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7 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

18 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.

23 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

23 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,.