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1 - 10 of 12 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 12 match some words.

  1. Results that match 1 of 2 words

  2. Mon. Not. R. Astron. Soc. 000, 1–?? (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/mpwd15.pdf
    10 Dec 2014: We selected a 200-channels wide(85 km/s) spectral window around the CO line, expected at345.789 GHz (vhel=6.5 0.5 km/s, Gontcharov 2006).

  3. TLA_large

    https://people.ast.cam.ac.uk/~wyatt/tgmk14.pdf
    4 Dec 2014: MNRAS 445, 2558–2573 (2014) doi:10.1093/mnras/stu1864. An unbiased study of debris discs around A-type stars with Herschel. N. D. Thureau,1‹ J. S. Greaves,1 B. C. Matthews,2,3 G. Kennedy,4 N. Phillips,5. M. Booth,2,3,6 G. Duchêne,7,8 J.

  4. Constraining the Exozodiacal Luminosity Function of Main Sequence…

    https://people.ast.cam.ac.uk/~wyatt/mmsc14.pdf
    18 Oct 2014: a) inside of the 6 mas KIN inner working angle (IWA), defined as the half transmission point at 10 µm -,. or (b) outside of its ' 200 mas outer working angle (OWA), ... zodi levels, exhibiting significantly more stars in the 200 to 400 zodi level bin

  5. arX iv:1 408. 4116 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kw14.pdf
    22 Aug 2014: 2/2 as our like-lihood function. Chains with an ensemble of 200 “walkers” areinitialised with parameters that vary randomly1% from theχ2 fitting results, and then run for 50 steps as ... 6 shows that a typical warmcomponent would haveTwarm = 200

  6. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/fwgb14.pdf
    31 Jul 2014: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 31 July 2014 (MN LATEX style file v2.2). ALMA and Herschel Observations of the Prototype Dustyand Polluted White Dwarf G29-38. J. Farihi1,2?†, M. C. Wyatt2, J. S. Greaves3, A. Bonsor4,5, B.

  7. Mon. Not. R. Astron. Soc. 000, ??–?? (2014) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/scw14.pdf
    2 Jul 2014: The decrease in C’s eccentricity between 200 and350 Myrs is not caused by Galactic tides; rather it is caused by sec-ular interactions between B and C. ... 0. 50. 100. 150. 200. 250. 300. 350. 1e06 1e05 0.0001 0.001 0.01 0.1 1.

  8. Mon. Not. R. Astron. Soc. 000, 1–22 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pw14.pdf
    2 Jul 2014: 200. 20. y (a. u). 100. 50. 0. 50. 100. ... Normalised surface density0.0 0.5 1.0. z (au. ) 200. 20. y (a.

  9. vpfit9.5.dvi

    https://people.ast.cam.ac.uk/~rfc/vpfit9.5.pdf
    14 Apr 2014: J012417-374423 1 6288.800 6290.060 vsig=2.810. J012417-374423 1 5344.700 5346.300 vsig=2.810. J012417-374423 1 5326.200 5327.610 vsig=2.810.

  10. arX iv:1 402. 1184 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/dawk14.pdf
    10 Feb 2014: 2005). All three sources have SEDs. that peak at a wavelength of 200–300 µm, typical of high-redshift, dust-rich galaxies.

  11. mn.dvi

    https://people.ast.cam.ac.uk/~wyatt/wfpb14.pdf
    23 Jan 2014: velocitysurveys, as well a more distant 8 200 AU population of gi-ant planets found in imaging surveys (Udry & Santos 2007).Our understanding of the debris discs, i.e. ... Wethen set a total number of timesteps, Ntot (set to 200,000.

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