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  2. The Triple Alpha Process for Helium Fusion Mathematics at ...

    https://people.ast.cam.ac.uk/~cat/maths/maths.html
    21 Nov 2016: Tests. Applicants will be required to sit a one-hour non-calculator pre-interview test in mathematical skills during their interview visit. ... The tests will not be based on any particular syllabus and no past papers are available.
  3. MATHEMATICAL TRIPOS Part III Friday, 27 May, 2016 1:30 ...

    https://people.ast.cam.ac.uk/~wyatt/psd_exam2016.pdf
    16 Sep 2016: 3. 2. Consider the motion of a test particle in the gravitational potential of a binarycomprised of two bodies of mass M1 and M2 M1. ... Part III, Paper 316 [TURN OVER. 4. 3. Consider the evolution of a test particle due to the secular perturbations of
  4. vpfit10.4.dvi

    https://people.ast.cam.ac.uk/~rfc/vpfit10.4.pdf
    5 Oct 2016: 3. statistics for whole fit:. Runs test K-S test Chi-squared Chans ndf APr Xp(.68) Xp(.95) Xp(.99). ... Runs test K-S test Chi-squared Chans ndf APr Xp(.68) Xp(.95) Xp(.99).
  5. Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf
    21 Jul 2016: 3.2 CO spectroscopy. Figure 3 shows the CO spectrum towards HD 32297, reduced bytwo different methods to test for robustness. ... 10 100. 1.0. 8. 6. 4. 2. 0. KS–Test Comparison Cumulative Fraction Plot.
  6. arX iv:1 601. 0686 6v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dhmh16.pdf
    27 Jan 2016: the phase fluctuations but on-sky verification tests haveshown that large phase jumps can occasionally occur andcause fringe jumps (even with the phase loop running at1 kHz).
  7. arX iv:1 604. 0828 6v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/mcbe16.pdf
    29 Apr 2016: 2014). To test this hypothesis we have mea-sured the degree of polarization of six hot dust stars with-out any notable excess at mid- or far-infrared wavelengthsusing the HIgh
  8. arX iv:1 610. 0071 4v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/wbjm16.pdf
    7 Oct 2016: 1987), showedhow the ultimate fate of any test particles encounteringand subsequently being scattered by a planet depends onthe planet’s mass and semimajor axis. ... 2.5 Applicability to scattered planets. The division of parameter space described in
  9. Mon. Not. R. Astron. Soc. 000, 1–16 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/kwcp16.pdf
    7 Jun 2016: To test thedependence on the IRF, we fix Ṁ/Ṁ0 = 1 and we createa second χ2 map, shown in Fig.
  10. MNRAS 000, 1–12 (2015) Preprint 12 May 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mmsw16.pdf
    17 May 2016: To test the significance of this detec-tion and whether this could be a product of our image synthesismethod, we produce Clean images obtaining roughly the same re-sults.
  11. MNRAS 000, 1–21 (2016) Preprint 23 September 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mdwk16.pdf
    23 Sep 2016: MNRAS 000, 1–21 (2016) Preprint 23 September 2016 Compiled using MNRAS LATEX style file v3.0. Exocometary gas structure, origin and physical propertiesaround β Pictoris through ALMA CO multi-transitionobservations. L. Matrà1,2?, W. R. F. Dent3,

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