…astrophysics. More information about Suzaku and the XIS can be found at the ISAS/JAXA Suzaku page (http://www.isas.jaxa.jp/e/enterp/missions/suzaku/index.shtml), the NASA/GSFC Suzaku Guest Observer Facility (http://heasarc.gsfc.nasa.gov/docs/astroe), and the MKI Suzaku/XIS page (http://space.mit.edu/XIS)….
…systematically, galaxy populations exhibit striking regularities, with clear trends with mass and redshift. How does this “regular complexity” emerge from the hot Big Bang? I will present results from the…
…2012, IDCS 1426 was observed using the Hubble Space Telescope and the Keck Observatory to determine its distance. Observations from the Combined Array for Millimeter Wave Astronomy indicated it was…
…accretion flow onto it is not well understood. At large scales (10^5 R_sch and beyond), the primary source of information about accretion flow comes from observations of hot X-ray emitting…
Abstract: Turbulence and magnetized disk winds are agents that can remove angular momentum and facilitate inflow through accretion disks. Initially considered as largely alternate hypotheses for why disks accrete, current…
…compact, unresolved region coincident with a strongly star-forming cluster complex, spatially separated from other clump complexes with no such ionizing emission, seen in high enough spatial resolution to obtain non-overlapping…
…formation and sub-mm line emission models. We simulate a mock lightcone of 2 deg^2 over a redshift range 0<z<10, comprising discrete galaxies and galaxy CII, CO, CI emission. We present…
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…will discuss the challenges in determining mass-observable relations, and how the combination of weak gravitational lensing and X-ray observations can address these. I will review current cluster cosmology results, including…
…The Shaw Prize Foundation announced the Shaw Laureates for 2016. Information was posted on the website http://www.shawprize.org at Hong Kong time 15:30 (GMT 07:30). The Shaw Prize consists of three…