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10 Feb 2014: IRS pick-up camera at 16 and 22 µm and the MIPS 24 µm photometry to establish the absolute. ... and 22 µm and MIPS 24 µm broadband fluxes (listed in Table 3).

21 Jan 2014: Argon lamps were used for wave-length calibration. 24 images were taken with 1 second exposures.

11 Mar 2014: which at 50AU from the Sun corresponds to σv/vk = 0.056,0.13, 0.27, 0.55, and 1.24.

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

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

14 Apr 2014: 4990.24 0.9262011 0.03116661. 4990.28 0.9371514 0.03115548. 4990.32 0.9425622 0.03101928. Note that this example has only three columns. ... 2. H I 0.56100 0.0004240 24.5479 0.00 0.00E00! 3. statistics for whole fit:.

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

23 Jul 2014: 1 -2.4 3.8 4.84 18.4#2 3.7 4.2 4.87 20.5#3 -9.0 4.2 5.80 24.4#4 49.1

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.