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MATHEMATICAL TRIPOS Part III Friday, 27 May, 2016 1:30 ...
https://people.ast.cam.ac.uk/~wyatt/psd_exam2016.pdf16 Sep 2016: 1 2B 0 0 20 1 B 2 0. . . -
MNRAS 000, 1–6 (2016) Preprint 13 July 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/agwk16.pdf13 Jul 2016: The occurrence rate of dippers in co-eval clusters (e.g.,20–30% of classical T Tauri stars in NGC 2264; Alencaret al. ... However, giant planets alone likely cannot account forall the dippers, as dipper occurrence rates (e.g., 20–30% inNGC 2264; -
Draft version December 23, 2016Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/cmws17.pdf23 Dec 2016: 0.00005. 0.0005. 20 40 60 80 100. 17. 16. 15. 14. ... star with luminosity 20.97 L, and the 8 µm blowoutsize of the silicate-carbon mixture. -
Astronomy & Astrophysics manuscript no. letter_HD206893 c©ESO…
https://people.ast.cam.ac.uk/~wyatt/mhcc16.pdf2 Dec 2016: 2016), where a 3015 MJup brown dward wasdetected at 20 au of its host star, within a debris disc of innerradius 75 au. ... 40. 20. 0. 20. 40. 60. 80. 100. Surface. Brigh. tnessin. -
ms.dvi
https://people.ast.cam.ac.uk/~wyatt/wmke16.pdf10 Nov 2016: For star subtraction, we usedthe LOCI algorithm (Lafreniere et al. 2006) to subtract the best linear combination of library (not science) images fromeach science image, in annular rings of 20 pixels, ... Appendix D: Detection limits on planetary -
arX iv:1 604. 0828 6v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/mcbe16.pdf29 Apr 2016: Instead we calculated an expectation valueof 1.20 for thepgreen:pPlanetPolratio based on normalised prob-. ... 4 20.1 17.6 22.6 17.5 19.2 1.18 58.7 27.0. -
Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...
https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf21 Jul 2016: The entire passbandwas first fitted with a high-order polynomial, in order to fully usethe information present, and excluding only a region of 20 chan-nels of 1.27 km/s -
arX iv:1 601. 0686 6v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/dhmh16.pdf27 Jan 2016: 0 10 20 30 40 50 60Elapsed time [s]. 0.1. 1.0. ... 10.0. 100.0. Inst. anta. neou. s nu. ll de. pth. [%]. -2 0 2 4 6Instantaneous null depth [%]. 0. 20. 40. -
MNRAS 000, 1–21 (2016) Preprint 23 September 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mdwk16.pdf23 Sep 2016: 4 L. Matrà et al. -200 -100 0 100 200. -60-40-20. ... 60-40-20. 0204060. Ste. lloce. ntr. ic d. ista. nce. (A. U). -
MNRAS 000, 1–12 (2015) Preprint 12 May 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mmsw16.pdf17 May 2016: 1 INTRODUCTION. Recent surveys have shown that at least 20% of nearby solar-typestars (FGK) host Kuiper belt analogue debris discs (Hillenbrandet al. ... 20406080. r. [AU. ]. 40 80 120. 160. r0 [AU]20 40 60 80. -
MNRAS 000, 1–22 (2016) Preprint 7 November 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mwpm16.pdf7 Nov 2016: 2014 Dec 25 72-83 38 48 20 60 3c279 J1256-0547 J1245-1616. ... 2015 Jan 01 62-77 37 48 20 50 Titan J1256-0547 J1245-1616. -
Mon. Not. R. Astron. Soc. 000, 1–16 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/kwcp16.pdf7 Jun 2016: Fig. 9b gives the temperature profile expected for thegas. From 10 to 20 AU, the temperature scales as R1/3. ... 9d. Here also 3 regimes can be distinguished.Between 20 and 200AU, H/R is shallow and scales R0.1. -
arX iv:1 610. 0071 4v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wbjm16.pdf7 Oct 2016: 7 of T93). Mp = 0.8 103M1/2 a3/4p a3/4f ρ1/20 , (5). ... age; e.g., if Neptune andUranus were each Earth mass then the Oort Cloud wouldbe at 1000 au, but would take 20 Gyr to form. -
Space Science Reviews manuscript No.(will be inserted by the ...
https://people.ast.cam.ac.uk/~wyatt/wj16.pdf15 Mar 2016: Space Science Reviews manuscript No.(will be inserted by the editor). Insights into planet formation from debris disks. II. Giant impacts in extrasolar planetary systems. Mark C. Wyatt Alan P. Jackson. Received: date / Accepted: date. Abstract Giant
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