'Collecting area' diaporamas de présentation

Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation. Professor Don Figer X-ray Astronomy. Aims of Lecture. review x-ray photon path describe x-ray detection describe specific x-ray telescopes give examples of x-ray objects. X-ray Photon Path. Atmospheric Absorption.

573 views • 57 slides

Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation. Professor Don Figer X-ray Astronomy. Aims of Lecture. review x-ray photon path describe x-ray detection describe specific x-ray telescopes give examples of x-ray objects. X-ray Photon Path. Atmospheric Absorption.

535 views • 53 slides

Chapter 6 Telescopes: Portals of Discovery

Chapter 6 Telescopes: Portals of Discovery. 6.1 Eyes and Cameras: Everyday Light Sensors. Our goals for learning: How does your eye form an image? How do we record images?. How does your eye form an image?. Refraction.

524 views • 52 slides

Chapter 6 Telescopes: Portals of Discovery

Chapter 6 Telescopes: Portals of Discovery. 6.1 Eyes and Cameras: Everyday Light Sensors. Our goals for learning: How does your eye form an image? How do we record images?. How does your eye form an image?. Refraction.

539 views • 52 slides

The Imaging Chain for X-Ray Astronomy

680 views • 50 slides

Chapter 6 Telescopes: Portals of Discovery

Chapter 6 Telescopes: Portals of Discovery. 6.1 Eyes and Cameras: Everyday Light Sensors. Our goals for learning: How does your eye form an image? How do we record images?. How does your eye form an image?. Refraction.

567 views • 48 slides

Telescopes of the future: SKA and SKA demonstrators

Telescopes of the future: SKA and SKA demonstrators. Elaine Sadler, University of Sydney. Aperture synthesis techniques have now been in use for over 40 years (1974 Nobel prize to Martin Ryle) - what next? Why are we planning new telescopes? What will they look like?

619 views • 44 slides

Astronomical Institute, Academy of Sciences of the Czech Republic, Ond?ejov, Czech Republic

555 views • 42 slides

Telescopes: Portals of Discovery

428 views • 42 slides

Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation. RIT Course Number 1060-771 Professor Don Figer X-ray Astronomy. Aims of Lecture. review x-ray photon path describe x-ray detection describe specific x-ray telescopes give examples of x-ray objects. X-ray Photon Path.

524 views • 40 slides

High energy Astrophysics Cosmology and extragalactic astronomy

High energy Astrophysics Cosmology and extragalactic astronomy. Mat Page. Mullard Space Science Lab, UCL. 15. Cosmology and High Energy Astrophysics in the future. Slide 2. 15. High energy astrophysics in the future. This lecture: Future missions and observatories: What they are

556 views • 37 slides

Neutral Hydrogen at High Redshift

Neutral Hydrogen at High Redshift. Jared Bowden Dain Kavars. Agenda. Brief introduction and current knowledge N-Body simulations and models Projected integration times Techniques of detection (Instruments) Results and conclusions. Introduction. HI at large z

452 views • 31 slides

373 views • 28 slides

On A Large Array Of Midsized Telescopes

On A Large Array Of Midsized Telescopes. Stephen Fegan Vladimir Vassiliev UCLA. Primary Science Goals. Detect and measure VHE transients at cosmological distances Self triggering Measure lightcurve from Mrk-421 at z=1 with few minute resolution Survey of VHE sky to level of 1-2 mCrab

341 views • 27 slides

The SKAMP Project & Virtual Observatory Considerations

The SKAMP Project & Virtual Observatory Considerations. The SKAMP Project & Virtual Observatory Considerations. Outline: SKA (Square Kilometre Array) overview SKAMP (SKA Molonglo Prototype) Project Aims & Overview Status SKAMP VO Considerations Data & data-pipeline.

347 views • 23 slides

Will exobiology out of the Solar System stop after the DARWIN mission ?

345 views • 23 slides

Astro-H XRT system

Astro-H XRT system. Contents 1. Astro-H satellite 2. XRT components & design 3. HXT (foil production, calibration facility) 4. SXT (improvements from Suzaku to Astro-H). H.Awaki (Ehime University) + Astro-H XRT team

351 views • 21 slides

University of Sydney Facilities

322 views • 19 slides

Lecture 2 : Telescopes and the Diffraction Limit

Lecture 2 : Telescopes and the Diffraction Limit. Large astronomical telescopes are used as cameras. Can apply simple optics: all targets so distant, light enters as parallel rays parallel rays focussed distance f (= focal length) from lens/mirror

179 views • 7 slides