Thursday, February 20, 2014

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

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

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

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

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

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])

{\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])

Tuesday, February 18, 2014

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

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

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])

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

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

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