Table 3
Cosmological constraints on the uncoupled Galileon model from the SNLS3 and JLA samples.
Sample |
![]() |
![]() |
![]() |
![]() |
α | β |
![]() |
![]() |
χ 2 |
|
|||||||||
SNLS3 Stat+sys |
![]() |
![]() |
![]() |
![]() |
1.428 | 3.263 | 23.997 | 23.950 | 415.4 |
|
|||||||||
JLA Stat+sys |
![]() |
![]() |
![]() |
![]() |
0.141 | 3.101 | 24.072 | 24.081 | 692.8 |
Notes. Results were computed using statistical and systematic
uncertainties combined. α and β were kept fixed to
their marginalised values. No errors are given on
and
because
they were analytically marginalised over (see Conley
et al. 2011).
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