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19 Feb 2003: data/cass36h/wfc_nonsurvey/watson_jul2000_reduced/:Y:Y:Y:S:S:S:S:0.080/0.004/0.016/17:a href=./lplogs/20000725.int:: ... Y:Y /data/cass36h/wfc_nonsurvey/watson_jul2000_reduced/:Y:Y:Y:S:S:S:S:0.095/0.005/0.022/18:a href=./lplogs/20000726.int::

17 Nov 2005: 3:PATT-XID:Y:Y /data/cass36h/wfc_nonsurvey/watson_jul2000_reduced/:Y:Y:Y:S:S:S:S:0.080/0.004/0.016/17:./lplogs/20000725.int:: ... 26:3:PATT-XID:Y:Y

15 Apr 2024: Mark Wyatt. My research mostly focusses on the formation and evolution of stars and their planetary systems. In particular I am interested in the dusty debris material that surrounds some stars, including the Sun, during their main sequence phase.

25 Sep 2002: ac.uk To: Weimin Yuan wmy@ast.cam.ac.uk, Jonathan Tedds jat@star.le.ac.uk, Mike Watson mgw@star.le.ac.uk Subject: Almanac Info for Dates of UKIRT

5 Jun 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J.

29 Apr 2008: Astronomy & Astrophysicsmanuscript no. 8719 c ESO 2008April 28, 2008. The Nature of Mid-Infrared Excesses From Hot Dust AroundSun-like Stars. R. Smith1,2, M. C. Wyatt1, and W.R.F. Dent3. 1 Institute of Astronomy, University of Cambridge, Madingley

22 Aug 2014: arX. iv:1. 408. 4116. v1 [. astr. o-ph. EP. ] 18. Aug. 201. 4Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 20 August 2014 (MN LATEX style file v2.2). Do Two Temperature Debris Disks Have Multiple Belts? G. M. Kennedy, M. C. WyattInstitute

23 Jul 2014: primordial protoplanetary disk (Watson et al.

23 Nov 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J.

29 Apr 2016: arX. iv:1. 604. 0828. 6v1. [ast. ro-p. h.E. P]. 28 A. pr 2. 016. DRAF T VERS IONA P RIL 29, 2016Preprint typeset using LATEX style emulateapj v. 5/2/11. POLARIZATION MEASUREMENTS OF HOT DUST STARSAND THE LOCAL INTERSTELLAR MEDIUM. J. P. MARSHALL 1,2,

4 Dec 2014: MNRAS 445, 2558–2573 (2014) doi:10.1093/mnras/stu1864. An unbiased study of debris discs around A-type stars with Herschel. N. D. Thureau,1‹ J. S. Greaves,1 B. C. Matthews,2,3 G. Kennedy,4 N. Phillips,5. M. Booth,2,3,6 G. Duchêne,7,8 J.

23 Dec 2017: WATSON,130 R.C. WEIR,4. KLAUS WENZEL,131 MICHAEL W. WILLIAMSON,56 JASON T. WRIGHT,10, 11, 132 M.

2 Nov 2015: Accepted to ApJ: October 28, 2015Preprint typeset using LATEX style emulateapj v. 5/2/11. YOUNG “DIPPER” STARS IN UPPER SCO AND ρ OPH OBSERVED BY K2. M. Ansdell1,10, E. Gaidos2,3,4,10, S. A. Rappaport5, T. L. Jacobs6, D. M. LaCourse6, K. J. Jek6

15 Mar 2016: Space Science Reviews manuscript No.(will be inserted by the editor). Insights into planet formation from debris disks. II. Giant impacts in extrasolar planetary systems. Mark C. Wyatt Alan P. Jackson. Received: date / Accepted: date. Abstract Giant

16 Jun 2015: Spot a 00:47:33.410 -25:17:13.6 Spot i 00:47:33.013 -25:17:18.12 Spot n 00:47:33.063 -25:17:17.20

19 Feb 2018: MNRAS 475, 3046–3064 (2018) doi:10.1093/mnras/stx3188Advance Access publication 2017 December 11. Analysis of the Herschel DEBRIS Sun-like star sample. B. Sibthorpe,1,2‹ G. M. Kennedy,3 M. C. Wyatt,4 J.-F. Lestrade,5 J. S. Greaves,6. B. C.

31 Jul 2018: MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled using MNRAS LATEX style file v3.0. A gap in the planetesimal disc around HD 107146 andasymmetric warm dust emission revealed by ALMA. S. Marino,1?, J. Carpenter,2 M. C. Wyatt1, M. Booth3, S.

5 May 2017: arX. iv:1. 701. 0656. 8v1. [as. tro-. ph.S. R]. 23. Jan. 2017. rsos.royalsocietypublishing.org. Research. Article submitted to journal. Subject Areas:. astrophysics, extrasolar planets, stars. Keywords:. variable stars, protoplanetary disks,. debris

25 Nov 2015: arX. iv:1. 511. 0591. 9v1. [ast. ro-p. h.E. P]. 18 N. ov 2. 015. Mon. Not. R. Astron. Soc.000, 1–18 (2002) Printed 19 November 2015 (MN LATEX style file v2.2). IR-excesses around nearby Lambda Boo stars are caused by debrisdisks rather than ISM

29 Oct 2013: Le Bouquin et al. 2009; Watson et al.2011; Kennedy et al.