'5 arcsec' presentation slideshows

3D Spectrography From first principles to science

3D Spectrography From first principles to science. Eric Emsellem Centre de Recherche Astronomique de Lyon. emsellem@obs.univ-lyon1.fr. Menu. Basics of 2D spectrography: Why ? How ? What can we trace with 2D spectrography ? A few illustrations:

750 views • 73 slides

Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation. Professor Don Figer Instruments. Aims for Lecture. Introduce modern Optical/NIR/UV instrumentation. instrument requirements instrument examples Describe capabilities of commonly used instruments. HST Spitzer Chandra JWST ELTs

538 views • 53 slides

Hubble Space Telescope Cutaway

Hubble Space Telescope Cutaway. Hubble Space Telescope Field of View. WFC3 ACS STIS COS FGS. HST: WFC3. HST: WFC3. HST: ACS. HST: ACS. HST: STIS. HST: STIS. Spitzer Space Telescope. IRAC IRS MIPS. Spitzer Space Telescope: IRAC. Spitzer Space Telescope: IRS.

551 views • 50 slides

Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation. RIT Course Number 1060-771 Professor Don Figer Instruments. Aims for Lecture. Introduce modern Optical/NIR/UV instrumentation. instrument requirements instrument examples Describe capabilities of commonly used instruments. HST

569 views • 41 slides

Sviluppi tecnologici

457 views • 31 slides

Sergio Campana

336 views • 24 slides

ALMA Design Reference Science Plan

311 views • 21 slides

Introduction of RAVEN

Introduction of RAVEN. Internal meeting on future instrument projects at Subaru. 2010/4/26 @ Hilo. Shin Oya ? Subaru Telescope/NAOJ) ?. Outline. RAVEN project project outline Multi-Object Adaptive Optics (MOAO) ? Subaru Telescope and RAVEN carry-in instrument (PI instrument) ?

217 views • 21 slides

Strumentazione sub-mm/mm pre-ALMA

Strumentazione sub-mm/mm pre-ALMA. APEX SCUBA & SCUBA-2 IRAM SMA CSO OVRO, BIMA ? CARMA NMA. APEX : A tacama P athfinder EX periment. Location: Llano de Chajnantor (Chile, 5000 m) Antenna modified copy of US ALMA prototype MPIfR=50% Onsala Sp. Obs=23% ESO=27%

332 views • 16 slides

285 views • 13 slides

HST Snapshot Images of Asteroids

HST Snapshot Images of Asteroids. Alex Storrs Khaldoun Makhoul Mike Gaffey, U. of N. Dakota Rob Landis, JPL Faith Vilas, JSC and NASA HQ Ed Wells, CSC/STScI Chuck Wood Ben Zellner, Ga. Southern Univ. 1 Ceres, F439W. 0.5 arcsec.

178 views • 10 slides

NGS and LGS Adaptive Optics Improving faint light performance

NGS and LGS Adaptive Optics Improving faint light performance. Chris Shelton Mitchell Troy, Antonin Bouchez, Jennifer Roberts, Thang Trinh, Tuan Truong September 14, 2006. Why AO?. Frosty Leo J, H, K false color Guide object was upper blue lobe, integrated R magnitude 10.5

218 views • 9 slides

LAMP LuckyCam, AO, Aperture Masking and Polarization @ Palomar

LAMP LuckyCam, AO, Aperture Masking and Polarization @ Palomar. Nicholas Law (Caltech), Craig Mackay (Cambridge), Mike Ireland (Caltech), Peter Tuthill (Sydney), Jamie Lloyd (Cornell) Rich Dekany P3K Meeting 15 Feb 2007. LAMP Overview. Concept: AO-Assisted Observations in the visible

187 views • 7 slides