All Tables
- Table 1:
XMM-Newton observation information. All observations are
performed in Full Frame with the Thin Optical filter applied except
in Rev. 175 where the Medium filter was used.
- Table 2:
The pn and MOS 1 data for all observations are
fitted in the 0.18-1.2 keV band with an absorbed BB model
including a Gaussian absorption line. The Gaussian width has
been fixed to
eV.
- Table 3:
Joint fits to all EPIC pn FF mode observations in the
0.18-1.2 keV band with absorbed BB plus absorption Gaussian line
model with a width of
eV.
The absorption is forced to be the same in all
observations. NC indicates that a parameter cannot be constrained
(i.e. the corresponding model is not required by the data).
The total
is 902 for 811 d.o.f.
- Table 4:
X-ray spectral analysis. Individual fits to the EPIC-pn and EPIC-MOS1 observations
in the energy band 0.18-1.2 keV for a purely
dipolar magnetic field structure (
),
and
.
We allow to vary the magnetic field intensity at the pole (
)
and the unredshifted
temperature at the pole (
).
- Table 5:
Joint fits to EPIC-pn FF mode observations for a purely dipolar field (
)
with
and
,
forcing the hydrogen column density,
the normalization constant and the magnetic field intensity to be the same for all observations.
The best fit yields
for 819 d.o.f.
- Table 6:
Individual fits to the EPIC-pn EPIC-MOS1 observations in the energy band
0.18-1.2 keV for a quadrupole dominated magnetic field (
)
with
and
.
We allow to vary the magnetic field intensity and the temperature at the pole.
- Table 7:
Joint fits to EPIC-pn FF mode observations for a
quadrupole dominated magnetic field (
)
with
and
,
forcing the hydrogen column density,
the normalization constant and the magnetic field intensity to be the same for all observations.
The best fit yields
for 819 d.o.f.