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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

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

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

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,

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

8 Jan 2019: MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled using MNRAS LATEX style file v3.0. A gap in HD 92945’s broad planetesimal disc revealed byALMA. S. Marino1,2?, B. Yelverton1, M. Booth3, V. Faramaz4, G. M. Kennedy5,6, L. Matrà7. and M.

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

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.

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

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,

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

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.

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

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.

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,