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

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

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

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

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

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

19 Feb 2010: arX. iv:1. 002. 3469. v1 [. astr. o-ph. EP]. 18. Feb. 2010. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 19 February 2010 (MN LATEX style file v2.2). Are debris disks self-stirred? G. M. Kennedy and M. C. WyattInstitute of Astronomy,

21 Jan 2014: 4.8. Schneider et al. (2013)report a detection in the XMM-Newton Serendipitous Source Cat-alog (Watson et al.

5 Oct 2007: performed (Watson et al. 2004). The reduction and analysis of the spectra was conducted with.

7 Jul 2012: arX. iv:1. 207. 0521. v1 [. astr. o-ph. EP. ] 2. Jul 2. 012. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 5 July 2012 (MN LATEX style file v2.2). Confusion limited surveys: using WISE to quantify the rarit y ofwarm dust around Kepler stars.

6 Apr 2010: arX. iv:1. 004. 0644. v1 [. astr. o-ph. EP. ] 5. Apr. 201. 0Astronomy & Astrophysicsmanuscript no. astars˙3rd c ESO 2010April 6, 2010. Warm dusty discs: Exploring the A star 24µm debris populationR. Smith1,2 and M.C. Wyatt2. 1 Astrophysics Group,

1 Aug 2012: 2004). In order to avoid time-consuming peak-up, theobservatory was operated in IRS spectral mapping mode wherea 2 3 raster (spatial dispersion) centered on the star wasperformed (Watson et al.