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arX iv:1 402. 1184 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/dawk14.pdf10 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). -
arX iv:1 312. 4531 v2 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kmlm13.pdf21 Jan 2014: Argon lamps were used for wave-length calibration. 24 images were taken with 1 second exposures. -
Mon. Not. R. Astron. Soc. 000, 1–22 (2013) Printed ...
https://people.ast.cam.ac.uk/~wyatt/jwbv14.pdf11 Mar 2014: which at 50AU from the Sun corresponds to σv/vk = 0.056,0.13, 0.27, 0.55, and 1.24. -
Five steps in the evolution from protoplanetary to debrisdisk ...
https://people.ast.cam.ac.uk/~wyatt/wpkm15.pdf17 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 -
Mon. Not. R. Astron. Soc. 000, 1–?? (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/mpwd15.pdf10 Dec 2014: 11 and 12) is solved to obtain fractional pop-ulations xj for all levels up to jmax=24. -
Mon. Not. R. Astron. Soc. 000, 1–22 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pw14.pdf2 Jul 2014: low inclination planets. a plt (. au). 24.8. 25.0. e plt. -
Irwin06draft.dvi
https://people.ast.cam.ac.uk/~wfcam/ukreview/Irwin06draft.pdf23 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 -
mn.dvi
https://people.ast.cam.ac.uk/~wyatt/wfpb14.pdf23 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.
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