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arX iv:1 201. 1911 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwsd12.pdf12 Jan 2012: 57,PA = 3171 , ρ = 1.200.014”). ... An object in such an orbit would havea period of at least 200 years, so could not have been detectednear the star in 2005 and be outside the NIRC2 field of -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/bksm12.pdf5 Oct 2012: γ Tri 70 777.638.8 21.200.40 756.438.8 40 10.240.04100 718.835.5 10.290.20 708.535.5 40 11.630.04160 -
midi_terr_sub3_nobold.dvi
https://people.ast.cam.ac.uk/~wyatt/swh12.pdf24 Feb 2012: Mon. Not. R. Astron. Soc. 000, 1–22 (2011) Printed 24 February 2012 (MN LATEX style file v2.2). Resolving the terrestrial planet forming regions of. HD113766 and HD172555 with MIDI. R. Smith1,2, M. C. Wyatt2 and C. A. Haniff31Astrophysics Group, -
Observing Kepler stars with WISE
https://people.ast.cam.ac.uk/~wyatt/kw12.pdf7 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. -
Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed ...
https://people.ast.cam.ac.uk/~wyatt/jw12.pdf19 Jun 2012: Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed 18 June 2012 (MN LATEX style file v2.2). Debris from terrestrial planet formation: the Moon-forming collision. Alan P. Jackson1? and Mark C. Wyatt1?1Institute of Astronomy, University of Cambridge,
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