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PPT - Cornell University
PPT - Cornell University

... peculiar velocity of a single galaxy is typically ~0.16cz For clusters, the error can be reduced by a factor , N , if N galaxies per cluster are observed ...
Integrative Studies 410 Our Place in the Universe
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teachers version.
teachers version.

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A 6% measurement of the Hubble parameter at ζ ∼ 0.45: direct

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... It is probable that our universe is infinite and has been filled with matter everywhere since the Big Bang There is also good evidence that in the early universe that the universe may have expanded much faster than the speed of light. It is possible to inflate space so that although particles are n ...
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Expected Coalescence Rates of NS/NS Binaries for Ground Based

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Full PDF

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... One type of evidence that has been used to support the Big Bang Theory is spectrum analysis. Spectrum analysis involves studying the wavelengths of light in the universe. We can study the wavelength of light from distant stars and galaxies to draw conclusions about their movement. For example, if ob ...
TF_final3 - Arecibo Observatory
TF_final3 - Arecibo Observatory

... The purpose of this research was to study the LIRGs (Luminous Infrared Galaxies) and see if they follow the Tully-Fisher relation. The LIRGs are different to normal galaxies in the fact that they emit 90% of their light i in infrared. The TullyFisher relation states that the bigger the galaxy is, th ...
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Searching for Dwarf Galaxies and Population III Star

... Currently, it is extremely difficult to estimate the likelihood of success. These sources are fainter than anything yet discovered. Extrapolating from known sources at lower redshifts is necessarily misleading because we are seeking the epoch at which both Lyman  and HeII emission are anomalously s ...
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Redshift



In physics, redshift happens when light or other electromagnetic radiation from an object is increased in wavelength, or shifted to the red end of the spectrum. In general, whether or not the radiation is within the visible spectrum, ""redder"" means an increase in wavelength – equivalent to a lower frequency and a lower photon energy, in accordance with, respectively, the wave and quantum theories of light.Some redshifts are an example of the Doppler effect, familiar in the change of apparent pitches of sirens and frequency of the sound waves emitted by speeding vehicles. A redshift occurs whenever a light source moves away from an observer. Another kind of redshift is cosmological redshift, which is due to the expansion of the universe, and sufficiently distant light sources (generally more than a few million light years away) show redshift corresponding to the rate of increase in their distance from Earth. Finally, gravitational redshift is a relativistic effect observed in electromagnetic radiation moving out of gravitational fields. Conversely, a decrease in wavelength is called blueshift and is generally seen when a light-emitting object moves toward an observer or when electromagnetic radiation moves into a gravitational field. However, redshift is a more common term and sometimes blueshift is referred to as negative redshift.Knowledge of redshifts and blueshifts has been applied to develop several terrestrial technologies such as Doppler radar and radar guns. Redshifts are also seen in the spectroscopic observations of astronomical objects. Its value is represented by the letter z.A special relativistic redshift formula (and its classical approximation) can be used to calculate the redshift of a nearby object when spacetime is flat. However, in many contexts, such as black holes and Big Bang cosmology, redshifts must be calculated using general relativity. Special relativistic, gravitational, and cosmological redshifts can be understood under the umbrella of frame transformation laws. There exist other physical processes that can lead to a shift in the frequency of electromagnetic radiation, including scattering and optical effects; however, the resulting changes are distinguishable from true redshift and are not generally referred to as such (see section on physical optics and radiative transfer).
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