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5 Jun 2007: 7. Legacy value, serendipity, curiosity and new classes of object, 21st century Infra-Red equivalent of thePalomar-UK-ESO Schmidt Surveys. ... ESO Public Surveys Proposal Form Phase 1. 2. To discover objects cooler than the T-dwarfs and define the new Y

27 Jul 2010: Parameter Orginal value New value. Mmid 10.0 7.8 MDc 60.0 1.9kme 0.05 0.05. ... lation that incorporates the optical properties of realisticgrains, to find new values for this parameter set.

1 Feb 2008: This is still ongoing research but isleading to new perspective on debris disk evolution. ... New Hub-ble/ACS observations in scattered light show that the inner“warp” in β Pic is really a secondary disk inclined by 5with respect to the primary disk.

6 Apr 2010: Su et al. (2006) presented new 24 and 70µmphotometry which also confirms the excess.

17 Dec 2008: Greater planetary masses during the migratory stagecould allow the planets to self-excite to much greater eccentricities.Therefore, we run a new suite of simulations to look at the effectof

5 Oct 2012: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 3 October 2012 (MN LATEX style file v2.2). Resolved Debris Discs Around A Stars in the HerschelDEBRIS Survey? Mark Booth1,2†, Grant Kennedy3, Bruce Sibthorpe4, Brenda C. Matthews2,1,Mark C.

15 Dec 2010: arX. iv:1. 012. 3079. v1 [. astr. o-ph. EP. ] 14. Dec. 201. 0. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 15 December 2010 (MN LATEX style file v2.2). A general model of resonance capture in planetary systems:First and second order

15 Sep 2009: or more planets. Combining this new data with 42 already published observa-.

19 Jun 2009: Mon. Not. R. Astron. Soc. 000, 000–000 (2009) Printed 19 June 2009 (MN LATEX style file v2.2). The History of the Solar System’s Debris Disc: ObservableProperties of the Kuiper Belt. Mark Booth1?, Mark C. Wyatt1, Alessandro Morbidelli2, Amaya

4 Apr 2011: 1. SETTING THE SCENE. From the perspective of astronomers, the first decade of the new millennium has been termed the era ofprecision cosmology, when the parameters that describe our Universe have –