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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. 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.

  3. 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.

  4. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_071211.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_071211.txt
    3 Jan 2008: The release covers about 50% of the Northern Galactic Plane and contains r,i,Ha data for some 200 million stars.

  5. 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).

  6. 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

  7. 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.

  8. 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

  9. 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.

  10. 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.

  11. Astronomy & Astrophysicsmanuscript no. 8719 c© ESO 2008April 28,…

    https://people.ast.cam.ac.uk/~wyatt/swd08.pdf
    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.

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