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4 May 2011: respectively). Some reshuffling and rationalising of the stored WFCAM and VISTA data will take place over the next few weeks as a test of the JBOD and hopefully to tidy up

22 Feb 2011: The main culprit in these tests was the Z-band where average detector zero-point offsets of /- 1% were derived in this band for the month in question (Sep 2010).

5 Apr 2011: We conclude in Section 6. In a companion paper (Raymond et al 2011; referred to in thetext as Paper 2) we test the effects of several system parameterson this process: the ... In paper 2 we test the effect of the mass distribution of giantplanets,

7 Oct 2011: 961 test particles were placed onorbits exterior to a planet of massµ = 108 and their orbits inte-grated for 10 Myr.

8 Nov 2011: Figure 2. The minimum pericentre for a test particle scatteredby a single planet, as a function of the Tisserand parameter value,from Eq. ... Figure 4. The minimum pericentre for a test particle scatteredby two planets, as a function of the ratio of the

16 Nov 2011: We test the goodness of these analytical approxima-tions by considering a close-in planet (at a0 = 2 AU) inthe robustly runaway regime of a supernova.

5 Jul 2011: Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed July 5, 2011 (MN LATEX style file v2.2). Multi-Wavelength Modelling of the β Leo Debris Disc: 1, 2 or 3planetesimal populations? L J Churcher 1†, M.C. Wyatt1, G. Duchêne2,3, B. Sibthorpe4, G.