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5 Mar 2014: AOB/news 1. Actions from last meeting ----------------------------- Agenda item: progress on ALL papers - nothing much has happened on this front due to unexpected retrenching. ... There were a few minor hiccups switching to transferring and ingesting

5 Mar 2014: The new modes have involved creating and testing to destruction a new post-processing pipeline toolkit. ... the new AB magnitude zeropoints from APASS have been generated but only for the fixed catalogues.

13 Oct 2014: Curiously, there are no foreground stars. Barnard 68 seems to bea molecular cloud in the earliest phase of collapse to form new stars; for this reason it isthe subject of many

4 Dec 2014: 7/4r. Additionally, with LSST expected to survey. for 10 years, new objects should enter the sphere of detec-tion at a rate of nd/P 0.7 yr1, for a

21 Jan 2014: 2.2 Summary of observations. Based on previous data and the new observations described abovewe assign the star a spectral type of G0V. ... 3). Instead, we speculate that HD 166191and HD 163296 may represent the first members of a yet-to-be-discovered

2 Jul 2014: 1997) and New Horizons(Poppe et al. 2010; Han et al. 2011), although direct observationof the dust emission from the EKB is confounded by the brightforeground thermal emission from the zodiacal ... 2012). The final new detection, HD 40307, wasnoted in

11 Mar 2014: The new velocity v′ is simply the vector sum of the oldvelocity v and the kick velocity v and thus v′2 = v2 v2 2v v. ... This arisesfrom the requirement that the new orbit of a particle must passthrough the point at which the kick is applied that is

10 Feb 2014: 2010). The new observations were obtained with the Photodetecting Array Camera and Spectrometer. ... 2005), although our. new observations are of somewhat higher resolution and signal-to-noise.

4 Dec 2014: Grenoble Alpes/CNRS, IPAG, F-38000 Grenoble, France9School of Physics, University of New South Wales, Sydney 2052, Australia10Australian Centre for Astrobiology, University of New South Wales, Sydney 2052, Australia11Computational Engineering and

2 Jul 2014: Mon. Not. R. Astron. Soc. 000, 1–22 (2002) Printed 1 July 2014 (MN LaTEX style file v2.2). Dynamical evolution of an eccentric planet and a lessmassive debris disc. Tim D. Pearce? and Mark C. WyattInstitute of Astronomy, University of Cambridge,

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,.