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PHD THESIS Theory and applications for transiting extrasolar planets
PHD THESIS Theory and applications for transiting extrasolar planets

... later, Johhannes Kepler discovered the planetary motion laws and at the end of 17th century, P. Laplace and E. Kant suggested the first scientific theory for planetary creation. In early 19th century, after measuring the temperature of stars, astronomers realized that stars are too hot to harbour li ...
How can double-barred galaxies be long-lived?
How can double-barred galaxies be long-lived?

Document
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... colours and does this over a shorter (from 330 nm to 680 nm) and longer (from 640 to 1050 nm) wavelength range. These measurements will in turn be used to determine the colour of each star - the portion of the spectrum where it emits most of its light - which is key to determine its temperature, age ...
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Planet Formation and Evolution: The Solar System and Extrasolar
Planet Formation and Evolution: The Solar System and Extrasolar

Polarization Study 1 Introduction
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... phase difference between the two orthogonal polarization components A0k and A0⊥ . As a result, linearly polarized light becomes elliptically polarized. There are two noteworthy cases where tan(αr ) is real and the light remains linearly polarized upon reflection: 1. Normal Incidence: θ1 = 0, which r ...
Flux Calibration of the ACS CCD Cameras SPACE TELESCOPE SCIENCE
Flux Calibration of the ACS CCD Cameras SPACE TELESCOPE SCIENCE

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Slide 1

... About 4.6 billion years old ...
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Homework extension

Birefringent Thin Films for LCDs Pochi Yeh
Birefringent Thin Films for LCDs Pochi Yeh

Non-linear Optical Microscopy and Spectroscopy for
Non-linear Optical Microscopy and Spectroscopy for

Light, Mirrors, and Lenses
Light, Mirrors, and Lenses

... Drop a rock on the smooth surface of a pond and you’ll see ripples spread outward from the spot where the rock struck. The rock produced a wave much like the one in Figure 1. A wave is a disturbance that carries energy through matter or space. The matter in this case is the water, and the energy ori ...
Introduction to Isotope Effect
Introduction to Isotope Effect

... are isotopes of the elements forming a crystal. If the impurity concentration (isotopes) in a crystal is high enough that the interaction between impurity atoms (ions) plays an important role, such a system is called a mixed crystal with a various degree of disorder. There are two types of disordere ...
Visible Light Generation of Iodine Atoms and I
Visible Light Generation of Iodine Atoms and I

... inhibited with phenyl-ethyne spacers between the carboxylic acid anchoring groups and the redox active metal center.23 There also exists some evidence that the important electron acceptor is not I3- but rather iodine, I2 or its reduced radical anion, I2-•.24 These species are present in such low con ...
Meade Introduction: 7" Mak, 8", 10" and 12"
Meade Introduction: 7" Mak, 8", 10" and 12"

Plasmon Enhanced Fluorescence (PEF) of High and Low Quantum
Plasmon Enhanced Fluorescence (PEF) of High and Low Quantum

Direct Imaging of Exoplanets - American Museum of Natural History
Direct Imaging of Exoplanets - American Museum of Natural History

... science, so each of them is valuable. Radial velocity has been very successful in measuring masses and periods of planets with masses greater than several Earths and in short-period orbits. Transits have been valuable in measuring the diameters and periods of giant planets, and in combined-light mod ...
Building a Better Flat-Field: An Instrumental Telescope
Building a Better Flat-Field: An Instrumental Telescope

... by how much. Relative magnitudes between different broadband filters, each spanning a separate range of wavelengths, can be compared to determine an object’s color. Astronomical CCD detectors convert incident photons into photoelectric measurements. But of those photons from a given source that reach ...
Colloquial Jakartan Indonesian
Colloquial Jakartan Indonesian

... record their navigational strategies. His resulting book, We, the Navigators (1972),2 is the most complete record we are likely to get of this body of knowledge, rapidly disappearing with the increased presence of motorised boats and Western navigational technology. He was also at pains to record, i ...
SkyProdigy Series Manual
SkyProdigy Series Manual

... itself with the night sky and determine where the telescope is currently pointing.The camera automatically captures an image of the sky, which is processed internally to positively identify the stars in the image. Once a positive match is found, SkyProdigy determines the coordinates of the center of ...
Maximum Mass Restraint of Neutron Stars
Maximum Mass Restraint of Neutron Stars

... star are influenced at high levels. A solid conclusion is not possible however, until more high level magnetic fields can be observed. In most cases particular temperature, pressure, and quantum state requirements must be met for significant changes in the EOS to take place. Even if just the outer l ...
Multipolarization Dynamic Light Scattering of Nonspherical
Multipolarization Dynamic Light Scattering of Nonspherical

Radiative hydrodynamics simulations of red supergiant stars. III
Radiative hydrodynamics simulations of red supergiant stars. III

... The top panel of Fig. 5 shows the temporal photocenter displacement over the ≈ 5 years of simulation, which is comparable to the total length of the Gaia mission. As seen in the Figure, for t < 22 yr, the random displacement is small and increases to a maximum value of 0.30 AU at t ∼ 23 yr. In relat ...
الشريحة 1
الشريحة 1

... and electromagnetic waves such as visible light, x-rays and radio waves. As physical objects have wave-like properties (at the atomic level), diffraction also occurs with matter and can be studied according to the principles of quantum mechanics. Richard Feynman[4] said that "no-one has ever been ab ...
chapter 6
chapter 6

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Astronomical spectroscopy



Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.
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