{ "id": "1412.1172", "version": "v1", "published": "2014-12-03T03:27:18.000Z", "updated": "2014-12-03T03:27:18.000Z", "title": "ASTRO-H White Paper - New Spectral Features", "authors": [ "R. K. Smith", "H. Odaka", "M. Audard", "G. V. Brown", "M. E. Eckart", "Y. Ezoe", "A. Foster", "M. Galeazzi", "K. Hamaguchi", "K. Ishibashi", "K. Ishikawa", "J. Kaastra", "S. Katsuda", "M. Leutenegger", "E. Miller", "I. Mitsuishi", "H. Nakajima", "T. Ogawa", "F. Paerels", "F. S. Porter", "K. Sakai", "M. Sawada", "Y. Takei", "Y. Tanaka", "Y. Tsuboi", "H. Uchida", "E. Ursino", "S. Watanabe", "H. Yamaguchi", "N. Yamasaki", "for the ASTRO-H Science Working Group" ], "comment": "37 pages, 19 figures, ASTRO-H White Paper", "categories": [ "astro-ph.HE" ], "abstract": "This white paper addresses selected new (to X-ray astronomy) physics and data analysis issues that will impact ASTRO-H SWG observations as a result of its high-spectral-resolution X-ray microcalorimeter, the focussing hard X-ray optics and corresponding detectors, and the low background soft gamma-ray detector. We concentrate on issues of atomic and nuclear physics, including basic bound-bound and bound-free transitions as well as scattering and radiative transfer. The major topic categories include the physics of charge exchange, solar system X-ray sources, advanced spectral model, radiative transfer, and hard X-ray emission lines and sources.", "revisions": [ { "version": "v1", "updated": "2014-12-03T03:27:18.000Z" } ], "analyses": { "keywords": [ "astro-h white paper", "spectral features", "low background soft gamma-ray detector", "impact astro-h swg observations", "solar system x-ray sources" ], "note": { "typesetting": "TeX", "pages": 37, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1332475, "adsabs": "2014arXiv1412.1172S" } } }