New Worlds, New Horizons with X-ray Astronomy

Sunday, January 12, 2014

X-Ray Absorption by the Warm-Hot Intergalactic Medium in the Hercules Supercluster. (arXiv:1401.2221v1 [astro-ph.CO])





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Dust from AGBs: relevant factors and modelling uncertainties. (arXiv:1401.1332v1 [astro-ph.SR])





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The Cosmological Parameters 2014. (arXiv:1401.1389v1 [astro-ph.CO])





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Nuclear constraints on the EoS and rotating neutron stars. (arXiv:1401.1114v1 [astro-ph.SR])





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A millisecond pulsar in a stellar triple system. (arXiv:1401.0535v1 [astro-ph.SR])





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A clear and measurable signature of modified gravity in the galaxy velocity field. (arXiv:1401.0706v1 [astro-ph.CO])





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Cosmological parameter estimation from CMB and X-ray clusters after Planck. (arXiv:1401.0717v2 [astro-ph.CO] UPDATED)





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On the determination of the spin and disc truncation of accreting black holes using X-ray reflection. (arXiv:1401.1615v1 [astro-ph.HE])





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The Spin of the Black Hole GS 1124-683: Observation of a Retrograde Accretion Disk?. (arXiv:1401.1794v1 [astro-ph.HE])





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Randall Smith
I'm an astrophysicist at the Smithsonian Astrophysical Observatory in Cambridge, MA. Any opinions expressed are my personal views and not those of the Smithsonian.
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