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https://people.ast.cam.ac.uk/~vasily/oxford_homepage/abstract
https://people.ast.cam.ac.uk/~vasily/oxford_homepage/abstract13 Jul 2010: In the first two chapters of the thesis, I present a new method for lightcurve classification based on neural networks. -
Iceland - Photo by Ralf Donner
https://people.ast.cam.ac.uk/~vasily/oxford_homepage/iceland.html13 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. -
https://people.ast.cam.ac.uk/~pettini/canaries13/cupconf.sty
https://people.ast.cam.ac.uk/~pettini/canaries13/cupconf.sty5 Oct 2010: def@subeqnnum{{reset@fontrm (thesubequation)}} % % A new label command to refer to subequations. -
14667ms.dvi
https://people.ast.cam.ac.uk/~wyatt/mskp10.pdf27 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 -
arX iv:1 009. 0248 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf2 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 -
arX iv:1 011. 1437 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/mctw10.pdf10 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. -
arX iv:1 008. 0865 v2 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/cws10.pdf22 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 -
arX iv:1 007. 4517 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/bw10.pdf27 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. -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: Su et al. (2006) presented new 24 and 70µmphotometry which also confirms the excess. -
arX iv:1 012. 3079 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/mw11.pdf15 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 -
Collisional Evolution of Irregular Satellite Swarms: Detectable Dust…
https://people.ast.cam.ac.uk/~wyatt/kw11.pdf25 Nov 2010: arX. iv:1. 011. 4858. v1 [. astr. o-ph. EP]. 22. Nov. 201. 0Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 23 November 2010 (MN LATEX style file v2.2). Collisional Evolution of Irregular Satellite Swarms:. Detectable Dust around Solar -
Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 Feb 2010: When stirring reachesthe outer edge, all disks break to a faster decline in fbecause no new regions can be stirred.
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