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  2. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_140122.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_140122.txt
    5 Mar 2014: One of these (apm48) will be used for update tests prior to killing off the entire lot. ... The list comes from VISTA, WFCAM, or VST. JRL will test these out shortly.
  3. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_140226.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_140226.txt
    5 Mar 2014: still playing catchup due to the upgraded security EGS - took pity and sent a text file of the latest VST and VISTA grades SC - system update tests on hold but in ... Slightly hidden from view WFCAM processing continues apace with a mix of normal astro
  4. MATHEMATICAL TRIPOS Part III Thursday, 3 June, 2010 9:00 ...

    https://people.ast.cam.ac.uk/~wyatt/psd_exam2010.pdf
    23 Jan 2014: 2. 1. Consider a test particle orbiting a binary comprised of a star and planet of massesM and Mpl. ... ẋ′ = ẋ µα0.5(1 e2)0.5A sin nplt ,. ẏ′ = ẏ µα0.5(1 e2)0.5A cos nplt ,where µ =. MplM Mpl. and α =apla. Even though the test
  5. arX iv:1 309. 1466 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwbw13.pdf
    23 Jul 2014: Curiously however, all three systemswith directly imaged planets (around A-stars) allow this test.Despite uncertainties about the orbit and nature of the planetaround Fomalhaut (Kalas et al. ... test binary orbital plane - disk alignment ifthe binary
  6. MATHEMATICAL TRIPOS Part III Friday, 30 May, 2014 9:00 ...

    https://people.ast.cam.ac.uk/~wyatt/psd_exam2014.pdf
    17 Jul 2014: Part III, Paper 59 [TURN OVER. 4. 3. A test particle orbits a star of mass M with a semimajor axis a, eccentricity e andlongitude of pericentre ̟.
  7. MATHEMATICAL TRIPOS Part III Monday, 11 June, 2012 1:30 ...

    https://people.ast.cam.ac.uk/~wyatt/psd_exam2012.pdf
    23 Jan 2014: Part III, Paper 64 [TURN OVER. 4. 3. Consider a test particle in a binary system comprised of two masses M1 and M2.The massive bodies orbit the centre of mass
  8. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/sjvw14.pdf
    4 Dec 2014: Simulations are run for 4.5 Gyrs, oruntil all test particles have been removed. ... 4 DETECTABILITY WITH LSST. To test this prediction, we want to find some asteroids in-bound from the Oort cloud.
  9. Mon. Not. R. Astron. Soc. 000, ??–?? (2014) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/scw14.pdf
    2 Jul 2014: To investigate this, we perform a smaller sample of 50 simula-tions in which we place a circular4 disk of 100 test particles aroundFomalhaut A, with semimajor axis distributed randomly in ... Toevaluate the plausibility of this suggestion, we also
  10. vpfit9.5.dvi

    https://people.ast.cam.ac.uk/~rfc/vpfit9.5.pdf
    14 Apr 2014: Runs test K-S test Chi-squared Chans ndf APr Xp(.68) Xp(.95) Xp(.99). ... and KS test respectively [0.01,1E-8]. OR, threshold normalized CHI2 (if >1).
  11. Mon. Not. R. Astron. Soc. 000, 1–22 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pw14.pdf
    2 Jul 2014: Our systems consisted ofa massive particle representing the planet and 103 to104 massive test particles to model the disc.

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