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Astroparticle_14
https://people.ast.cam.ac.uk/~gpe/Astroparticle_14.pdf12 Mar 2012: GeV. ]1/. 2m. 200. 300. 400. 500. 600. (600)g. (800)g. (1000)g. -
Astroparticle_16
https://people.ast.cam.ac.uk/~gpe/Astroparticle_16.pdf13 Mar 2012: Photon easy to detect and measure! [GeV]Tγp. 200 300 400 500 600 700. ... n=4.0 0.6 - 1.0!•MPL = 1029 200 - 100 GeV! 3/12/12 Astroparticle 23. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120118.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120118.txt10 Feb 2012: He took with him an overview of what VST data for 200 band-merged ATLAS fields currently yields. -
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 -
1 A SELF-CONSISTENT MODEL OF THE CIRCUMSTELLAR DEBRIS CREATED ...
https://people.ast.cam.ac.uk/~wyatt/jlcm12.pdf23 Oct 2012: 2006) and the effective. temperature of the large rubble, 200 K, they placed the dust populations at 5.8 0.6 (1) AU. ... fine dust” are much better at radiating heat and needs only to reach a color temperature of 200. -
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, -
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. -
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 -
arX iv:1 208. 1759 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwsp12.pdf9 Oct 2012: Coplanar Circumbinary Debris Disks 11. 0 50 100 150 200 250 300Semi-major axis (AU). -
Searching for Saturn's Irregular Satellite Swarm with Spitzer
https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf29 Jun 2012: Stansberry. OFF ON IE IW. -600 -400 -200 0 200 400 600offset (Saturn radii). ... 400. -200. 0. 200. 400. offs. et (. Sat. urn. radi.
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