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https://people.ast.cam.ac.uk/~wyatt/wmke16.pdf10 Nov 2016: With the advent of an extreme adaptive op-tics instrument like the Spectro-Polarimetric High-contrastExoplanet REsearch (SPHERE; Beuzit et al. -
Draft version December 23, 2016Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/cmws17.pdf23 Dec 2016: It summarizes previous findings aswell as results from this work. EC acknowledges support from NASA through HubbleFellowship grant HST-HF2-51355 awarded by STScI, op-erated by AURA, Inc. -
arX iv:1 601. 0686 6v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/dhmh16.pdf27 Jan 2016: 2014; Veillet et al. 2014). The LBT is locatedon Mount Graham in southeastern Arizona and is op-erated by an international collaboration among institu-tions in the United States, Italy, and ... The op-tics provide a field of view of 1010 arcsec2 with -
MNRAS 000, 1–21 (2016) Preprint 23 September 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mdwk16.pdf23 Sep 2016: before through modelling observations of op-tical and near-IR scattered light from the dust disk (e.g.Ahmic et al. -
Mon. Not. R. Astron. Soc. 000, 1–16 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/kwcp16.pdf7 Jun 2016: Mon. Not. R. Astron. Soc. 000, 1–16 (2002) Printed 7 June 2016 (MN LATEX style file v2.2). A self-consistent model for the evolution of the gasproduced in the debris disc of β Pictoris. Q. Kral?, M. Wyatt, R. F. Carswell, J. E. Pringle, L. Matrà
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