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1 - 10 of 14 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 14 match some words.

  1. Results that match 1 of 2 words

  2. MATHEMATICAL TRIPOS Part III Friday, 27 May, 2016 1:30 ...

    https://people.ast.cam.ac.uk/~wyatt/psd_exam2016.pdf
    16 Sep 2016: 1 2B 0 0 20 1 B 2 0. . .

  3. MNRAS 000, 1–6 (2016) Preprint 13 July 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/agwk16.pdf
    13 Jul 2016: The occurrence rate of dippers in co-eval clusters (e.g.,20–30% of classical T Tauri stars in NGC 2264; Alencaret al. ... However, giant planets alone likely cannot account forall the dippers, as dipper occurrence rates (e.g., 20–30% inNGC 2264;

  4. Draft version December 23, 2016Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/cmws17.pdf
    23 Dec 2016: 0.00005. 0.0005. 20 40 60 80 100. 17. 16. 15. 14. ... star with luminosity 20.97 L, and the 8 µm blowoutsize of the silicate-carbon mixture.

  5. Astronomy & Astrophysics manuscript no. letter_HD206893 c©ESO…

    https://people.ast.cam.ac.uk/~wyatt/mhcc16.pdf
    2 Dec 2016: 2016), where a 3015 MJup brown dward wasdetected at 20 au of its host star, within a debris disc of innerradius 75 au. ... 40. 20. 0. 20. 40. 60. 80. 100. Surface. Brigh. tnessin.

  6. ms.dvi

    https://people.ast.cam.ac.uk/~wyatt/wmke16.pdf
    10 Nov 2016: For star subtraction, we usedthe LOCI algorithm (Lafreniere et al. 2006) to subtract the best linear combination of library (not science) images fromeach science image, in annular rings of 20 pixels, ... Appendix D: Detection limits on planetary

  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: Instead we calculated an expectation valueof 1.20 for thepgreen:pPlanetPolratio based on normalised prob-. ... 4 20.1 17.6 22.6 17.5 19.2 1.18 58.7 27.0.

  8. Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf
    21 Jul 2016: The entire passbandwas first fitted with a high-order polynomial, in order to fully usethe information present, and excluding only a region of 20 chan-nels of 1.27 km/s

  9. arX iv:1 601. 0686 6v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dhmh16.pdf
    27 Jan 2016: 0 10 20 30 40 50 60Elapsed time [s]. 0.1. 1.0. ... 10.0. 100.0. Inst. anta. neou. s nu. ll de. pth. [%]. -2 0 2 4 6Instantaneous null depth [%]. 0. 20. 40.

  10. MNRAS 000, 1–21 (2016) Preprint 23 September 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mdwk16.pdf
    23 Sep 2016: 4 L. Matrà et al. -200 -100 0 100 200. -60-40-20. ... 60-40-20. 0204060. Ste. lloce. ntr. ic d. ista. nce. (A. U).

  11. MNRAS 000, 1–12 (2015) Preprint 12 May 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mmsw16.pdf
    17 May 2016: 1 INTRODUCTION. Recent surveys have shown that at least 20% of nearby solar-typestars (FGK) host Kuiper belt analogue debris discs (Hillenbrandet al. ... 20406080. r. [AU. ]. 40 80 120. 160. r0 [AU]20 40 60 80.

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