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

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

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

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.

12 Oct 2021: H. Chen, A. Morlok, D. M. Watson, P. Manoj, P. Sheehan, T.

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

10 Feb 2002: e.q. 0100 0112570401 PROCESSING Dr Michael Watson M31 Core 00:42:43.0 41:15:46.0 59262 - - - - - - - - - - Flag of status: SAS ERROR (29) but PPS products exist?

22 Feb 2011: Finally we note that Watson Varricatt took over from Chris Davis a few months ago as the official contact person for all matters relating to WFCAM data processing.

22 May 2012: H., Sheehan, P., Watson, D. M., Manoj, P., & Najita, J.

4 Sep 2012: Watson Varricat came up with an interesting problem relating to WFCAM and crowded field photometry, e.g.

22 Aug 2010: arX. iv:1. 008. 0865. v2 [. astr. o-ph. SR. ] 6. Aug. 201. 0. Mon. Not. R. Astron. Soc.000, 1–11 (2010) Printed August 9, 2010 (MN LATEX style file v2.2). Resolved Imaging of the HD191089 Debris Disc. Laura Churcher1, Mark Wyatt1, Rachel

24 Nov 2023: Watson, E. Westra, T. Wold & C. WolfNature 461, 1254-1257(29 October 2009)doi:10.1038/nature08459.

18 Sep 2007: 842. Publications of the Astronomical Society of the Pacific, 119: 842–854, 2007 August 2007. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A. An Unbiased Survey of 500 Nearby Stars for Debris Disks: A JCMT Legacy

8 Nov 2011: arX. iv:s. ubm. it/03. 5390. 2 [. astr. o-ph. EP]. 8 N. ov 2. 011. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 8 November 2011 (MN LATEX style file v2.2). The scattering of small bodies in planetary systems:. constraints on the possible

11 Apr 2019: MNRAS 000, 1–12 (2018) Preprint 4 December 2018 Compiled using MNRAS LATEX style file v3.0. The wavelength dependence of interstellar polarization inthe Local Hot Bubble. Daniel V. Cotton1,2?, Jonathan P. Marshall3,4, Priscilla C. Frisch5,Lucyna

6 Jun 2006: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H.

20 Feb 2024: 2006 ), (14) Watson et al. ( 2011 ), (15) Sepulveda & Bowler ( 2022 ), (16) Mamajek & Bell ( 2014 ), (17) Plavchan et al. (

25 Oct 2009: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 19 October 2009 (MN LATEX style file v2.2). Collisional evolution of eccentric planetesimal swarms. M. C. Wyatt1?, M. Booth1, M. J. Payne1, L. J. Churcher11 Institute of Astronomy, University