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10 Feb 2021: Frasca A., Biazzo K., Alcalá J. M., Manara C. F., Stelzer B., Covino E.,Antoniucci S., 2017,A&A, 602,A33.

20 Nov 2019: P., Tollerud, E. J.,. et al. 2013, A&A, 558, A33. Astropy Collaboration, Price-Whelan, A.

30 Jul 2018: The HOSTS Survey for Exozodiacal Dust: Preliminaryresults and future prospects. Ertel, S.a, Kennedy, G. M. b,c, Defrère, D.d, Hinz, P.a, Shannon, A. B.e,f, Mennesson, B.g,Danchi, W. C.h, Gelino, C.g, Hill, J. M.i, Hoffmann, W. F.a, Rieke, G.a,

9 Nov 2018: MNRAS 000, 1–11 (2015) Preprint 9 November 2018 Compiled using MNRAS LATEX style file v3.0. An automated search for transiting exocomets. Grant M. Kennedy,1,2? Greg Hope,3 Simon T. Hodgkin,3 Mark C. Wyatt31Department of Physics, University of

17 Apr 2013: Dashed line:analytical prediction from the Heppenheimer–Kaula theory. and. A. Gm/a33. 4μα2ᾱ, (7).

19 Jul 2021: Draft version February 20, 2021Typeset using LATEX default style in AASTeX63. SpiKeS: Precision Warm Spitzer Photometry of the Kepler Field. Michael W. Werner ,1 Varoujan Gorjian ,1 Farisa Y. Morales ,1 John H. Livingston ,2. Grant M. Kennedy ,3, 4

21 Feb 2019: MNRAS 000, 000–000 (2018) Preprint 21 February 2019 Compiled using MNRAS LATEX style file v3.0. Asymmetric mid-plane gas in ALMA images of HD 100546. J. M. Miley1?, O. Panić 1, T. J. Haworth 2, I. Pascucci 3, M. Wyatt 4, C. Clarke 4,. A. M. S.

15 Dec 2010: arX. iv:1. 012. 3079. v1 [. astr. o-ph. EP. ] 14. Dec. 201. 0. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 15 December 2010 (MN LATEX style file v2.2). A general model of resonance capture in planetary systems:First and second order

17 Jan 2020: MNRAS 000, 1–19 (2019) Preprint 20 December 2019 Compiled using MNRAS LATEX style file v3.0. Are Inner Disc Misalignments Common? ALMA Reveals an IsotropicOuter Disc Inclination Distribution for Young Dipper Stars. M. Ansdell,1,2,3? E. Gaidos,4 C.

10 Mar 2020: Draft version March 10, 2020Typeset using LATEX twocolumn style in AASTeX62. The HOSTS survey for exozodiacal dust: Observational results from the complete survey. Ertel, S.,1, 2 Defrère, D.,3 Hinz, P.,2 Mennesson, B.,4 Kennedy, G. M.,5 Danchi, W.

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,

5 May 2017: 3/22. 2M 1/2? a33. 11 L1/L2. (18). As eq. (15) shows that the maximum value of the mu-tual inclination between the inner pair of planets cannot belarger

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 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

15 Jan 2015: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 9 January 2015 (MN LATEX style file v2.2). Capture and evolution of dust in planetary mean-motionresonances: a fast, semi-analytic method for generatingresonantly trapped disk images. Andrew