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Draft version January 1, 2018Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/mwoa18.pdf2 Jan 2018: take. )C. /200. 1 A. 2 (L. INEA. R). C/2. 012. -
M. Pettini: Introduction to Cosmology — Lecture 16 DARK ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture16.pdf22 Nov 2018: Figure 16.1: M31, the Andromeda galaxy, photographed with a Canon 200 mm telephotolens. -
Analysis of the Herschel DEBRIS Sun-like star sample
https://people.ast.cam.ac.uk/~wyatt/skwl18.pdf19 Feb 2018: With the exception of HD166, with an age of 200 Myr, these five bright discs are all fairlyold systems, with a mean age of 2.5 Gyr. -
The HOSTS Survey for Exozodiacal Dust: Preliminaryresults and future…
https://people.ast.cam.ac.uk/~wyatt/ekdh18.pdf30 Jul 2018: 2002). [20] Mérand, A., Bordé, P., and Coudé du Foresto, V., “A catalog of bright calibrator stars for 200-m baselinenear-infrared stellar interferometry,” A&A 433, 1155–1162 (Apr. -
MNRAS 000, 1–23 (0000) Preprint 6 June 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mbwk18.pdf31 Jul 2018: 4.1 Planet mass and semi-major axis distribution. We consider a chain of planets on circular co-planar orbits,with masses varying from 1 to 200 M (0.63 MJup) ... Inorder to minimise random effects caused by the finite num-ber of particles used in these -
MNRAS 000, 1–13 (2018) Preprint 23 August 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/irgm18.pdf23 Aug 2018: MNRAS 000, 1–13 (2018) Preprint 23 August 2018 Compiled using MNRAS LATEX style file v3.0. Fast spectrophotometry of WD 1145017. Paula Izquierdo1,2?, Pablo Rodŕıguez-Gil1,2, Boris T. Gänsicke3,4, Alexander J. Mustill5,Odette Toloza3, -
MNRAS 000, 1–11 (2018) Preprint 27 June 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/sbbc18.pdf31 Jul 2018: year for the first thousanddays (for a drop of 0.9%), then a fast drop by 2% over 200days, followed by a slow decline for the last 200 days (Montet& Simon ... that wouldhave a duration of perhaps 200 years. -
Draft version April 5, 2018Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/mmkw18.pdf5 Apr 2018: HD 8907 34.8 F8 2.0 1.2 200 80.0 52.0 46.5 2.3e-04 1. ... HD 107146 27.5 G2V 1.0 1.0 200 88.6 126.8 37.8 8.6e-04 9. -
Debris Disks: Probing Planet Formation Mark C. Wyatt Abstract ...
https://people.ast.cam.ac.uk/~wyatt/wyat18.pdf20 Jul 2018: Fig. 3 Observations of the debris disk of the 80-200 Myr G2V star HD107146 (Marino et al., inprep.). -
MNRAS 000, 1–21 (2017) Preprint 14 June 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/wvkb17.pdf14 Jun 2018: 2017 The Authors. 2 M. C. Wyatt et al. 200 400 600 800 1000 1200 1400 1600Time (BJD-2454833). ... min(rt)/R? = (π/4)min(δobs)/max(fobs) 200, (16). Figure 4. Geometrical quantities that translate into observables.
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