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1 - 10 of 21 search results for katalk:za33 24 |u:people.ast.cam.ac.uk where 0 match all words and 21 match some words.

  1. Results that match 1 of 2 words

  2. /astro/data/upsand1/mpayne/PLANETESIMAL_DRIVEN_MIGRATION/plots/plot_31…

    https://people.ast.cam.ac.uk/~wyatt/pwt09.pdf
    3 Sep 2009: 0.24), while its mass has further doubled to 0.4M.Only a very small amount of additional migration is observed. ... 0.24. Similarly, the mass of theouter-most body also increases significantly as the surfacedensityand the surface density ratio are

  3. 11626.dvi

    https://people.ast.cam.ac.uk/~wyatt/swh09.pdf
    23 Jun 2009: June 23, 2009. Resolving the hot dust around HD69830 and η Corvi with MIDI andVISIR. R. Smith1, M.C. Wyatt1, and C.A. Haniff2. 1 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0AHe-mail:rsed@ast.cam.ac.uk. 2

  4. arX iv:0 911. 3426 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/pgdm09.pdf
    19 Nov 2009: The majority of SUNS and DEBRIS tar-gets also have photometry at 24 and 70 µm from the MIPS(Multiband Imaging Photometer and Spectrometer) instru-ment on the Spitzer space telescope, ... 90. -60. -30. 0. 30. 60. 90. 0 3 6 9 12 15 18 21 24.

  5. CASU WFCAM/VISTA Documentation (Sorted)

    https://people.ast.cam.ac.uk/~wfcam/documentation_sorted.html
    13 May 2009: Pipeline science requirements. 23-10-2002. 24-01-2003 [ps]. ... Pipeline document (old version submitted to CDR). 23-10-2002. 24-01-2003 [ps].

  6. Craig  Mackay

    https://people.ast.cam.ac.uk/~cdm/cdm_pub_list_130509.htm
    14 May 2009: ApJ, 270, 342 (1983). 24. Mackay, C.D. and Astill, D.M., CCD Development at Cambridge, England'. ... 31. Mackay, C.D., CCDs in Astronomy'. Ann. Rev. Ast. And Astrophys., 24, 255, 1986.

  7. Debris discs around nearby solar analogues

    https://people.ast.cam.ac.uk/~wyatt/gwb09.pdf
    8 Jul 2009: All of our target stars have now been searched with Spitzer for de-bris discs, using Multiband Imaging Photometer for Spitzer (MIPS)at 24 and 70 μm wavelengths.

  8. Debris disk dynamical theory Mark Wyatt Institute of Astronomy, ...

    https://people.ast.cam.ac.uk/~wyatt/MarkWyatt_Spitzer2008Conference.pdf
    12 Jan 2009: Spitzer imaging of Vega disk. 850µm (Holland et al.). 24 and 70µm (Su et al. ... Diameter, D. σ(D), AU2. Dmin. Dmax. Evolution of size distribution. Steady-state evolution explains 24 and 70µm stats.

  9. https://people.ast.cam.ac.uk/~vasily/sdss/orphan/orphan_south_fields.t…

    https://people.ast.cam.ac.uk/~vasily/sdss/orphan/orphan_south_fields.txt
    29 Jan 2009: 19 167.94027 -11.87500 20 166.64250 -11.87500 21 165.34473 -11.87500 22 168.65123 -13.42500 23 167.34556 -13.42500 24 166.03988 -13.42500 25 ... 21.17500 38 171.17104 -21.17500 39 169.80908 -21.17500 40 173.37749 -22.72500 41 172.00060 -22.72500 42

  10. https://people.ast.cam.ac.uk/~vasily/sdss/sgr/bellazzini_clusters.txt

    https://people.ast.cam.ac.uk/~vasily/sdss/sgr/bellazzini_clusters.txt
    29 Jan 2009: 5.3 -55.7 Terzan 3 6.18 -24.8 NGC 5466 8.55 21.9 NGC 288 9.88 17.2 NGC 7089 10.14 -18.9 NGC 6426

  11. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090518.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090518.txt
    7 Jun 2009: takes 24 hours from observing finishing for the data to be transferred, verified and ingested here).

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