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Comment: An error in Fig. 10 in the published version in PRD has been
corrected in this version; an erratum has been submitted to PRD. After
correction, this figure reflects a significant difference in the ways RF and
DC readout schemes are susceptible to laser noise. In addition, the levels of
mirror loss imbalances and input laser amplitude noise have also been updated
to be more realistic for Advanced LIGO
Comment: 27 pages, lectures given at the 42nd Karpacz Winter School of
Theoretical Physics, Ladek, Poland, February 6-11, 2006
Comment: Proceedings of GWDAW-11. Corrected Challenge 2 definition (esp. Table
1), definition of polarization tensors in simulators, definition of
polarization angle in EMRIs
Comment: revised version
Comment: 9 pages (including 1 table); accepted for publication in GRG
Comment: 1 figure. Extended analysis to treat general thick branes RSII-type.
Added references
Comment: 5 pages, proceedings of the First Stueckelberg Workshop, to appear on
"Il Nuovo Cimento B"
The Pioneer 10/11 missions, launched in 1972 and 1973, and their navigation
are reviewed. Beginning in about 1980 an unmodeled force of ~ 8 x 10^{-8}
cm/s^2 appeared in the tracking data, it later being verified. The cause
remains unknown, although radiant heat remains a likely origin. A set of
efforts to find the solution are underway: a) analyzing in detail all available
data, b) using data from the New Horizons mission, and c) considering an ESA
dedicated mission.
