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arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: 2008). To test the limits we can place on disc extension with un-resolved images, we performed the same PSF subtraction andresiduals testing on models of stars+ discs. ... temperature fit is 70K). Photometric confirmation of the excessis necessary to -
MNRAS 000, 1–23 (0000) Preprint 6 June 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mbwk18.pdf31 Jul 2018: the most optimum at producing exozodis anddelivering cometary material to inner planets, and we test. ... 1987). Below we present the mainanalytic considerations and predictions from previous worksthat we will test with our simulations. -
Mon. Not. R. Astron. Soc. 000, 1–22 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pw14.pdf2 Jul 2014: Our systems consisted ofa massive particle representing the planet and 103 to104 massive test particles to model the disc. ... outermost line) exterior resonances with the planet. Middle:. the line shows the path of the planet and the cross marks -
Astronomy & Astrophysics manuscript no. SHARDDS ©ESO 2022August…
https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf22 Mar 2024: The PSO framework was chosen as it showed, during tests,a higher convergence rate than Bayesian optimisation and al-lowed multi-core estimation7, reducing the computation time.More standard minimisation frameworks -
A planetesimal orbiting within the debris discaround a white ...
https://people.ast.cam.ac.uk/~wyatt/mgeh19.pdf25 Apr 2019: Manual, http://pencil-code.nordita.org/doc/manual.pdf. 96. C. P. McNally, W. Lyra, J.-C. Passy, A Well-posed Kelvin-Helmholtz Instability Test and. ... S6 &. S7 can be found in the directory pencil-code/samples/2d-tests/WhiteDwarfDisk, using version. -
MNRAS 000, 1–24 (2017) Preprint 30 March 2017 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/rwt17.pdf5 May 2017: 16) and eq. (17). For the top panels i = 10,for the middle panels m3 = 1MJ and for the bottom panels a3 = 2au. -
arX iv:1 503. 0207 3v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf10 Mar 2015: 4 (i.e. top right and middle right) that removing the stel-lar flux density does not account for all of the emission locatedat the stellar position. ... Thus, the limit on CO gas is not stringentenough to test different scenarios for the production of -
MNRAS 000, 1–19 (2019) Preprint 20 December 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/aght19.pdf17 Jan 2020: Dipper Disc Inclinations 5. Figure 1. ALMA images (left) and associated visibilities (middle) as well as K2/C2 light curves (right) for the sources in our sample. ... In order to more robustly test whether the inclina-tion distribution at id. -
MNRAS 000, 1–21 (2022) Preprint 28September 2022 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lwkk22.pdf29 Sep 2022: We will test this with simple modelsthat parameterise the surface density distribution of dust as a func-tion of the radial distance from the star. ... Albeitwith less significant fits in additional tests, i.e., poorer 𝜒2 andBICvalues, and visibly -
Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 Feb 2010: right panel) we estimate the significance of changes be-tween different age bins with the KS test. ... According tothis test, each pair of cumulative distributions for thethree youngest bins (three upper curves) could have allcome from the same
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