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Observations, Modeling and Theory of Debris Disks Brenda C. ...
https://people.ast.cam.ac.uk/~wyatt/mkwb14.pdf7 Jan 2014: This is im-portant because it impacts disk incidences, interpretationof structures, and the identification of new cold disk pop-ulations. ... Col-lisions between SPs in intersecting orbits are modeled bygenerating a set of new SPs that represent the -
Constraining the Exozodiacal Luminosity Function of Main Sequence…
https://people.ast.cam.ac.uk/~wyatt/mmsc14.pdf18 Oct 2014: effective wavelength using a Rayleigh-Jeans assumption. These revised stellar fluxes result in new estimates. ... the goal of identifying possible new excess stars, i.e., stars with excess only present at the longest KIN. -
mn.dvi
https://people.ast.cam.ac.uk/~wyatt/wfpb14.pdf23 Jan 2014: orbiting 0.05 5 AU from their stars, but a new populationof low mass planets (220 times the mass of Earth) orbitingwithin 1 AU has been found in transit and radial -
Irwin06draft.dvi
https://people.ast.cam.ac.uk/~wfcam/ukreview/Irwin06draft.pdf23 Jul 2014: Mon. Not. R. Astron. Soc. 000, 1–26 (2006) Printed 15 May 2013 (MN LATEX style file v2.2). Pipeline processing of wide-field near-infrared data fromWFCAM (draft - not for circulation). Mike Irwin1, Jim Lewis1, Marco Riello1, Simon Hodgkin1,.
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