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  2. https://people.ast.cam.ac.uk/~vasily/oxford_homepage/abstract

    https://people.ast.cam.ac.uk/~vasily/oxford_homepage/abstract
    13 Jul 2010: In the first two chapters of the thesis, I present a new method for lightcurve classification based on neural networks.
  3. Iceland - Photo by Ralf Donner

    https://people.ast.cam.ac.uk/~vasily/oxford_homepage/iceland.html
    13 Jul 2010: The waste water is used to heat a swimming pool. For a while it was popular with jetsets on their way from New York to Europe.
  4. https://people.ast.cam.ac.uk/~pettini/canaries13/cupconf.sty

    https://people.ast.cam.ac.uk/~pettini/canaries13/cupconf.sty
    5 Oct 2010: def@subeqnnum{{reset@fontrm (thesubequation)}} % % A new label command to refer to subequations.
  5. 14667ms.dvi

    https://people.ast.cam.ac.uk/~wyatt/mskp10.pdf
    27 May 2010: All three stars are known disc hosts.Herschel spatially resolves the dust emissionaround all three stars (marginally, in the case ofβ UMa), providing new information about discs as close as 11
  6. arX iv:1 009. 0248 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf
    2 Sep 2010: The de-bris absorbs starlight and re-emits it at longer wavelengths,and observations since 2003 with the Spitzer space telescopehave yielded many new debris detections in the mid- to ... 3 OBSERVATIONS AND DATA REDUCTION. The eleven new stars were
  7. arX iv:1 011. 1437 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/mctw10.pdf
    10 Nov 2010: 5. Discussion and conclusions. Using new mid-IR images at 18 and 25µm, we have confirmedthe previously observed brightness asymmetry discovered byTelesco et al. ... 350,Hipparcos, the New Reduction of the Raw Data. Wahhaj, Z., Koerner, D.
  8. arX iv:1 008. 0865 v2 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/cws10.pdf
    22 Aug 2010: arX. iv:1. 008. 0865. v2 [. astr. o-ph. SR. ] 6. Aug. 201. 0. Mon. Not. R. Astron. Soc.000, 1–11 (2010) Printed August 9, 2010 (MN LATEX style file v2.2). Resolved Imaging of the HD191089 Debris Disc. Laura Churcher1, Mark Wyatt1, Rachel
  9. arX iv:1 007. 4517 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/bw10.pdf
    27 Jul 2010: Parameter Orginal value New value. Mmid 10.0 7.8 MDc 60.0 1.9kme 0.05 0.05. ... lation that incorporates the optical properties of realisticgrains, to find new values for this parameter set.
  10. arX iv:1 004. 0644 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/sw10.pdf
    6 Apr 2010: Su et al. (2006) presented new 24 and 70µmphotometry which also confirms the excess.
  11. arX iv:1 012. 3079 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/mw11.pdf
    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

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