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1 - 10 of 11 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 11 match some words.
  1. Results that match 1 of 2 words

  2. arX iv:0 812. 2475 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/pfwb08.pdf
    17 Dec 2008: 200. 8. Mon. Not. R. Astron. Soc.000, 000–000 (2008) Printed 12 December 2008 (MN LATEX style file v2.2).
  3. 15 December 2008 Science from UKIDSS II WFCAM Science ...

    https://people.ast.cam.ac.uk/~wfcam/talks/ukidss_dec2008_mji.ppt
    16 Dec 2008: 115 TB Raw Data (30 TB compressed). 200 TB processed Data (50 TB compressed).
  4. arX iv:0 810. 5087 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/scwm08.pdf
    3 Nov 2008: 200. 8Astronomy & Astrophysicsmanuscript no. 10706 c ESO 2008October 28, 2008.
  5. Cambridge XMM Survey Science Centre

    https://people.ast.cam.ac.uk/~xmmssc/
    10 Oct 2008: 2. s. -1. (0.1-10 keV) and contain 100-200 serendipitous" X-ray sources.
  6. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080806.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080806.txt
    19 Aug 2008: The GPS astrometry glitches affecting 200 files over the 05A-07B period noted in the previous minutes were fixed and have been re-transferred by WFAU.
  7. Dynamics of small bodies in planetary systems Mark C. ...

    https://people.ast.cam.ac.uk/~wyatt/wyat08.pdf
    8 Jul 2008: This emission comes from dust that is heatedby the star and which re-radiates that energy in the thermal infrared, attemperatures between 40-200 K, depending on the distance of the ... It is possible that the effect seen in Fig. 6 may be the explanation
  8. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080623.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080623.txt
    27 Jun 2008: The only reported UKIDSS problem turned out not to be new DR4 data but a previously missed astrometry problem affecting a small percentage of GPS data (affecting 200 files over a
  9. 29 Apr 2008: withS = 200 and 5000 whenr/θ is small. ... Error Background limit, mJyb. 10800 11.59 1800 TIMMI2 513 477 54 15 3918.72 3762 VISIR 200 186 29 6 14.
  10. Microsoft PowerPoint - wyatt

    https://people.ast.cam.ac.uk/~wyatt/wyatt_hst08.pdf
    7 Feb 2008: ACS image of 5Myr HD141569 shows dense rings at 200 and 325 AU with tightly wound spiral structure (Clampin et al.
  11. 7009.pmd

    https://people.ast.cam.ac.uk/~wyatt/mwmt08.pdf
    1 Feb 2008: fit to this data suggests a t0/t de-cline, with t0 = 100–200 m.y. ... Thepersistence of excesses beyond 200 m.y. rules out a fast 1/t2.

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