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1 - 10 of 13 search results for katalk:PC53 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. 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.

  3. 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.

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

    https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf
    2 Sep 2010: 0.088725 24.3 0.4 2.3 3.2 -0.03 0.9 -0.1. ... K-band magnitudes from2MASS were extrapolated to 24 µm based on a set of pho-.

  5. 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.

  6. 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

  7. 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.

  8. 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.

  9. 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.

  10. arX iv:1 004. 0644 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/sw10.pdf
    6 Apr 2010: Afit to the Q band excess emission and the 24 and 70µm excessreported in Su et al. ... Su et al. (2006) presented new 24 and 70µmphotometry which also confirms the excess.

  11. 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

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