Translation of "Kosmische hintergrundstrahlung" in English

This relic radiation is known as the cosmic microwave background radiation.

The Planck satellite is to measure background radiation with previously unprecedented precision.

And hopefully, that'll give you a sense of where the cosmic microwave background radiation comes from.

The cosmic microwave background radiation is an emission of uniform, black body thermal energy coming from all parts of the sky.

What is the origin of the cosmic microwave radiation, and what have we learned from it?

The microwave pattern is the cosmic blueprint from which today’s clusters and superclusters of galaxies were built.

This is the noise that Penzias and Wilson heard -- the oldest sound that you're ever going to hear, the cosmic microwave background radiation left over from the Big Bang.

These measurements were able to rule out cosmic strings as the leading theory of cosmic structure formation, and suggested cosmic inflation was the right theory.

It starts at the epoch when the cosmic background radiation was emitted, about 379,000 years after the Universe began.

So, that's why we study things like dark matter, black holes, dark energy, and we also look at remnants of the early universe, the cosmic microwave background that satellites.

We'll talk more about this when we talk about the cosmic microwave background radiation, but at this point in the universe it was kind of this almost uniform whitehot plasma of hydrogen.

On one hand, the big bang theory is convincingly supported by observations (cosmic background radiation, Hubble’s red shift, frequency of occurrence of chemical elements in the universe), on the other hand, it cannot explain some basic properties of the universe:

Two American radio astronomers, Penzias and Wilson, discovered this cosmic background radiation in 1965, more or less by accident, when calibrating a microwave antenna which they planned to use to search for astronomic sources that could generate radio interference.

According to the CTH (G ~ t - 2/3), the effective matter- densifying gravitation force was, in the 300000 years old universe, when the matter decoupled from the radiation – wich today we still observe as cosmic background radiation- about 1000 times stronger than today!

The Heidelberg physicist studies the role played by dark energy in connection with cosmic background radiation and the structural evolution of the Universe. Another of his major research interests focuses on couplings between dark energy and dark matter.

Arno Penzias, an American physicist and Nobel laureate who co-discovered the cosmic microwave background radiation which helped establish the Big Bang, sums up what he sees,

September Learn how and when to remove this template message The cosmic microwave background radiation and the cosmological redshift -distance relation are together regarded as the best available evidence for the Big Bang theory.

The cosmic background radiation, for example, (“echo of the Big Bang”) is being investigated, as are molecular clouds in the Milky Way and in other galaxies.

Here, the Heidelberg researcher examined the role of dark energy on cosmic background radiation and the structure formation in the universe as well as possible coupling between dark energy and dark matter.

The recipients of the award include Jocelyn Bell, who was at the forefront of the discovery of the first pulsars, and Arno Penzias and Robert W. Wilson, who received the Nobel Prize in 1978 for the discovery of cosmic background radiation.

Deals with the observation and study of celestial objects (such as galaxies, stars, planets, moons, asteroids and comets) and processes (such as supernovas, explosions, gamma ray bursts and cosmic microwave background radiation).

The Hubble space telescope and the 10 meter Keck telescope in Hawaii were able to collect important information on the properties of the intergalactic medium and on cosmic background radiation in far distances which are in agreement with predictions of the big bang theory [6].

This energy exists today in the form of cosmic background radiation.

The echo of this huge explosion still reverberates today in the cosmic background radiation.

His calculations were confirmed thirty years later by the observations of thecosmic background radiation.

Bond's most famous work concerns the theoretical modeling of anisotropies of the cosmic background radiation.

It was big enough to be transparent to light, and that's what we see in the cosmic microwave background that George Smoot described as looking at the face of God.

And those fluctuations were stretched to astronomical sizes, and those fluctuations eventually are the things we see in the cosmic microwave background.

Four other proposals are still competing for the second L-mission place: a large X-ray telescope called "Athena", which among other things would research black holes, "Icy Planets", another mission to the outer planets of the solar system, "prism", a mission for the measurement of cosmic background radiation, and the "Exoplanet Finder", which would find and investigate planets similar to Earth.

The BOOMERanG experiment (Balloon Observations Of Millimetric Extragalactic Radiation ANd Geophysics) measured the cosmic microwave background radiation of a part of the sky during three sub-orbital (high altitude) balloon flights.

BICEP (Background Imaging of Cosmic Extragalactic Polarization) and the Keck Array are a series of cosmic microwave background (CMB) experiments.

He has developed data analysis tools based on information theory and applied them to Cosmic Microwave Background experiments such as COBE, QMAP, and WMAP, and to galaxy redshift surveys such as the Las Campanas Redshift Survey, the 2dF Survey and the Sloan Digital Sky Survey.

Differences in the temperature of the cosmic background are smoothed by cosmic inflation, but they still exist.