Describes an experiment for the temperature measurement of the Cosmic Microwave Background. A radiometer is used to measure the intensity of the sky signal at 10 GHz. The radiometer is calibrated to reduce systematic effects, and the signal from a cryogenically cooled reference load is periodically measured to catch changes in the gain of the amplifier circuit over time.
AAPT Summer Meeting
Part of the Advanced Labs Workshop series
Philadelphia, Pennsylvania: July 28th - August 1st, 2012
<a href="https://advlabs.aapt.org/items/detail.cfm?ID=12506">Princeton University . "Observation of the Cosmic Microwave Background." Paper presented at the AAPT Summer Meeting , Philadelphia, Pennsylvania, July 28th - August 1st, 2012.</a>
Observation of the Cosmic Microwave Background, presented at the AAPT Summer Meeting , Philadelphia, Pennsylvania, 2012, <https://www.compadre.org/Repository/document/ServeFile.cfm?ID=12506&DocID=3145>.
Observation of the Cosmic Microwave Background. (2012, July 28th - August 1st). Paper presented at AAPT Summer Meeting , Philadelphia, Pennsylvania. Retrieved September 7, 2024, from Princeton University : https://www.compadre.org/Repository/document/ServeFile.cfm?ID=12506&DocID=3145
Princeton University . "Observation of the Cosmic Microwave Background." Paper presented at the AAPT Summer Meeting , Philadelphia, Pennsylvania, July 28th - August 1st, 2012. https://www.compadre.org/Repository/document/ServeFile.cfm?ID=12506&DocID=3145 (accessed 7 September 2024).
%0 Conference Proceedings %D July 28th - August 1st 2012 %T Observation of the Cosmic Microwave Background %B AAPT Summer Meeting %C Philadelphia, Pennsylvania %I Princeton University %S Advanced Labs Workshop %8 July 28th - August 1st %U https://www.compadre.org/Repository/document/ServeFile.cfm?ID=12506&DocID=3145
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