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https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120118.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120118.txt10 Feb 2012: We have also done a few test processings of one of the VST GTO programmes partly to assess issues with mosaicing the whole array for projects that are using tiles as -
Astroparticle_16
https://people.ast.cam.ac.uk/~gpe/Astroparticle_16.pdf13 Mar 2012: between 1906 and 1909 to test the weak equivalence principle using a variation on the Cavendish balance. ... Membrane between attractor and test mass shields EM forces All surfaces gold plated to avoid static. -
Dynamical effects of stellar massloss on a Kuiperlike belt
https://people.ast.cam.ac.uk/~wyatt/bmw11.pdf22 May 2012: In factin these simulations no test particle has a semimajor axis less than0.5apl. ... Each test particle that is scattered in is plottedwith a discrete value of Ṁ. -
arX iv:1 201. 3622 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/ramb12.pdf19 Jan 2012: We find that the gaps between these planets arenot only dynamically stable to test particles, but are frequently populated by planetesimals. ... The gas simulations test the effect of the presence of agas disk during and after the giant planet -
midi_terr_sub3_nobold.dvi
https://people.ast.cam.ac.uk/~wyatt/swh12.pdf24 Feb 2012: As a final test for extended emission around HD113766the surface brightness profiles of the standard star imagesand HD113766 were examined. ... As a fi-nal test of the extension detection, we examine the FWHMsof the sub-integration profiles. -
arX iv:1 201. 1911 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwsd12.pdf12 Jan 2012: Prelimi-nary tests found that icy grains provided a much better fit thansilicates. ... In addition, secular per-turbations lead to precession of test particles’ nodes coupledwith inclination variations. -
Searching for Saturn's Irregular Satellite Swarm with Spitzer
https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf29 Jun 2012: Our aim here is to test this prediction for Saturn’s dustcloud using the 24µm Spitzer Space Telescope observationsused to discover the Phoebe ring. -
arX iv:1 208. 1759 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwsp12.pdf9 Oct 2012: arX. iv:1. 208. 1759. v1 [. astr. o-ph. EP. ] 8. Aug. 201. 2Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 10 August 2012 (MN LATEX style file v2.2). Coplanar circumbinary debris disks. G. M. Kennedy1, M. C. Wyatt1, B. Sibthorpe2, N. M. -
arX iv:1 205. 0004 v2 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/fgwg12.pdf9 Oct 2012: More sensitive infraredobservations can test this prediction. Detailed spectroscopy of DBZ white dwarfs has the po-tential to constrain the frequency of events that producesignificant masses of gaseous debris, or distinct -
cv.dvi
https://people.ast.cam.ac.uk/~gpe/cv.pdf24 Jan 2012: CURRICULUM VITAE. FULL NAME: George Petros EFSTATHIOUNATIONALITY: BritishDATE OF BIRTH: 2nd Sept 1955. QUALIFICATIONS. Dates Academic Institution Degree. 10/73 to 7/76 Keble College, Oxford. B.A. in Physics10/76 to 9/79 Department of Physics, Ph.D.
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