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Cited article:

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Statistical Study of the Optimal Local Sources for Cosmic Ray Nuclei and Electrons

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The Astrophysical Journal 930 (1) 82 (2022)
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A Systematic Study of the Dust of Galactic Supernova Remnants. I. The Distance and the Extinction

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The Astrophysical Journal 891 (2) 137 (2020)
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Three-dimensional dust mapping of 12 supernovae remnants in the Galactic anticentre

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Monthly Notices of the Royal Astronomical Society 488 (3) 3129 (2019)
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X-Ray and Gamma-Ray Observations of the Fermi Bubbles and NPS/Loop I Structures

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Galaxies 6 (1) 27 (2018)
https://doi.org/10.3390/galaxies6010027

Perspective on the Cosmic-ray Electron Spectrum above TeV

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G181.1+9.5, a new high-latitude low-surface brightness supernova remnant

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Astronomy & Astrophysics 597 A116 (2017)
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The connection between supernova remnants and the Galactic magnetic field: A global radio study of the axisymmetric sample

J. L. West, S. Safi-Harb, T. Jaffe, et al.
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CONSTRAINING THE AGE AND DISTANCE OF THE GALACTIC SUPERNOVA REMNANT G156.2+5.7 BY Hα EXPANSION MEASUREMENTS

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Interpretation of AMS-02 electrons and positrons data

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Radio polarization observations of large supernova remnants at λ6 cm

J. L. Han, X. Y. Gao, X. H. Sun, et al.
Proceedings of the International Astronomical Union 9 (S296) 202 (2013)
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SUZAKUOBSERVATIONS OF THE DIFFUSE X-RAY EMISSION ACROSS THE FERMI BUBBLES' EDGES

J. Kataoka, M. Tahara, T. Totani, et al.
The Astrophysical Journal 779 (1) 57 (2013)
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THE RADIO SURFACE-BRIGHTNESS-TO-DIAMETER RELATION FOR GALACTIC SUPERNOVA REMNANTS: SAMPLE SELECTION AND ROBUST ANALYSIS WITH VARIOUS FITTING OFFSETS

M. Pavlović, D. Urošević, B. Vukotić, B. Arbutina and Ü. D. Göker
The Astrophysical Journal Supplement Series 204 (1) 4 (2013)
https://doi.org/10.1088/0067-0049/204/1/4

A Suzaku Study of Ejecta Structure and Origin of Hard X-Ray Emission in the Supernova Remnant G 156.2+5.7

Hiroyuki Uchida, Hiroshi Tsunemi, Satoru Katsuda, Koji Mori, Robert Petre and Hiroya Yamaguchi
Publications of the Astronomical Society of Japan 64 (3) (2012)
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Suzaku Observations of Thermal and Non-Thermal X-Ray Emission from the Middle-Aged Supernova Remnant G156.2$+$5.7

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