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1 Mar 2011: WFCAM simulations - PSF and galaxy tests. 01-09-2003. 03-10-2003 [html]. ... VDF-TRE-IOA-00012-0001. Interleaving tests. 25-09-2003. 29-10-2004 [html].

19 Dec 2011: in the interim he released the processed VST test data to the ATLAS and VPHAS PIs via a simple passwd-protected web page - ongoing ALL - progressed as much as possible all ... There will be a VPHAS meeting here at the IoA November 14-15 to discuss among

11 Apr 2011: EGS - checked the EVALSO test file internet transfers from ESO Garching to AKY Cambridge and found that for the month of data under consideration a total of 8 files were missing ... We also heard news that the VST test camera is on and delivering Image

19 Dec 2011: There was much discussion of observing strategy and the results from the test data taken so far (any choice bits are incorporated in the VST section). ... image tests, require much more effort to characterise and attempt to find solutions for.

27 Sep 2011: EGS will find out if the EVALSO test transfers will recommence since getting more data more quickly would be useful here Upcoming: 27/06/11: the next VMC skypecon - will probably ... At some point, after yet more tests, this will require a re-run of all

10 Jun 2011: tests suggest (mostly) harmless 9. CASUHELPSs ------------- No corkers this month. ... JRL EGS JRL - sneakily attempt to get some VST data during 6th June meeting MJI - implement WFCAM astrometric fixes as revealed by GPS tests EGS - chew over the ESO

22 Oct 2011: The new server for VST, apm45, was spec'd, cost'd, ordr'd, delivr'd and installed and is rapidly filling up with assorted VST test data for ATLAS, VPHAS and ... To add to the pressure there will be a VPHAS meeting at the IoA November 14,15 to discuss the

26 Jan 2011: EGS will look at the impact of grouting on a sample of VVV data to extend these tests to more traumatic fields before we commit. ... With the grouting procedure in place, and assuming remaining tests go well, the plan is that all existing tile catalogues

25 Mar 2011: R is now 200 microns. This is very large on a quantum scale, but small on the scale used to test gravity in experiments – close to current limit of 100 ... Plot shows signal for a 1.5 TeV resonance, in the test model.

11 Mar 2011: EGS has been monitoring the internet transfer of data from ESO to CASU following JPE's request for a test on the efficiency.

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.