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16 Feb 2012: PARTICLE ASTROPHYSICS LECTURE 9 Tests of Inflation. Polarization: So far, we have assumed that Thomson scattering is isotropic.

5 Dec 2012: order some HBA FC cards and give it a shot using the now spare RAID array for tests. ... From now on STH will attend regular telecons, and has already downloaded some prototype NGTS test data.

27 Apr 2012: to the current IPHAS equivalent and carry out their own band-merging tests in the interim. ... After a few more tests this will be back-propagated to all the ATLAS U-band stackedimage catalogues.

24 Jul 2012: SC will contact network support downtown and see if they can shed some light since all internal tests here reveal nothing wrong. ... 9. Spectroscopic stuff ----------------------- GaiaESO pipeline tests e.g. derived velocities, are looking good and the

4 Sep 2012: This has been upgraded to use double precision in the inversion and an extra iteration and now produces sub-mas precision in forward-backward transformation tests. ... test. So far so good, but even better is to observe complete tiles for shallow surveys.

26 Jan 2012: PARTICLE ASTROPHYSICS LECTURE 2. Planck Units. :Ways of testing fundamental physics: Direct tests in accelerators (e.g. ... creating Higgs, SUSY particles) Indirect tests (e.g. radiative corrections) Low energy experiments (e.g.

5 Dec 2012: to twilights - hard to believe but needs following up with a few tests. ... To be continued. 9. Spectroscopic stuff ----------------------- Gaia-ESO the Gaia-ESO pipeline products velocity tests look good with sub-km/s accuracy.

28 Aug 2012: Tests on one night (20120104) where this problem happened with montonous regularity yield much improved results. ... 9. Spectroscopic stuff ----------------------- GaiaESO pipeline comparison test results look generally very good and there has even been

5 Dec 2012: The postgres tests on apm49 were successful which lead to a further discussion of which machines do what on the cluster aka plone and assorted DB serving for VISTA, VST, WFCAM ... After a few manual tests and some surprisingly complex scripting, it

24 Aug 2012: apm48 was duly installed and the HAWKI and VIMOS imaging data transferred across as a test. ... Tests so far indicate that a correction to the level of /-1% is achievable for the broadband u,g,r,i,z filters, and at the /-2% level for the

10 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

13 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.

22 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.

19 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

24 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.

12 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.

29 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.

9 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.

9 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

24 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.

24 Nov 2012: Hence, we conclude that this test rejects the possibility thatthe superposition of two background point sources can be re-sponsible for the central emission. ... 2011) (see also Sibthorpe et al. (2012)). Second,the spectra of these test sources removed

30 Oct 2012: Because μ is dominated by M, an isolated giantplanet would react to stellar mass loss nearly equivalently to an iso-lated test particle on the same orbit.

7 Jul 2012: However, we now test whether thesecould arise from chance alignments with background galaxies.

5 Oct 2012: To test whether this is the case for anyof our systems we have also calculated which model bestfits all images simultaneously (table 6).

23 Oct 2012: The non-unique nature of the spectral modeling allows us to test additional PSDs that can.

7 Nov 2012: Mon. Not. R. Astron. Soc. 424, 1206–1223 (2012) doi:10.1111/j.1365-2966.2012.21298.x. Herschel imaging of 61 Vir: implications for the prevalence of debrisin low-mass planetary systems. M. C. Wyatt,1 G. Kennedy,1 B. Sibthorpe,2 A. Moro-Martı́n,3

19 Jun 2012: See Section 3.2.1 for furtherinformation. point-like test particles. When a debris particle is further than100 AU from the Sun it is removed from the simulation and isconsidered to

4 Nov 2012: Indeed, the Li abundance is oftenused as a test to decide whether the atmospheric abundances can be trustedto represent the composition of the gas from which the star formed. ... It is with this idea inmind that Bergeron, Saffer, & Liebert (1992, BSL