...
In
...
this
...
page
...
you
...
find
...
the
...
spectra,
...
responses
...
and
...
background
...
files
...
necessary
...
to
...
reproduce
...
the
...
spectral
...
analysis
...
in
...
Nevalainen
...
et
...
al.,
...
2010
...
(A&A,
...
523,
...
22)
...
which
...
yielded
...
results
...
summarised
...
in
...
Fig
...
1.
...
Fig.1:
...
The
...
average
...
relative
...
difference
...
(diamonds)
...
+
...
-
...
the
...
error
...
of
...
the
...
mean
...
of
...
the
...
fluxes
...
(solid
...
line)
...
and
...
temperatures
...
(dotted
...
line)
...
for
...
different
...
instrument
...
pairs
...
in
...
the
...
soft
...
band
...
(left
...
side
...
of
...
the
...
plot)
...
and
...
in
...
the
...
hard
...
band
...
(right
...
side
...
of
...
the
...
plot)
SASv9.0
...
was
...
used
...
for
...
processing
...
the
...
XMM-Newton
...
data
...
with
...
calibration
...
information
...
from
...
December
...
2009
...
(see
...
details).
...
XMM-Newton
...
MOS1
...
and
...
MOS2
...
spectra
...
and
...
responses
...
are
...
combined
...
and
...
referred
...
to
...
as
...
MOS
...
instrument.
...
Chandra data are processed with CIAO 4.2.
...
(see
...
...
).
...
For
...
most
...
clusters
...
the
...
Chandra
...
data
...
are
...
obtained
...
with
...
ACIS-S,
...
but
...
for
...
some
...
ACIS-I
...
is
...
used,
...
and
...
marked
...
accordingly.
...
The script files bestfit....xcm
...
will
...
set
...
up
...
the
...
best
...
fit.
...
In
...
more
...
detail:
...
- The
...
- scripts
...
- use
...
- a
...
- 1-temperature
...
- phabs
...
- x
...
- mekal
...
- model.
...
- The
...
- column
...
- density
...
- is
...
- from
...
- Kalberla
...
- et
...
- al.
...
- (2005)
...
- and
...
- the
...
- absorption
...
- cross-sections
...
- are from Balucinska-Church
...
- &
...
- McCammon
...
- (1992).
...
- The
...
- scripts
...
- use
...
- the
...
- metal
...
- abundance
...
- table
...
- from
...
- Grevesse
...
- &
...
- Sauval
...
- (1998).
...
- 2.
...
- and
...
- 3.
...
- term
...
- in
...
- the
...
- script
...
- file
...
- name
...
- are
...
- the
...
- inner
...
- and
...
- outer
...
- radii
...
- of
...
- the
...
- spectrum
...
- extraction
...
- annulus
...
- in
...
- arcmin.
...
- *hard*, *soft* and *wide* refer to the fits done in 2.0-7.0
...
- keV,
...
- 0.5-2.0
...
- keV
...
- and
...
- 0.5-7.0
...
- keV
...
- bands,
...
- respectively.
...
- *fe
...
- *
...
- refers
...
- to
...
- the
...
- Fe
...
- XXV/XXVI
...
- "constr."
...
- fit
...
- in
...
- [6.45
...
- -
...
- 7.25
...
- ]/(1+z)
...
- band,
...
- i.e.
...
- with
...
- a
...
- prior
...
- for
...
- the
...
- emission
...
- measure.
...
For
...
flux
...
comparison,
...
scale
...
the
...
measured
...
fluxes
...
to
...
the
...
full
...
annulus
...
by
...
dividing
...
with
...
...
...
...
...
...
...
The following links provide a single tar file for each cluster-instrument combination, containing the spectral analysis material described above:
Cluster Instrument
A1795 XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-S
A2029 XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-S
A2052 XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-S
A2199 XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-S
A262 XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-S
A3112 XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-S
A3571 XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-S
A85 XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-I
Coma XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-I
HydraA XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-S
MKW3S XMM-Newton/pn XMM-Newton/MOS Chandra/ACIS-I
The following links contain some tabulated data from Nevalainen et al., 2010 paper in electronic form.
The first column gives the number X the of the cluster name AX, except for non-Abell names:
Coma = 1111, HydraA = 2222, MKW3S = 3333
Note that for A262 the soft and wide band temperatures are not presented, but instead marked with -999
XMM-Newton pn temperatures obtained within Chandra-driven regions
XMM-Newton pn, MOS1 and MOS2 wide band temperatures with large XMM-only regions
...
Attachments
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