New Worlds, New Horizons with X-ray Astronomy

Thursday, February 20, 2014

Planning the Future of U.S. Particle Physics (Snowmass 2013): Chapter 1: Summary. (arXiv:1401.6075v1 [hep-ex])





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Planning the Future of U.S. Particle Physics (Snowmass 2013): Chapter 4: Cosmic Frontier. (arXiv:1401.6085v1 [hep-ex] CROSS LISTED)





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C IV absorption line variability in X-ray bright BALQSOs. (arXiv:1401.5593v1 [astro-ph.CO])





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X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue. (arXiv:1402.0004v1 [astro-ph.HE])





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Development of Multilayer Readout Wiring TES Calorimeter for Future X-ray Missions. (arXiv:1402.0285v1 [physics.ins-det])





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Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive. (arXiv:1401.7995v1 [astro-ph.SR])





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{\it NuSTAR} Reveals an Intrinsically X-ray Weak Broad Absorption Line Quasar in the Ultraluminous Infrared Galaxy Markarian 231. (arXiv:1402.4811v1 [astro-ph.HE])





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Tuesday, February 18, 2014

Can AGN feedback break the self-similarity of galaxies, groups, and clusters?. (arXiv:1401.5067v1 [astro-ph.CO])





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Evolution of multiple supernova remnants. (arXiv:1401.5070v1 [astro-ph.GA])





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The soft X-ray emission of Ark 120. XMM-Newton, NuSTAR, and the importance of taking the broad view. (arXiv:1401.5235v1 [astro-ph.HE])





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A cosmic web filament revealed in Lyman-alpha emission around a luminous high-redshift quasar. (arXiv:1401.4469v1 [astro-ph.CO])





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Magnified Views of the Ultrafast Outflow of the z = 1.51 AGN HS 0810+2554. (arXiv:1401.4486v1 [astro-ph.HE])





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Hydrodynamical simulations of coupled and uncoupled quintessence models I: Halo properties and the cosmic web. (arXiv:1401.5005v1 [astro-ph.CO])





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Monday, February 17, 2014

The XMM-Newton spectral-fit database. (arXiv:1402.3041v1 [astro-ph.CO])





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Sunday, February 16, 2014

Evaluation of the surface strength of glass plates shaped by hot slumping process. (arXiv:1402.3445v1 [astro-ph.IM])





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Wednesday, February 12, 2014

Detection of An Unidentified Emission Line in the Stacked X-ray spectrum of Galaxy Clusters. (arXiv:1402.2301v1 [astro-ph.CO])





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Wednesday, February 5, 2014

Mass and radius constraints for compact stars and the QCD phase diagram. (arXiv:1402.0478v1 [astro-ph.HE])





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What does a measurement of mass and/or radius of a neutron star constrain? Equation of state or gravity?. (arXiv:1402.0488v1 [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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