Similar comments can be made about the cosmic microwave background.

He found part of the cosmic microwave background radiation in 1964.

We check that against the cosmic microwave background, and it seems to hold.

For more information, see Discovery of cosmic microwave background radiation.

This is far less than the 2.7 K produced by the cosmic microwave background.

Another reference frame is provided by the Cosmic microwave background.

It was designed to measure the cosmic microwave background radiation.

Through their measurements of something called "cosmic microwave background radiation."

It started operations in 1999 to study the cosmic microwave background radiation and ran until 2008.

Other ground and balloon based cosmic microwave background experiments are ongoing.

Called the cosmic microwave background radiation, it was discovered accidentally in 1965.

In 2003, observations of the cosmic microwave background confirmed this discovery.

The light which constitutes the cosmic microwave background comes from the surface of last scattering.

The cosmic microwave background radiation was also first detected using radio telescopes.

The cosmic microwave background radiation observed today is "the most perfect black body ever measured in nature".

The cosmic microwave background was initially thought to be isotropic-it's the same where ever you look.

In some ways it is analogous to the cosmic microwave background, but at shorter wavelengths.

With the formation of neutral hydrogen, the cosmic microwave background was emitted.

This produces a "shadow" in the observed cosmic microwave background at some radio frequencies.

On 21 March 2013, the mission's all-sky map of the cosmic microwave background was released.

The best good guess of the Universe's age is 13.73 0.12 billion years old, based on what was seen of the cosmic microwave background radiation.

Recently the telescope was able to detect tiny fluctuations in the cosmic microwave background radiation.

The cosmic microwave background radiation has proven to be fertile ground for cosmologists.

These photons are still traveling today and can be detected as the "cosmic microwave background radiation."

The accidental discovery of cosmic microwave background radiation is a major development in modern physical cosmology.

It had only 45 seats, compared to the previous 52 in Cmb 13.

The CMB would then turn hard over and get out of its path.

By 1874, most significant deposits in the CMB had been found.

The line received two Cmb 13 diesel multiple units in 1927, and a third in 1930.

Without it, the CMB cannot be seen across all its frequency range.

Oh, and cmb is right, nursery rhymes are evil.

In 1927, Cmb 13 diesel multiple units were taken into use, this increasing the number of halts.

This should be more than enough data to get a very clean picture of the CMB.

This is often taken as the "time" at which the CMB formed.

I'm fairly skeptical about anyone trying to get anything out of the CMB right now.

These called for the CMB to be scanned across the full sky at least twice.

Since then, astronomers have tried to detect and interpret the CMB.

As for inflation, there are some hints that one might be able to see its effects in the CMB.

He is known especially for his work on the cosmic microwave background (CMB).

In addition the CMB provides a measurement of this scale to high accuracy.

CMB experiments have now seen this distinctive scale in temperature and polarization measurements.

"The CMB is isotropic to about one part in a hundred thousand.

Actually CMB had already withdrawn several in the 1990s.

Cosmic inflation is also necessary to address the "horizon problem" in the CMB.

This would leave an imprint on the CMB.

Posted by cmb on July 10th, 2004.

Molybdenum deposits in the CMB are of continuing interest.

The CMB was, in essence, the radiation signature of the early, expanding universe.

Another reference frame is provided by the cosmic microwave background (CMB).

This value can be calculated independently from the detailed structure of CMB fluctuations.