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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,

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.

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.