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Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/bksm12.pdf5 Oct 2012: β Uma PACS 70/160 1342220802/3 2011-04-29. PACS 100/160 1342197015/6 2010-05-24. SPIRE 1342195687 2010-04-29. ... PSF fit500 4.24.9 0.420.01 3.84.9 PSF fit. -
Searching for Saturn's Irregular Satellite Swarm with Spitzer
https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf29 Jun 2012: However, progress will be difficult.Table 3 inJewitt & Haghighipour(2007) shows that the faintestknown irregulars at Saturn have R magnitudes of 24.5,3 and thedeepest survey for Uranian irregulars had ... 3 The faintest published survey hasR = 24.5 -
arX iv:1 211. 4898 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/lmsk12.pdf24 Nov 2012: Finally, we used the SPIRE 3σ upper limits as a constraint toreject any model with a flux density of the dust emission largerthan 24 mJy at 250µm. ... The upper inset zooms on the IRS wavelengths and displays spectra asSν(λ/24)2 on a linear scale -
Observing Kepler stars with WISE
https://people.ast.cam.ac.uk/~wyatt/kw12.pdf7 Jul 2012: Also shown is the sensitivity with MIPS at 24 and 70µm to55 Cancri, a typical nearby star at 12pc withKs 4.2 (grey lines). -
1 A SELF-CONSISTENT MODEL OF THE CIRCUMSTELLAR DEBRIS CREATED ...
https://people.ast.cam.ac.uk/~wyatt/jlcm12.pdf23 Oct 2012: which could be readily detectable around other stars by Spitzer 24 μm surveys for 25 Myr after. ... SiO h (24). which occurs with a rate coefficient m3 s-1 (Andreazza et al. -
Dynamical effects of stellar massloss on a Kuiperlike belt
https://people.ast.cam.ac.uk/~wyatt/bmw11.pdf22 May 2012: However, the lowest mass planets scatter test particles moreweakly and thus fewer test particles end up with e > eSD = 0.24,our definition of the scattered disc and MSD is low -
mnr_20522_LR
https://people.ast.cam.ac.uk/~wyatt/vw12.pdf30 Oct 2012: 2009), with q 24 au and a 796 au, and 2000 OO67 (Veillet, Doressoundiram &. Marsden 2001; Millis et al. 2002), with q 21 au and a 552 au.The perihelia and -
cv.dvi
https://people.ast.cam.ac.uk/~gpe/cv.pdf24 Jan 2012: CURRICULUM VITAE. FULL NAME: George Petros EFSTATHIOUNATIONALITY: BritishDATE OF BIRTH: 2nd Sept 1955. QUALIFICATIONS. Dates Academic Institution Degree. 10/73 to 7/76 Keble College, Oxford. B.A. in Physics10/76 to 9/79 Department of Physics, Ph.D. -
The Astrophysical Journal, 701:2019–2032, 2009 August 20…
https://people.ast.cam.ac.uk/~wyatt/lcwm09.pdf1 Aug 2012: edu. Received 2008 November 24; accepted 2009 June 16; published 2009 August 7. ... This agrees well with the200 K temperature of the large, cool grain dust grains fromthis work, and with Wyatt et al.’s (2007b) Spitzer 24/70 μmbased estimate of 4–5 -
arX iv:1 201. 3622 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/ramb12.pdf19 Jan 2012: 0 2 4 6 8 10 12 14 16 18 20 22 24 26 28 300.0.
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