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  2. MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/kw20.pdf
    18 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.
  3. 29 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.
  4. MNRAS 000, 1–27 (2020) Preprint 27October 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/lwak20.pdf
    10 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.
  5. arX iv:1 310. 6936 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/gkte13.pdf
    28 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.
  6. arX iv:1 408. 4116 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kw14.pdf
    22 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?
  7. TLA_large

    https://people.ast.cam.ac.uk/~wyatt/tgmk14.pdf
    4 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).
  8. arX iv:1 604. 0828 6v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/mcbe16.pdf
    29 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.
  9. arX iv:1 311. 2977 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/mksb13.pdf
    14 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.
  10. Five steps in the evolution from protoplanetary to debrisdisk ...

    https://people.ast.cam.ac.uk/~wyatt/wpkm15.pdf
    17 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.
  11. Analysis of the Herschel DEBRIS Sun-like star sample

    https://people.ast.cam.ac.uk/~wyatt/skwl18.pdf
    19 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.

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