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Cited article:

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Spatially Resolved Chandra Spectroscopy of Supernova Remnant DEM L71 in the Large Magellanic Cloud

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X-Ray Spectroscopic Evidence of Charge Exchange Emission in the Disk of M51

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Charge Exchange X-Ray Emission Detected in Multiple Shells of Supernova Remnant G296.1–0.5

Yukiko Tanaka, Hiroyuki Uchida, Takaaki Tanaka, Yuki Amano, Yosuke Koshiba, Takeshi Go Tsuru, Hidetoshi Sano and Yasuo Fukui
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High-resolution X-ray study of supernova remnant J0453.6−6829 with unusually high forbidden-to-resonance ratio

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An exploration of X-ray Supernova remnants in the Milky Way and nearby galaxies

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Evidence for Resonance Scattering in the X-Ray Grating Spectrum of the Supernova Remnant N49

Yuki Amano, Hiroyuki Uchida, Takaaki Tanaka, Liyi Gu and Takeshi Go Tsuru
The Astrophysical Journal 897 (1) 12 (2020)

Smoothed particle inference analysis and abundance calculations of DEM L71, and comparison to SN explosion models

Jared Siegel, Vikram V. Dwarkadas, Kari Frank, David N. Burrows and Aldo Panfichi
Astronomische Nachrichten 341 (2) 163 (2020)

High Forbidden-to-resonance Line Ratio of O vii Discovered from the Cygnus Loop

H. Uchida, S. Katsuda, H. Tsunemi, K. Mori, L. Gu, R. S. Cumbee, R. Petre and T. Tanaka
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Smoothed Particle Inference Analysis of SNR DEM L71

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The Astrophysical Journal 875 (1) 14 (2019)

Chandrasekhar and Sub-Chandrasekhar Models for the X-Ray Emission of Type Ia Supernova Remnants. I. Bulk Properties

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Extended calculations of level and transition properties in the nitrogen isoelectronic sequence: Cr XVIII, Fe XX, Ni XXII, and Zn XXIV

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Multifrequency study of a new Fe-rich supernova remnant in the Large Magellanic Cloud, MCSNR J0508−6902

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High-resolution X-ray spectroscopy and imaging of the nuclear outflow of the starburst galaxy NGC 253

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Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants. II. Parameters Affecting the Spectrum

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Dirac-Fock energy levels and transition probabilities for oxygen-like Fe XIX

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