Issue |
A&A
Volume 373, Number 2, July II 2001
|
|
---|---|---|
Page(s) | 369 - 376 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361:20010627 | |
Published online | 15 July 2001 |
Statistical evaluation of the observational information on
and
Physics Department, High Energy Physics Division, POB 64, 00014 University of Helsinki, Finland
Corresponding author: S. M. Harun-or-Rashid, hsrashid@pcu.helsinki.fi
Received:
6
February
2001
Accepted:
27
April
2001
We undertake a critical evaluation of recent observational
information on and
in order to identify possible
sources of systematic errors and effects of simplified
statistical analyses. We combine observations for which the
results have been published in the form of likelihood contours in
the
plane. We approximate the contours by fifth order
polynomials, and we then use the maximum likelihood method to
obtain joint likelihood contours for the combined data. In the
choice of statistical merits we aim at minimum loss of information
rather than at minimum variance. We find that
, where the first error
is mainly statistical and the second error is systematical. In a flat
Universe we find
.
Key words: cosmology: observations / methods: statistical
© ESO, 2001
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