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Did you mean economiespast |u:people.ast.cam.ac.uk?
11 - 20 of 21 search results for Economics test |u:people.ast.cam.ac.uk where 2 match all words and 19 match some words.

  1. Results that match 1 of 2 words

  2. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090416.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090416.txt
    21 Apr 2009: STH will inquire about possibility/status of new WFCAM linearity measures when he goes out observing next week or so MJI forwarded UDS test results to JRL STH figured out the ... He has also being doing some extended mosaicing tests with MONTAGE which

  3. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090715.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090715.txt
    20 Jul 2009: Feeling upbeat he then tried to repeat the trick on test tile OB J,Ks data taken of the Sculptor dwarf (to compare with CIRSI observations) at airmass of 1.5

  4. New Page 1

    https://people.ast.cam.ac.uk/~cdm/cdm_CV_130509.htm
    14 May 2009: The tests carried out produced images with better resolution from the ground than have been obtained in space with the Hubble Space Telescope, and reached nearly 1000 times fainter than was

  5. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_091021.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_091021.txt
    26 Oct 2009: It turns out that the linearity sequences taken in August that were not quite deep enough for purpose were also meant to be used as a test of the stability of

  6. /astro/data/upsand1/mpayne/PLANETESIMAL_DRIVEN_MIGRATION/plots/plot_31…

    https://people.ast.cam.ac.uk/~wyatt/pwt09.pdf
    3 Sep 2009: Set H Number of (massive test-particle)planetesimals in the outer zone,NP,T est,Outer. ... However, for thesake of computational efficiency and practicality we simulated onlythe planetary embryos as fully interacting particles, modelling theplanetesimals

  7. survey07_rev2.dvi

    https://people.ast.cam.ac.uk/~wyatt/lwbm09.pdf
    21 Jul 2009: We now test whether or not such a source cluster can arisefrom the distribution of background sources. ... The two tests carried out above provide indica-tions that this structure is statistically unconsistent with knownspatial distributions of

  8. Planets and Debris Disks: Results from a Spitzer/MIPS Search ...

    https://people.ast.cam.ac.uk/~wyatt/bbcr09.pdf
    15 Sep 2009: software (ASURV; Lavalley et al. 1992). Several tests are commonly used for determining. ... It is possible,. however, to improve upon these tests by developing a test that incorporates all relevant.

  9. 11626.dvi

    https://people.ast.cam.ac.uk/~wyatt/swh09.pdf
    23 Jun 2009: The residual image shows no evidencefor emission beyond the PSF. Further tests comparing the pro-files of the observations, Gaussian and Moffat profile fits to theimages and comparisons of FWHM measurements ... Different test regions (annuli of different

  10. lecture8_debrisdiskapp

    https://people.ast.cam.ac.uk/~wyatt/lecture8_debrisdiskapp.pdf
    17 Feb 2009: be used to test models. …

  11. lecture4_planetformation

    https://people.ast.cam.ac.uk/~wyatt/lecture4_planetformation.pdf
    3 Feb 2009: 2006). Dependence on stellar mass • Low mass stars are equally likely to form planets (assuming they have equally massive disks) offering observational test (Boss 2006).

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