{"paper":{"title":"Murchison Widefield Array and XMM-Newton observations of the Galactic supernova remnant G5.9+3.1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"(10) Raman Research Institute, 11000 Belgrade, (11) International Centre for Radio Astronomy Research (ICRAR), (12) Centre for Astrophysics Research, (13) CSIRO Astronomy, (14) Research School of Astronomy, 15 Broadway, (15) School of Physics, (16) Shanghai Astronomical Observatory, 17), (17) Isaac Newton Institute of Chile, 200000, 235 Martindale Drive, (2) Western Sydney University, (3) International Centre for Radio Astronomy Research, (4) Space Science Center, (5) Max-Planck-Institut f\\\"ur extraterrestrische Physik, 6), (6) School of Physics, 7990AA Dwingeloo, (7) School of Physical Sciences, 80 Nandan Rd, 85748 Garching, (8) University of Technology Sydney, (9) Netherlands Institute for Radio Astronomy (ASTRON), ACT 2611, Adelaide 5005, A. D. Kapi\\'nska (11), A. R. Offringa (9), Astronomy, Astrophysics, Australia, Australian National University, Bangalore 560080, B. Arbutina (1), B. McKinley (14), B.-Q. For (11), Canberra, China, C. Maitra (5), College Lane, Crawley, Curtin University, C. Wu (11), Department of Earth, D. Oni\\'c (1), D. Uro\\v{s}evi\\'c (1, E. Lenc (13), Faculty of Mathematics, F. Haberl (5), Germany, G. F. Wong (2, Giessenbachstra{\\ss}e, GPO Box U1987, G. Rowell (7), Hatfield AL10 9AB, I. Boji\\v{c}i\\'c (2), India, J. Morgan (3), J. R. Callingham (9), K. S. Dwarakanath (10), KY 40351, L. E. Porter (4), L. Hindson (12), Locked Bag 1797, L. Staveley-Smith (11), M468, Marsfield, Mathematics, M. D. Filipovi\\'c (2), M. E. Bell (8), M. Johnston-Hollitt (3), Morehead, Morehead State University, N. Hurley-Walker (3), N. Maxted (2, NSW, NSW 1710, NSW 2007, Parkville, Penrith South DC, Perth WA 6845, P. J. Hancock (3), PO Bus 2, P. Procopio (15), Q. Zheng (16) ((1) Department of Astronomy, R. B. Wayth (3), School of Physics, Serbia, Shanghai Shi, Space Science, Space Sciences, Studentski trg 16, Sydney 2052, T. G. Pannuti (4), The Netherlands, The University of Adelaide, The University of Melbourne, The University of New South Wales, UK, Ultimo, University of Belgrade, University of Hertfordshire, University of Western Australia, USA, VIC 3010, WA 6009, Xuhui Qu, Yugoslavia Branch)","submitted_at":"2019-04-13T13:03:54Z","abstract_excerpt":"In this paper we discuss the radio continuum and X-ray properties of the so-far poorly studied Galactic supernova remnant (SNR) G5.9+3.1. We present the radio spectral energy distribution (SED) of the Galactic SNR G5.9+3.1 obtained with the Murchison Widefield Array (MWA). Combining these new observations with the surveys at other radio continuum frequencies, we discuss the integrated radio continuum spectrum of this particular remnant. We have also analyzed an archival XMM-Newton observation, which represents the first detection of X-ray emission from this remnant. The SNR SED is very well ex"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.06541","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}