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1 - 10 of 17 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 17 match some words.

  1. Results that match 1 of 2 words

  2. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_101027.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_101027.txt
    3 Dec 2010: The faulty CCD has been replaced and the whole array is co-planar to /- 20 microns. ... Approximately 20% of the band-merged VHS tile products investigated had a serious problem with the photometry due to this effect (though it is a moot point if most of

  3. Question_sheet

    https://people.ast.cam.ac.uk/~gpe/Question_sheet_1.pdf
    1 Mar 2010: Consider the process. ˜ χ 20 ˜   ˜ χ 1.

  4. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100216.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100216.txt
    24 Mar 2010: 4. Data archives update AAT, ING, WFCAM, VISTA: all going smoothly UKIRT: JRL reported that he was still awaiting the last 20 or so nights of missing data.

  5. https://people.ast.cam.ac.uk/~pettini/canaries13/cupconf.sty

    https://people.ast.cam.ac.uk/~pettini/canaries13/cupconf.sty
    5 Oct 2010: start of cupconf.sty %%%%%%%%%%%%%%%%%%%%%% % CUPconf.sty -- CUP conference proceedings style file % V0.1 released 20 September 1993, by Alison Woollatt % Copyright (1993) Cambridge University Press % This software may only be used ... 2,space}}% %

  6. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100826.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100826.txt
    30 Aug 2010: Although only a few % in the Ks band the effect is approaching 15-20% in the Y and Z-bands.

  7. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100421.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100421.txt
    5 May 2010: 5 new BLADES (20 cores) have been acquired and added to the VISTA processing kit and SC is in the process of connecting them up and installing an operating system on

  8. 14667ms.dvi

    https://people.ast.cam.ac.uk/~wyatt/mskp10.pdf
    27 May 2010: For point-source mode ob-servations, seven contiguous repeat chop/nod observations wereperformed. Scan map observations had eight repeats in a singlescan direction at a rate of 20′′/s. ... 20 Dept. of Physics & Astronomy, University of California,

  9. CASU WFCAM/VISTA Diary Page

    https://people.ast.cam.ac.uk/~wfcam/diary.html
    24 Mar 2010: March 2008. 18-20 March - UltraVista meeting in Leiden, MJI and JRL part attended and gave talks.

  10. arX iv:1 009. 0248 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf
    2 Sep 2010: In the general stellar population, theextrapolated planet total is 17-20 % (Cumming et al. ... 2008; Greaves & Wyatt 2010), which agreewell with the predictions of 21 and 20 % respectively.

  11. arX iv:1 001. 5177 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/gw10.pdf
    29 Jan 2010: The high-est mass appears realistic, for example it is comparable tothe 20-30 M of colliders inferred around the A-star Fomal-haut (Wyatt & Dent 2002), which hosts a bright ... 2008) estimate that 18 % of Sun-likestars host giant planets, of above about

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