Glao PowerPoint PPT Presentations

Title: Raven with Subaru Author: Shin Oya Last modified by: oya Created Date: 12/17/2002 1:14:08 AM Document presentation format:

EE x 2 in 0.2'' pixel or Diffraction limited (NFM) Visible ... Tip-tilt guide star flux. 2.8' off-axis (x=2',y=2') Position of NGS. 0.4. Loop gain. 3 e- rms ...

MUSE - ASSIST and GLAO Update. Remko Stuik and Ralf Flicker. Leiden Observatory ... MUSE AO - MUSE. AO Technical Specifications. LGS positioning. On the edge ...

Extreme AO for imaging planets around nearby stars ... Credit: J-M Conan. GLAO uses 1 ground-conjugated DM, corrects near-ground turbulence ...

NGS, Mauna Kea Atmospheric Profile. 2 DMs / 5 NGS. 320 stars / K band / 0.7'' seeing ... Gemini South MCAO. Credit: Eric James & Brent Ellerbroek, Gemini ...

Atmospheric tomography requires multiple high power lasers, ... Spinning shutters/mirrors. LGS/NGS AO system. Xinetics 97 DM. 2 arcmin FOV. 300Hz loop speed ...

TELESCOPE GROWTH SINCE GALILEO. Telescope size driven by glas technology for ... Today, advances in fabrication and control technologies allow EL segmented ...

Multi-conjugate AO (MCAO) Adaptive secondary mirror is the first deformable element in all AO systems. Ground Layer AO (GLAO) with GMT Emerging technology.

Title: Raven with Subaru Author: Shin Oya Last modified by: oya Created Date: 12/17/2002 1:14:08 AM Document presentation format:

Gemini North has just begun operating with a laser guide star. ... VLT, Subaru, Gemini South, Keck I are all actively working to deploy lasers. ...

Ground layer wavefront reconstruction using dynamically refocused Rayleigh laser beacons C. Baranec, M. Lloyd-Hart, M. Milton, T. Stalcup, M. Snyder, N. Putnam and R ...

LGS AO for LBT: possible Implementation Options

MultiObject AO [MOAO] Falcon study. Extra-galactic 3D spectrocopy ... Falcon: H band VLT obs. in 25' FoV. 60 GS for WFS. 15 to 20 IFU on galaxies ...

... is a pulsed Rayleigh system. projection system should be independent of laser ... projector for each of the pupils and use simple reflective/lens optics, ...

3 in concentration, operability significantly above median seeing ... tradeoff between PSF stability across field and FWHM, predictability of PSF ...

peculiar velocity fields, bow shocks. Stellar disks and Jets. 0.5' Magnetic flow surfaces ... Marconi & Hunt (2003) correlation BH mass bulge mass ...

Natural Guide Star. Laser Guide Star. Deformable Mirror. C. Max. RASC, Victoria, 1/08/06 ... AO works best if star light is BRIGHT and NEARBY. RASC, Victoria, 1 ...

Donald Gavel. Chair, AO Working Group. Tucson, Dec. 17, 2003. 2. Purpose of our visit ... Estimate the effort needed to study the trade offs and give feedback ...

Brazilian Tunable Filter Imager (BTFI) Preliminary Design ... Natural guide-star (NGS) operations: Sep'09. Laser guide-star (LGS) operations: ~Sep'10 (tbc) ...

OS: CentOS with RTAI real-time extensions. Frame Grabber: EDT PCI-DV ... Linearization using LUT 1024 element vector. Read tip/tilt signal from tilt computer ...

Stop Press: Gem-S now the world's first 8m telescope with a silvered primary! Ag. Al ... on Gem-S successfully coated with silver. ATNF Marsfield, 8 June 2004 ...

The long exposure PSF delivered by an NGS or LGS AO system varies in ... Tweeter Phase Variance in a Woofer/Tweeter AO Architecture. The PSF of an LGS System ...

JRA1: 2nd generation Adaptive Optics for 810 m class Telescopes

Widefield IR astronomy at Dome C. Mark Casali. European Southern Observatory ... very low temperatures reduce thermal background by 50. typical PWV of 0.25 mm ...

Pacing the design and development effort. Scientific utility, cost, ... 'Woofer-tweeter' DM configurations. Piezostack, MEMs, and/or an adaptive secondary ...

GMT Board: each institution has two members ... 3.2-m adaptive Gregorian secondary mirror. Instruments mount below M1 at the ... by tilt anisotropy ...

Extragalactic Studies on Galaxy Evolution with a Wide ... Given the known characteristics of galaxies ... IRAS discovered Ultra Luminous IR Galaxies (ULIRG) ...

CANARY concept. Optomechanical design. Subsystem performance. System performance ... CANARY Aims. Perform NGS then LGS based tomographic WFSing ...

... in fab, science channel optics well along. Science channel/NGS delivery ... science ... Niche survey science in crowded Galactic fields. Must be done ...

Large visible fast low-noise detector for Shack-Hartmann based AO WFS ... Image lag = 'charges left behind': 2% per pixel at the next frame. ...

Adaptive Optics in the VLT and ELT era Beyond Basic AO Fran ois Wildi Observatoire de Gen ve * Usual stuff * * * Usual stuff * Numerical simulation tools written at ...

Guide Star. Companion. OTFgs * ATF = OTFoa. Turbulence theory. Cn2 profile ... Guide star configuration. How the adaptive mirrors are deployed. Zenith angle ...

Optics. Precision. Radial. Velocity. Spectrometer. Gemini. Planet. Imager. Wide. Field. Multi ... Relies on active optics that are always 'on' Primary mirror ...

Spectrometer. Gemini Planet Imager Remains On Track ... Spectrometer ... Precision Radial Velocity Spectrometer ...

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Introduction to Gamma-Ray Bursts (GRBs) Discovered in 1967 by the Vela satellites ... Light curve break :: collimation. Supernova association :: progenitors ...

GSMT Committee, Los Angeles, Oct. 20, 2005. 1. Giant Magellan Telescope ... GSMT Committee, Los Angeles, Oct. 20, 2005. 10. GMT1 Casting- 7/23/05. Peak T = 1160 C ...

Noyaux Actifs de Galaxies. Le Centre Galactique. Haute R solution ... Noyaux Actifs de Galaxie. connection starburst/NAG. structure/composition des r gions ...

... to a have a selector 'knob' for dialing up a preferred value. ... doesn't believe (may be required to be convinced that) we can manage a 'piss-up in a brewary' ...

414 System Design Phase Systems Engineering Management Plan ... 470 Keck NGAO sky coverage modeling. 471 NGAO Wavefront Error and Ensquared Energy Budgets ...

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Title: Project Manager Presentation to the TMT Board Author: Gary H Sanders Last modified by: Brent Ellerbroek Created Date: 10/17/2005 3:31:39 PM

We have requested suggestions for membership from members of ... Gemini Aspen instruments need $7M/year (US share) LSST Design & Development (already funded) ...

Flicker and Neyman has been working on analysis and computer simulations that ... Based on F. Rigaut's AO simulation (YAO), Modified by Flicker for KPAO ...

GMT conceptual design review February 2006 ... Four catadioptric cameras. 4k x 6.5k to 6k x 8k CCDs (15 m pixels) UV: 299 to 389 nm ...

... `XaXbXcXdXeXfXgXhXiXjXkXlXmXnXoXpXqXrXsXtXuXvXwXxXyXzX{X|X}X~X ... 456789:CDEFGHIJSTUVWXYZcdefghijstuvwxyz GpSs tFTO ...

Shack-Hartmann tomographic wavefront reconstruction using LGS: Analysis of spot ... Telescope diameter 21 m, 42x42 sous-pupilles, central occultation factor 0.3 ...

Stellar Populations and Chemical Evolution. Assembly of Galaxies. Black Holes in the Universe ... NIRMOS Properties with OH Suppression and low-noise Near-IR ...

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Taylor frozen flow temporal dynamics. Order 60x60 MCAO. SCAO, LTAO, MCAO. Initial ... Maui MALT median 3.60x10-9 atoms cm-2. Anchored to LLNL dye laser data ...

WFOS, a wide field, seeing-limited optical spectrograph ... MIRES, a mid-IR echelle spectrograph fed by MIRAO ... resolution optical echelle spectrograph ...

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The European Extremely Large Telescope EELT

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UCSC's ELVIS falls short in FoV but is very attractive in other ways ... ELVIS requires 0.25'slits and large CaF2. MILES requires even larger CaF2 ...

I was asked by SOC to give my comments. This is a 'WFMOS ... Flamingos-2 Tandem Tunable Filter. Fully-tunable across YJ. Tandem etalons for better OH blocking ...