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Cited article:

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XMM–Newtonlarge program on SN1006 – I. Methods and initial results of spatially resolved spectroscopy

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The Nature of a Cosmic-Ray Accelerator, CTB 37 B, Observed with Suzaku and Chandra

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Cosmic ray acceleration parameters from multi-wavelength observations. The case of SN 1006

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Evidence of a Curved Synchrotron Spectrum in the Supernova Remnant SN 1006

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In which shell-type SNRs should we look for gamma-rays and neutrinos from P–P collisions?

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Suzaku Wide-Band Observations of SN 1006

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Hadronic Contributions for TeV Gamma‐Ray Emission from Young Supernova Remnants

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Potential Neutrino Signals from Galactic γ‐Ray Sources

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Discovery of the Putative Pulsar and Wind Nebula Associated with the TeV Gamma‐Ray Source HESS J1813−178

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X‐Ray Observations of SN 1006 withINTEGRAL

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Astrophysics in 2005

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