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Limits of Gaussian fluctuations in the cosmic microwave background at 19.2 GHz
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Limits of Gaussian fluctuations in the cosmic microwave background at 19.2 GHz
Limits of Gaussian fluctuations in the cosmic microwave background at 19.2 GHz
SB
S. P. Boughn
S. P. Boughn
EC
E. S. Cheng
E. S. Cheng
DC
D. A. Cottingham
D. A. Cottingham
DF
D. J. Fixsen
D. J. Fixsen
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1 June 1992
journal article
Published by
American Astronomical Society
in
The Astrophysical Journal
Vol. 391
,
L49
https://doi.org/10.1086/186396
Abstract
No abstract available
Keywords
UPPER BOUND
POWER LAW
LEAST SQUARES METHOD
COSMIC MICROWAVE BACKGROUND
CORRELATION FUNCTION
TEMPERATURE MEASUREMENT
COSMIC BACKGROUND RADIATION
MICROWAVES
CONFIDENCE LEVEL
MONTE CARLO METHOD
ANISOTROPY
MILKY WAY GALAXY
GAUSSIAN PROCESS
COMPUTATIONAL ASTROPHYSICS
LEAST SQUARE METHOD
MILKY WAY
SCALE INVARIANCE
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