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1 A SELF-CONSISTENT MODEL OF THE CIRCUMSTELLAR DEBRIS CREATED ...
https://people.ast.cam.ac.uk/~wyatt/jlcm12.pdf23 Oct 2012: The non-unique nature of the spectral modeling allows us to test additional PSDs that can. ... Figure 6. middle shows a broken power law, with below 1 μm and. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120926.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120926.txt5 Dec 2012: These were characterized by incomplete tile coverage (i.e. not all 4 pawprint pointings were present) in the middle of sequences of otherwise normal tile observations. ... After a few manual tests and some surprisingly complex scripting, it turned out -
arX iv:1 211. 4898 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/lmsk12.pdf24 Nov 2012: Hence, we conclude that this test rejects the possibility thatthe superposition of two background point sources can be re-sponsible for the central emission. ... 2011) (see also Sibthorpe et al. (2012)). Second,the spectra of these test sources removed -
mnr_20522_LR
https://people.ast.cam.ac.uk/~wyatt/vw12.pdf30 Oct 2012: 5). In con-trast, the initial conditions which lead to instability for the η =0.5 simulations (middle panel of Fig. ... The middle and bottom panels of Fig. 10 indicate that the frac-tion of bodies which escape does not necessarily scale with a0;. -
arX iv:1 208. 1759 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwsp12.pdf9 Oct 2012: 33. 0.00. 1.33. 2.67. 4.00. Figure 6. Residuals after the resolved model ofα CrB is subtracted from the observations at 70µm (left) 100µm (middle) and 160µm (right). ... 1.33. 0.00. 1.33. 2.67. 4.00. Figure 8. Residuals after the resolved model ofβ -
Searching for Saturn's Irregular Satellite Swarm with Spitzer
https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf29 Jun 2012: Our aim here is to test this prediction for Saturn’s dustcloud using the 24µm Spitzer Space Telescope observationsused to discover the Phoebe ring. ... The ON scans are easily identifiable by thelarge bump in the middle due to the Phoebe ring. -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/bksm12.pdf5 Oct 2012: 70µm images on the left, 100µm images in the middle and 160µm onthe right. ... 70µm images are on the left,100µm images in the middle and 160µm on the right. -
mnr_21298_LR
https://people.ast.cam.ac.uk/~wyatt/wksm12.pdf7 Nov 2012: left – 70 µm; top middle – 100 µm; top right – 160 µm; bottom left – 250 µm; bottom middle – 350 µm and bottom right – 500 µm. ... 3 (middle) indicating a double-lobed structure. Fitting this as two Gaussians gives 8.0 mJy forthe -
arX iv:1 201. 3622 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/ramb12.pdf19 Jan 2012: We find that the gaps between these planets arenot only dynamically stable to test particles, but are frequently populated by planetesimals. ... The gas simulations test the effect of the presence of agas disk during and after the giant planet
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