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17 Dec 2008: As a simplified test of the model, we conduct simulations sim-ilar to those of Lufkin et al. ... entr. icity. Mass Multiplication. Middle Planet. 0. 0.05. 0.1. 0.15. 0.2.

16 Dec 2008: A simple test is to monitor the stability of the difference between ZPs derived from consecutive J and NB118 data. ... This data also provides an interesting test case for the nebulosity filter developed for GPS photometry in regions of high nebulosity.

3 Nov 2008: For eachmodel described below a range of parameters was tried and aχ2 goodness-of-fit test applied to find the best fitting parametersand confidence limits (errors from background statistical error).In ... To test whether more complicated models are

19 Aug 2008: JRL reported that he is in the middle of revamping the UKIRT archive to fix a few long standing problems with headers and legality of PHUs. ... Since then a steady stream of test data and on-sky data has been received, some directly in small doses from

8 Jul 2008: Dynamics of small bodies in planetary systems. Mark C. Wyatt. Institute of Astronomy, University of Cambridge, Cambridge CB3 0HA, UKwyatt@ast.cam.ac.uk. The number of stars that are known to have debris disks is greater than thatof stars known to

29 Apr 2008: 2000)? Or are we witnessing the colli-sional destruction of massive asteroid belts or the sublimationof comets in the middle of fully formed planetary systems? ... show three different models:Top: Face-on, large radiusr; middle: Face-on small radiusr;