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2 Jul 2014: 24 661 5566HD 33564 100/160 219019/20 705 720HD 39091 100/160 205212/13 502 576HD 40307 70/160 203666/67 471 180. ... 2012); (22)Bonfils et al. (2005); (23) Noyes et al. (1997); (24) Butler etal.

18 Oct 2014: at wavelengths of 24 µm or shorter (Beichman et al. 2006a; Lawler et al. ... In comparison, of the. 24 stars that have no cold excess, none show a KIN excess.

10 Dec 2014: 11 and 12) is solved to obtain fractional pop-ulations xj for all levels up to jmax=24.

2 Jul 2014: low inclination planets. a plt (. au). 24.8. 25.0. e plt.

4 Dec 2014: The Large Synoptic Survey Telescope (LSST) is ex-pected to detect objects to an apparent magnitude limitof m 24.5 (Moro-Mart́ın, Turner & Loeb 2009).

4 Dec 2014: Consequently, we find that thedisc detection rates are: 21/86 = 24 5 per cent at 100 µm and15/86 = 17 4 per cent at 160 µm. ... Mi. HD. 8769. 6A. 7V28. 24. 450. UM. a(3. ,4). 22.0.

23 Jan 2014: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 23 January 2014 (MN LATEX style file v2.2). Stochastic accretion of planetesimals onto white dwarfs:. constraints on the mass distribution of accreted material. from atmospheric pollution. M.

17 Dec 2014: 2007).η Tel: The debris disk of this system was resolved. in the mid-IR at a radius of 24 au, but it was shownthat there is an additional unresolved component ... limits at just one wavelength (left-pointing for upper limits at 70 µmand down-pointing

2 Oct 2014: Tube Number pH. 1. 7.12. 7.23. 6.24. 6.75. 5.86. 6.97. 5.18.

2 Oct 2014: MD1-14 is presented as a 24 x 10† mL stock conditions 2 x 10 mL of 5 different pH’d buffers. ... 24 0.8 M Na formate 8% PEG 20,000 8% PEG 500 MME.