All Tables
- Table 1:
Slopes of the linear fits to the logarithm of the mean weighted PWTs without any
correction for the magnitude of
the stars.
- Table 2:
Slopes of the linear fits to the logarithm of the mean weighted PWTs with
a linear correction for the magnitude of the stars
before averaging.
- Table 3:
Slopes of the linear fits to the logarithm of the mean weighted PWTs
leveling up all the stars of each spectral
type to have the same level of noise above 3 mHz.
- Table 4:
Slopes of the linear fits to the logarithm of the mean weighted PWTs
for sub-samples of the analysed stars and without any
correction for the magnitude of
the stars.
- Table 5:
Parameters A1 (in arbitrary units) and
(in seconds), related to the granular contrast
and its characteristic lifetime,
obtained from the weighted
average PWTs.
- Table 6:
Slopes of the linear fits to the logarithm of the PWTs
of the solar series for 480 days of data.
- Table 7:
Slopes of the linear fits to the logarithm of the PWTs
of the solar series for 54 days of data analysed as the stellar data,
including its observed window function.
- Table 8:
Ratios of the parameters A1 (obtained at maximum and minimum of
the solar activity) and A2. These parameters are related with the granular
and super-granulation contrast,
obtained from a non-linear fit of Eq. (1) to the solar PWTs.