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| v |
The acquired high-resolution spectra from Chandra
and XMM-Newton
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gratings need to be matched with equally
high-quality atomic data.
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|
| v |
For x-ray collisional plasmas, most of the
atomic data are satisfactory,
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allowing for high precision measurements of EM
structures, abundances,
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densities, and UV effects.
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| v |
PLEASE USE SPECIAL CAUTION with 2p-3s LINE
INTENSITIES,
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NON-Fe L-SHELL IONS, and the IONIZATION BALANCE.
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| v |
For x-ray photoionized plasmas, atomic data
allow for sound measurements
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of outflow velocities, temperatures, column
densities, and abundances.
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| v |
PLEASE USE SPECIAL CAUTION with
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INNER-SHELL LINE WAVELENGTHS (especially low-Z),
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the IONIZATION BALANCE (density & location),
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and FLUORESCENCE YIELDS.
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