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... • Writing a paper (if we could produce a substantial results). However, the instructor may not have know ledges about many of the above. • Exploit web resources for an easy solution. • Self-teaching and sharing of knowledge of each other are requested. Always think about what kind of contributions t ...
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... Seifahrt and Käufl, “High precision radial velocity measurements in the infrared - A first assessment of the RV stability of CRIRES”, A&A 491 (3) 929-939 (2008) T. Travouillon, L. Jolissaint, M. C. B. Ashley, J. S. Lawrence, and J. W. V. Storey, “Overcoming the Boundary Layer Turbulence at Dome C: G ...
B/W
B/W

The brightest ULIRG: watching the birth of a quasar
The brightest ULIRG: watching the birth of a quasar

Light Energy
Light Energy

... of image. Light is reflected from the paper of this book also but the surface of paper is much rougher than mirrors. That is why no image is formed by the paper. You might have seen people putting frosted window glass pane? Have you ever thought why are frosted glass used? The frosted glass has a ro ...
Sterrenstelsels en Cosmologie Docent: M. Franx, kamer 425
Sterrenstelsels en Cosmologie Docent: M. Franx, kamer 425

... magnitude (which would be appropriate for a star). Hence we measure the amount of light per area on the sky. This is called the surface brightness. It is often expressed as magnitude per square arcsec. How to measure average surface brightness profile ? Measure the intensity on ellipses of (nearly) ...
Galaxy Formation Leading questions for today • How do visible
Galaxy Formation Leading questions for today • How do visible

Section Notes Ch 2
Section Notes Ch 2

Lecture 24, The local group
Lecture 24, The local group

Functions of the Gravitational Potential
Functions of the Gravitational Potential

Galaxy Image Classification using Non
Galaxy Image Classification using Non

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... Star System – consists of a star (sometimes more than one star) and all the objects that orbit it. ...
L133 DIRECT DETECTION OF LARGE CLOSE
L133 DIRECT DETECTION OF LARGE CLOSE

... we show light curves one would expect under various assumptions about the lens and source systems. If the planet is very close to the primary a & 0.03 AU, relatively large R p * 1.5 RJup, or the lens has a low mass Mlens & 0.3 M,, then the magnitude of the deviation can be quite substantial (d p * 1 ...
File
File

... Periscope is an instrument for observation from a concealed position. In its simplest form it is a tube in each end of which are mirrors set parallel to each other and at an angle of 45° with a line between them. A periscope may be used as a toy or for seeing over people's heads in a crowd. This for ...
Ch. 22
Ch. 22

Section 2 Thin Lenses Chapter 14 Sample Problem, continued
Section 2 Thin Lenses Chapter 14 Sample Problem, continued

distancesinastronomy
distancesinastronomy

... THE EARTH: 1/10th of a light-second all the way around ...
Age patterns in a sample of spiral galaxies
Age patterns in a sample of spiral galaxies

SEIR™ Optic Technology
SEIR™ Optic Technology

Visible Light
Visible Light

The Eye - My Anatomy Mentor
The Eye - My Anatomy Mentor

... ◦ Light rays change speed as they pass through substances of different densities ◦ Light is refracted in 3 areas of the eye:  Cornea  Entrance of lens  Exit of lens ...
General Relativity and Gravitational Waves
General Relativity and Gravitational Waves

light1
light1

... atom through the bulk of the material; rather the electrons vibrate for short periods of time and then reemit the energy as a reflected light wave  Metals are opaque- free electrons will vibrate easily and reflects light…. This is why metals are shiny ...
Gravitational Waves from Neutron Stars
Gravitational Waves from Neutron Stars

g= -(1-~)dt2+(1- ~r! g= -(1-~)dt2+(1
g= -(1-~)dt2+(1- ~r! g= -(1-~)dt2+(1

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Gravitational lens

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