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18 Jan 2018: arX. iv:1. 801. 0542. 9v1. [as. tro-. ph.E. P] 1. 6 Ja. n 20. 18Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 18 January 2018 (MN LATEX style file v2.2). ALMA observations of the narrow HR 4796A debris ring. Grant M. Kennedy1, Sebastian

2 Dec 2021: MNRAS 000, 1–23 (2021) Preprint 1December 2021 Compiled usingMNRASLATEXstyle file v3.0. Comet fragmentation as a source of the zodiacal cloud. JessicaK.Rigley,1 MarkC.Wyatt,11Institute of Astronomy, University of Cambridge, Madingley Road,

28 Sep 2006: The low sensitivityof most optical CCD detectors at 1 µm, coupled with therelatively bright sky-background curtailed interest from op-tical astronomers.

24 May 2022: DRAFT VERSION MAY 24, 2022Typeset using LATEX twocolumn style in AASTeX62. The JWST Early Release Science Program for the Direct Imaging & Spectroscopyof Exoplanetary Systems. Sasha Hinkley ,1 Aarynn L. Carter ,2 Shrishmoy Ray ,1 Andrew Skemer,2

16 Jul 2021: MNRAS 000, 1–23 (2020) Preprint 14 June 2021 Compiled usingMNRASLATEXstyle file v3.0. High resolution ALMA and HST images of q1 Eri: an asymmetricdebris disc with an eccentric Jupiter. J. B. Lovell1, S.Marino1,2,M.C.Wyatt1,

22 Nov 2018: Mon. Not. R. Astron. Soc. 000, 1–23 (2002) Printed 22 November 2018 (MN LATEX style file v2.2). Imaging [CI] around HD 131835: reinterpreting youngdebris discs with protoplanetary disc levels of CO gas asshielded secondary discs. Quentin Kral,1,2?

2 Apr 2018: arX. iv:1. 803. 1126. 5v1. [as. tro-. ph.S. R]. 29. Mar. 201. 8Draft version April 2, 2018. Typeset using LATEX twocolumn style in AASTeX61. THE HOSTS SURVEY – EXOZODIACAL DUST MEASUREMENTS FOR 30 STARS. Ertel, S.,1 Defrère, D.,2 Hinz, P.,1

26 Sep 2005: The low sensitivityof most optical CCD detectors at 1 µm, coupled with therelatively bright sky-background curtailed interest from op-tical astronomers.

2 Jul 2014: yielding the ratio of the total cross-sectional area on op-posing sides of the disc.

30 Jan 2020: MNRAS 000, 1–22 (2019) Preprint 30 January 2020 Compiled using MNRAS LATEX style file v3.0. Population synthesis of exocometary gas around A stars. S. Marino1?, M. Flock1, Th. Henning1, Q. Kral2, L. Matrà3 and M. C. Wyatt41Max Planck Institute

14 Jun 2018: Note that the derivation above has only accounted for the op-tical depth along the line of sight from the star to the dust.

22 Aug 2014: For all systems, photometry ranging from op-tical to sub-mm wavelengths is compiled from a wide vari-ety of sources, including all-sky surveys such as Hipparcos(Perryman & ESA 1997;

5 Apr 2011: In following sections we will considertheoutcome of an ensemble of many simulations, so this is an op-portunity to inspect the detailed evolution of a particularly inter-esting system.

28 Sep 2006: tuwv »¿ x v , v &,-3'T$É!' v $%3& v x2#AÎG&ÖP-!1Y, uwv x v |, v &,-3'i3&(,) yGv 3' v )s%.;.

19 Jan 2015: Draft version January 19, 2015Preprint typeset using LATEX style emulateapj v. 05/12/14. DOES THE PRESENCE OF PLANETS AFFECT THE FREQUENCY AND PROPERTIES OF EXTRASOLARKUIPER BELTS? RESULTS FROM THE HERSCHEL DEBRIS AND DUNES SURVEYS. A.