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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