Atomic data for K-shell emission of Fe-peak elements used in our recent paper
"A Chandrasekhar Mass Progenitor for the Type Ia Supernova Remnant 3C 397 from
the Enhanced Abundances of Nickel and Manganese"
(Yamaguchi et al., 2015, ApJL, 801, L31)
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Centroid Energies
Cr Kα Mn Kα Fe Kα Fe Kβ Ni Kα
Emissivities
Cr Kα Mn Kα Fe Kα Fe Kβ Ni Kα
Emissivity Ratios
Cr/Fe (Kα) Mn/Fe (Kα) Ni/Fe (Kα) Mn/Cr (Kα) Fe Kβ/Kα
All Data
Each FITS file contains image data in the primary extension (in the same format as presented in Fig. 3 of our paper) and binary table data for the electron temperatures given as the name of each subsequent extension.
The data might be updated without notice.
Please contact us at hiroya.yamaguchi -at- nasa -dot- gov if you'd like to use them for your publications.
Other References
AtomDB Website The above data were calculated based on the latest version (v.3.0.0) of AtomDB
A. R. Foster et al., in preperation Paper regarding the updated NEI models
Yamaguchi et al., 2014, ApJ, 780, 136 Fe Kα and Kβ emission data for individual charge numbers