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J/A+A/527/A134
2559
Fe abundances for 28 XMM galaxy clusters (Matsushita, 2011)
ReadMe+ftp
2011A&A...527A.134M
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Post annotation
1.
J/A+A/527/A134/table2
Results of spectral fitting of annular spectra
(130 rows)
meta
J/A+A/527/A134/table2
Simple Constraint
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Constraints
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Column
Constraint
Explain
(
UCD
)
recno
Record number assigned by the VizieR team. Should Not be used for identification.
(
meta.record
)
(
RECORD
)
Cluster
(char)
Cluster name
(
meta.id;meta.main
)
(
ID_MAIN
)
rl
Lower value of radius interval, in units of r180
(
phys.size.radius;arith.ratio
)
(
PHYS_SIZE_RADIUS_NORM
)
ru
Upper value of radius interval, in units of r180
(
phys.size.radius;arith.ratio
)
(
PHYS_SIZE_RADIUS_NORM
)
kT
keV
Best-fit ICM temperature derived from the 1T model fits
(
phys.temperature
)
(
PHYS_TEMP_XRAY
)
e_kT
keV
1σ statistical error on kT
(
phys.temperature
)
(
PHYS_TEMP_XRAY
)
FeA
[Sun]
Best-fit Fe abundance using the ICM temperature derived from the 1T model fits (from F
FeHeK
/F
3.5–6
)
(
phys.abund.Fe;meta.modelled
)
(
PHYS_ABUND_FE/H
)
e_FeA
[Sun]
1σ statistical error on FeA
(Note 1)
(
stat.error
)
(
ERROR
)
DFeA
[Sun]
Difference in the derived FeA abundances using the best-fit multi-T model and the 1T model
(
stat.param;meta.modelled
)
(
MODEL_PARAM
)
FeB
[Sun]
(n)
Best-fit Fe abundance using the ICM temperature derived from the 1T model fits (for F
FeHK
/F
3.5–6
)
(
phys.abund.Fe;meta.modelled
)
(
PHYS_ABUND_FE/H
)
e_FeB
[Sun]
(n)
1σ statistical error on FeB
(Note 1)
(
stat.error
)
(
ERROR
)
DFeB
[Sun]
(n)
Difference in the derived FeB abundances using the best-fit multi-T model and the 1T model
(
stat.param;meta.modelled
)
(
MODEL_PARAM
)
ALL
cols
(n)
indicates a possible blank or NULL column
(i)
indexed column
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