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Mark Wyatt
https://people.ast.cam.ac.uk/~wyatt/15 Apr 2024: Hull C. L. H., Yang H., Cortes P. C., Dent W. ... Cotton D. V., Marshall J. P., Frisch P. C., Kedziora-Chudzer L., Bailey J., Bott K., Wright D. -
arX iv:2 110. 0431 9v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wyat21.pdf12 Oct 2021: H. Chen, A. Morlok, D. M. Watson, P. Manoj, P. Sheehan, T. ... Page, P. Panuzzo, A. Papageorgiou, C. P. Pearson, I. Perez Fournon,M. -
ms_v2.dvi
https://people.ast.cam.ac.uk/~wyatt/rcmw12.pdf22 May 2012: H. Chen, T. P. Greene, P. M. Hinz, M. J.Kuchner, C. ... H., Sheehan, P., Watson, D. M., Manoj, P., & Najita, J. -
MNRAS 000, 1–12 (2018) Preprint 4 December 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/cmfk19.pdf11 Apr 2019: Cotton1,2?, Jonathan P. Marshall3,4, Priscilla C. Frisch5,Lucyna Kedziora-Chudzer1,2, Jeremy Bailey1,2, Kimberly Bott6,7,Duncan J. ... 2010;Cotton et al. 2016b,c; Frisch et al. 2016; Cotton et al. -
MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mybf19.pdf8 Jan 2019: Matrà7. and M. C. Wyatt11Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK2Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany3Astrophysikalisches Institut und Universitätssternwarte -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: Warm dusty discs: Exploring the A star 24µm debris populationR. Smith1,2 and M.C. ... Smith and M.C. Wyatt: Warm dusty discs: Exploring the A star 24µm debris population 3. -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/wbpc09.pdf25 Oct 2009: c 0000 RAS, MNRAS 000, 000–000. 4 M. C. Wyatt et al. ... c 0000 RAS, MNRAS 000, 000–000. 6 M. C. Wyatt et al. -
Observing Kepler stars with WISE
https://people.ast.cam.ac.uk/~wyatt/kw12.pdf7 Jul 2012: c 0000 RAS. 2 G. M. Kennedy, M. C. Wyatt. 1984; Kalas et al. ... 5 Retrieved fromhttp://skyview.gsfc.nasa.gov/. c 0000 RAS, MNRAS000, 000–000. -
arX iv:1 312. 4531 v2 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kmlm13.pdf21 Jan 2014: 4.8. Schneider et al. (2013)report a detection in the XMM-Newton Serendipitous Source Cat-alog (Watson et al. ... 100. 50. 0. 50Z. [p. c]. 200 150 100 50 0 50Y [pc]. -
MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/kw20.pdf18 Aug 2020: as. tro-. ph.E. P] 1. 7 A. ug 2. 020. 2 Krivov and Wyatt. ... star (1 <p<2), we mayexpect that larger discs tend to be more massive. -
Astronomy & Astrophysicsmanuscript no. 8719 c© ESO 2008April 28,…
https://people.ast.cam.ac.uk/~wyatt/swd08.pdf29 Apr 2008: as negative;b=Age taken from Geneva-Copenhagen Survey;c= Identified as having excess by Hines. ... 2. Dec. offs. et, a. rcse. c. Residuals. 2 1 0 -1 -2RA offset, arcsec. -
MNRAS 000, 1–27 (2020) Preprint 27October 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lwak20.pdf10 Feb 2021: 2020TheAuthors. arX. iv:2. 010. 1265. 7v1. [as. tro-. ph.E. P] 2. ... Significant emission is notedwith eitheran "A", "B" or "C", and numerically counted ifmore than one source type in a single image is detected. -
arX iv:1 310. 6936 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/gkte13.pdf28 Oct 2013: et al., 2013, A&A 555, A11Eiroa C. et al., 2010, A&A 518, L131Figueira P. ... von Braun K. et al., 2011, ApJ 729, L26. Watson C.A. -
arX iv:1 408. 4116 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kw14.pdf22 Aug 2014: C. WyattInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK. ... component. c 0000 RAS, MNRAS000, 000–000. Two Temperature Debris Disks: Multiple Belts? -
TLA_large
https://people.ast.cam.ac.uk/~wyatt/tgmk14.pdf4 Dec 2014: 3 P R O P E R T I E S O F A - S TA R D E B R I S D I S C S. ... 0P. 160. R16. 0χ. 160. nam. ety. pe(p. arse. c)(M. yr). -
arX iv:1 604. 0828 6v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/mcbe16.pdf29 Apr 2016: Filter HD T/C λeff q u p d p/d θ[nm] [ppm] [ppm] [ppm] [pc] [ppm/pc] []. g′ 2262 Target 464.2 4.7 5.7 37.4 ... Sub-micron (0.1µm) dust grains are predicted to have. 10 J. P. -
arX iv:1 311. 2977 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/mksb13.pdf14 Nov 2013: of Fomalhaut b, though itnow appears to apply to a hypothetical Fomalhaut c(Chiang et al. ... 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. -
Five steps in the evolution from protoplanetary to debrisdisk ...
https://people.ast.cam.ac.uk/~wyatt/wpkm15.pdf17 Dec 2014: Five steps in the evolution from protoplanetary to debrisdisk. M. C. ... M. C. Wyatt. O. Panić. G. M. Kennedy. L. Matrà. Institute of Astronomy, University of Cambridge, MadingleyRoad, Cambridge CB3 0HA, UK. -
Analysis of the Herschel DEBRIS Sun-like star sample
https://people.ast.cam.ac.uk/~wyatt/skwl18.pdf19 Feb 2018: 3 D I S C I N C I D E N C E A R O U N D F, G , A N D KT Y P E S TA ... 4(c), is 28 per cent,the same as that given in Table 2. -
MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mcwb18.pdf31 Jul 2018: S. Marino,1?, J. Carpenter,2 M. C. Wyatt1, M. Booth3, S. Casassus4,5, V. ... P] 3. Jul. 201. 8. 2 S. Marino et al. than 10 au it has only been possible to detect a few gas gi-ants, mainly through direct imaging 1 (Marois -
arX iv:1 511. 0591 9v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf25 Nov 2015: Z. H. Draper1,2, B. C. Matthews2,1, G. M. Kennedy3, M. C. ... Continued. c 2002 RAS, MNRAS000, 1–18. 6 Z. H. Draper et al. -
arX iv:1 403. 6186 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/mmek14.pdf2 Jul 2014: Jonathan P. Marshall1,2,, A. Moro-Martı́n3,4, C. Eiroa1, G. Kennedy5, A. Mora6, B. ... J.P. Marshall, A. Moro-Martı́n, et al.: Herschel observations of exoplanet host stars. -
arX iv:1 610. 0071 4v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wbjm16.pdf7 Oct 2016: arX. iv:1. 610. 0071. 4v1. [as. tro-. ph.E. P] 3. Oct. ... scattered disks. M. C. Wyatt1, A. Bonsor1, A. P. Jackson2, S.
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