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)


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


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