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  2. DWE's Gallery

    https://people.ast.cam.ac.uk/~dwe/gallery/
    18 May 2018: To test out the design I made a scale model which could be used by my god-daughter's Barbie.
  3. MATHEMATICAL TRIPOS Part III Thursday, 31 May, 2018 9:00 ...

    https://people.ast.cam.ac.uk/~wyatt/psd_exam2018.pdf
    12 Jul 2018: Part III, Paper 316 [TURN OVER. 4. 3. (i) Consider a test particle orbiting a star in the same plane as a coplanar system ofN planets. ... Use this to describe, bothquantitatively and with a sketch, the physical space covered by test particles, all of
  4. M. Pettini: Introduction to Cosmology — Lecture 6 THE ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture06.pdf
    23 Oct 2018: sufficiently high that it can be detected overcosmological distances, then we could test for the cosmological parametersm,0, Λ,0, and k,0 that determine the form of dL = f(z) ... region. The angular diameter distance test onthe temperature fluctuations
  5. Gaia DFS PLS prop

    https://people.ast.cam.ac.uk/~gil/Gaia-RAeS-Leslie-Bedford-April2017.pdf
    29 Mar 2018: Gaia sees that in every measurement it makes so we can test Relativity to much improved accuracy.
  6. M. Pettini: Introduction to Cosmology — Lecture 5 REDSHIFTS ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture05.pdf
    18 Oct 2018: The measurementson which these tests are based generally involve the redshifts and radiantfluxes of distant objects—modern telescopes now have the capability ofreaching to early epochs in the history of the ... However any conclusions from such tests
  7. MNRAS 000, 1–11 (2015) Preprint 9 November 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/khhw18.pdf
    9 Nov 2018: In the case of Gaussian noise, the test would use a nullhypothesis of white noise with. ... The likelihood ratio test gives a test statistic of. Tn,w =(x̄n,w 1).
  8. Astronomy and Astrophysics in the Gaia skyProceedings IAU Symposium…

    https://people.ast.cam.ac.uk/~gil/gaia_from_proposal_to_gdr1.pdf
    26 Mar 2018: Tests of Galaxy Formation dynamical determination of dark matter distribution reconstruction of merger and accretion history.
  9. M. Pettini: Introduction to Cosmology — Lecture 1 BASIC ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture01.pdf
    8 Oct 2018: The power of the hypothesis of homogeneity is that our own observationsfrom Earth are then all we need to test a cosmological model. ... On galactic scales, consider Figure 1.8. With gravity supplying the cen-tripetal force required to keep a test
  10. arX iv:1 801. 0542 9v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kmmp18.pdf
    18 Jan 2018: These tests were however not exhaustive. Formally, we can use the Schwarz criterion (Bayesian In-. ... formation Criterion, or BIC) to test which among our models. should be preferred (Schwarz 1978).
  11. M. Pettini: Introduction to Cosmology — Lecture 17 THE ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture17.pdf
    28 Nov 2018: Ideally the method should have a solid physical underpinning andhigh internal accuracy, amenable to empirical tests for systematic errors. ... The masing clumps act as dynamical test particles. A rotation curve ismeasured along the major axis of the

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