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31 Jul 2018: MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled using MNRAS LATEX style file v3.0. A gap in the planetesimal disc around HD 107146 andasymmetric warm dust emission revealed by ALMA. S. Marino,1?, J. Carpenter,2 M. C. Wyatt1, M. Booth3, S.

25 Nov 2015: arX. iv:1. 511. 0591. 9v1. [ast. ro-p. h.E. P]. 18 N. ov 2. 015. Mon. Not. R. Astron. Soc.000, 1–18 (2002) Printed 19 November 2015 (MN LATEX style file v2.2). IR-excesses around nearby Lambda Boo stars are caused by debrisdisks rather than ISM

29 Oct 2013: Le Bouquin et al. 2009; Watson et al.2011; Kennedy et al.

5 May 2017: arX. iv:1. 701. 0656. 8v1. [as. tro-. ph.S. R]. 23. Jan. 2017. rsos.royalsocietypublishing.org. Research. Article submitted to journal. Subject Areas:. astrophysics, extrasolar planets, stars. Keywords:. variable stars, protoplanetary disks,. debris

2 Jul 2014: arX. iv:1. 403. 6186. v1 [. astr. o-ph. EP. ] 24. Mar. 201. 4Astronomy & Astrophysicsmanuscript no. dunes˙debris˙exoplanets˙v18 c ESO 2014March 26, 2014. Correlations between the stellar, planetary and debris componentsof exoplanet systems

7 Jan 2014: Observations, Modeling and Theory of Debris Disks. Brenda C. MatthewsNational Research Council of Canada – Herzberg Astronomy & Astrophysics. Alexander V. KrivovFriedrich-Schiller-Universität Jena. Mark C. WyattUniversity of Cambridge. Geoffrey

7 Oct 2016: arX. iv:1. 610. 0071. 4v1. [as. tro-. ph.E. P] 3. Oct. 201. 6. MNRAS 000, 1–25 (2016) Preprint 5 October 2016 Compiled using MNRAS LATEX style file v3.0. How to design a planetary system for different scattering. outcomes: giant impact sweet spot,

16 Jun 2015: Spot a 00:47:33.410 -25:17:13.6 Spot i 00:47:33.013 -25:17:18.12 Spot n 00:47:33.063 -25:17:17.20

5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H.

5 Jul 2011: Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed July 5, 2011 (MN LATEX style file v2.2). Multi-Wavelength Modelling of the β Leo Debris Disc: 1, 2 or 3planetesimal populations? L J Churcher 1†, M.C. Wyatt1, G. Duchêne2,3, B. Sibthorpe4, G.

28 Sep 2009: MJI is in communication with Watson Varricatt regarding the low light level non-linearity tests and also a revisit of the normal non-linearity tests. ... Watson and MJI will also be comparing dome flats with twilight sky flats.

5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H.

18 Aug 2020: MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled using MNRAS LATEX style file v3.0. Solution to the debris disc mass problem:planetesimals are born small? Alexander V. Krivov1? and Mark C. Wyatt21Astrophysikalisches Institut und

18 Feb 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J.

10 Feb 2021: MNRAS 000, 1–27 (2020) Preprint 27October 2020 Compiled usingMNRASLATEXstyle file v3.0. ALMA Survey of Lupus Class III Stars: Early Planetesimal BeltFormation and Rapid Disk Dispersal. J. B. Lovell1,M.C.Wyatt1,M.Ansdell2,M.Kama3,1, G.M.Kennedy4,5,

29 Apr 2008: Astronomy & Astrophysicsmanuscript no. 8719 c ESO 2008April 28, 2008. The Nature of Mid-Infrared Excesses From Hot Dust AroundSun-like Stars. R. Smith1,2, M. C. Wyatt1, and W.R.F. Dent3. 1 Institute of Astronomy, University of Cambridge, Madingley

25 Sep 2002: ac.uk To: Weimin Yuan wmy@ast.cam.ac.uk, Jonathan Tedds jat@star.le.ac.uk, Mike Watson mgw@star.le.ac.uk Subject: Almanac Info for Dates of UKIRT

23 Nov 2021: Publications of the Astronomical Society of Australia (PASA)doi: 10.1017/pas.2021.xxx. The formation of planetary systems with SPICA. Kamp, I.1, Honda, M.2, Nomura, H.3, Audard, M.4, Fedele, D.5, Waters, L.B.F.M.6,7, Aikawa,Y.8, Banzatti, A.9, Bowey,

2 Jul 2010: There has been a further shrinkage of staff at UKIRT. Tom Kerr is now our main contact with Watson the other UKIRT contact.

5 Jun 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J.