1996.

242 views • 15 slides

High-contrast imaging with AO

High-contrast imaging with AO. Claire Max with help of Bruce Macintosh GSMT Science Working Group December 2002. Types of high-contrast AO imaging. Point sources near bright stars: images and spectra Brown dwarfs Young Jupiters (still shining in IR)

260 views • 14 slides

ADAPTIVE OPTICS IN ASTRONOMY

272 views • 12 slides

Trade Study Report: NGAO versus Keck AO Upgrade

Trade Study Report: NGAO versus Keck AO Upgrade. NGAO Meeting #5 Peter Wizinowich March 7, 2007. Presentation Sequence. Dictionary Definition & Status Performance Budgets versus Requirements Potential Upgrade Plan Summary. WBS Dictionary Definition & Status.

210 views • 12 slides

LGS-AO observations of the HV Tau C edge-on protoplanetary disk

194 views • 10 slides