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1 - 10 of 13 search results for katalk:za33 24 |u:people.ast.cam.ac.uk where 0 match all words and 13 match some words.

  1. Results that match 1 of 2 words

  2. CASU WFCAM/VISTA Diary Page

    https://people.ast.cam.ac.uk/~wfcam/diary.html
    24 Mar 2010: 24/25th October - UK VDFS Review at Cambridge. The documents are available here.

  3. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt
    2 Jul 2010: It's hot (JCR) pleasant (MJI) down here - upper windows can be kept open 24/7 to keep the punters happier.

  4. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100922.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100922.txt
    26 Oct 2010: In the K-band, for example, the surface brightness of these stripes is between 23.5 and 24 mag/sq arcsec.

  5. arX iv:1 007. 4517 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/bw10.pdf
    27 Jul 2010: Su et al.(2006) search a sample of 160 stars for excess at both 24 and70µm. ... 2006) at 24 (upper) and 70µm (middle), comparable toFig.2 of Wyatt et al.

  6. arX iv:1 008. 0865 v2 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/cws10.pdf
    22 Aug 2010: Forexam-ple a disc with an inner radius of 24 AU, surface density profileΣ r7/3 between 24 and 34 AU, andΣ r1.5 from 34 to 90AU can fit the

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

    https://people.ast.cam.ac.uk/~wyatt/gw10.pdf
    29 Jan 2010: Averag-ing the measured E70 for these 24 stars we find 0.03 0.02. ... in prep.) will present the final model parame-ters fitting both 70 and 24 µm debris statistics among theSpitzer-surveyed FGK stars.

  8. Are Debris Disks Self-Stirred?

    https://people.ast.cam.ac.uk/~wyatt/kw10.pdf
    19 Feb 2010: We therefore arrive at Equation(9) by focusing on the 24 µm peak excesses. ... inferred from the 24 70 µm colour assuming blackbodygrains at a single temperature, Eq.

  9. Collisional Evolution of Irregular Satellite Swarms: Detectable Dust…

    https://people.ast.cam.ac.uk/~wyatt/kw11.pdf
    25 Nov 2010: The total flux in this 24 µm image is 320 Jy,which yields a peak surface brightness of around 1.25MJy/sr. ... Simple model of Saturn’s irregular satellite dustcloud at 24 µm. Grains follow parent body orbits.

  10. arX iv:1 011. 1437 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/mctw10.pdf
    10 Nov 2010: at 18.1µm and 0.3 mJy/pixeland 9.8 mJy/pixel at 24.5µm. ... in the 18.1-µmimage and 29.9 in the 24.5-µm image.

  11. 14667ms.dvi

    https://people.ast.cam.ac.uk/~wyatt/mskp10.pdf
    27 May 2010: Type A3 Va A1 V F2 VPACS OM scan point-source scanD [pc] 11.0 24.3 18.2rms100 [mJy/beam] 1.4 3.1 1.2rms160 [mJy/beam] 3.9 ... Stars mark the 100and 160µm flux densities fromHerschel. Optical data were obtainedfrom Simbad and Vizier.Spitzer 24 and 70µm

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