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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.

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

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::

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

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.

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

23 Nov 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

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,

28 Oct 2013: von Braun K. et al., 2011, ApJ 729, L26. Watson C.A.

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 Feb 2012: was performed, with 1 cycle of 6 s integration at eachposition (Watson et al.

14 Nov 2013: 2009).The suggestion that the entire HR 8799 system may be. coplanar is consistent with the results of Watson et al.(2011) and Greaves et al.

17 Dec 2014: Five steps in the evolution from protoplanetary to debrisdisk. M. C. Wyatt • O. Panić • G. M. Kennedy •. L. Matrà. Abstract The protoplanetary disks seen around Her-big Ae stars eventually dissipate leaving just a tenuousdebris disk,

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.

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,

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