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5 Mar 2014: One of these (apm48) will be used for update tests prior to killing off the entire lot. ... The list comes from VISTA, WFCAM, or VST. JRL will test these out shortly.

5 Mar 2014: still playing catchup due to the upgraded security EGS - took pity and sent a text file of the latest VST and VISTA grades SC - system update tests on hold but in ... Slightly hidden from view WFCAM processing continues apace with a mix of normal astro

23 Jan 2014: 2. 1. Consider a test particle orbiting a binary comprised of a star and planet of massesM and Mpl. ... ẋ′ = ẋ µα0.5(1 e2)0.5A sin nplt ,. ẏ′ = ẏ µα0.5(1 e2)0.5A cos nplt ,where µ =. MplM Mpl. and α =apla. Even though the test

23 Jul 2014: Curiously however, all three systemswith directly imaged planets (around A-stars) allow this test.Despite uncertainties about the orbit and nature of the planetaround Fomalhaut (Kalas et al. ... test binary orbital plane - disk alignment ifthe binary

17 Jul 2014: Part III, Paper 59 [TURN OVER. 4. 3. A test particle orbits a star of mass M with a semimajor axis a, eccentricity e andlongitude of pericentre ̟.

23 Jan 2014: Part III, Paper 64 [TURN OVER. 4. 3. Consider a test particle in a binary system comprised of two masses M1 and M2.The massive bodies orbit the centre of mass

4 Dec 2014: Simulations are run for 4.5 Gyrs, oruntil all test particles have been removed. ... 4 DETECTABILITY WITH LSST. To test this prediction, we want to find some asteroids in-bound from the Oort cloud.

2 Jul 2014: To investigate this, we perform a smaller sample of 50 simula-tions in which we place a circular4 disk of 100 test particles aroundFomalhaut A, with semimajor axis distributed randomly in ... Toevaluate the plausibility of this suggestion, we also

2 Jul 2014: Our systems consisted ofa massive particle representing the planet and 103 to104 massive test particles to model the disc.

22 Aug 2014: 2014). Our sample is not meant to becomplete, but to provide a sufficient number of sources for usto test whether the two-temperature disks arise from singleormultiple belts.

2 Jul 2014: 2, which were based only on far-infrared emission.To quantify the significance of any trend observed in the figureswe use the Fisher exact probability test, which has the virtue(compared ... to aχ2 test) of producing meaningful results even forlow

10 Feb 2014: nity to test theoretical models and to piece together the story of planetary systems. ... ometric tests using various permutations of a model consisting of a central source encircled by.

4 Dec 2014: MNRAS 445, 2558–2573 (2014) doi:10.1093/mnras/stu1864. An unbiased study of debris discs around A-type stars with Herschel. N. D. Thureau,1‹ J. S. Greaves,1 B. C. Matthews,2,3 G. Kennedy,4 N. Phillips,5. M. Booth,2,3,6 G. Duchêne,7,8 J.

21 Jan 2014: 2012), meaningthat we can test for differences between the BASS spectrum and theolder IRAC data (2006) at 3.5 to 4.5µm (also shown in Figure 2).The BASS/IRAC flux ... 4.2 A transition disc? To test whether HD 166191 can be modelled as a protoplane-tary

23 Jul 2014: the twilight sky is a dif-ferent colour from the dark sky, although tests of twilightflatfielded dark skies reveal no measureable effect from this).

10 Dec 2014: Mon. Not. R. Astron. Soc. 000, 1–? (2002) Printed 10 December 2014 (MN LATEX style file v2.2). CO mass upper limits in the Fomalhaut ring - theimportance of NLTE excitation in debris discs and futureprospects with ALMA. L. Matrà1,2?, O. Panić1,

17 Dec 2014: We also propose that a useful hypoth-esis to test is that the planet and planetesimal systemsseen on the main sequence are already in place dur-ing the protoplanetary disk phase, ... Hence a useful hypothesis to test is that the plan-. etary system and

23 Jan 2014: While Figs 2b and 2d provide the best estimate of theunderlying inferred accretion rate distributions in the sub-samples, we will also use Fisher’s exact test to assign a

7 Jan 2014: Bryden). As a test of such theories, many attempts have been madeto identify statistical correlations between debris and planetproperties.

18 Oct 2014: A Fisher’s exact test shows that there is only. a 0.7% chance of detecting rates as discrepant if the two groups had the same distribution.