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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.
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  2. VHS nominal exposure time and flux limits Waveband Exposure ...

    https://people.ast.cam.ac.uk/~rgm/vhs/vhs-summary.html
    6 Mar 2009: Last modified: Fri Mar 6 09:52:24 GMT 2009.
  3. survey07_rev2.dvi

    https://people.ast.cam.ac.uk/~wyatt/lwbm09.pdf
    21 Jul 2009: 1.50 -0.37 < 1.6GJ9809 M0 24.0 03 0.5 2.20 0.36 2.20 0.16 < 2.4. ... 2006), and excluding GJ526 at thisstage) makes the detection fraction to amount to 24.51.5 % in oursample of 50 M-dwarfs.
  4. SOMs 4 OGLE

    https://people.ast.cam.ac.uk/~vasily/ogle_som/map.html
    29 Jan 2009: Cataclysmic/Eruptive/Microlensing. Node x=8, y=25. Node x=9, y=26. Node x=9, y=24. Node x=8, y=23.
  5. Planets and Debris Disks: Results from a Spitzer/MIPS Search ...

    https://people.ast.cam.ac.uk/~wyatt/bbcr09.pdf
    15 Sep 2009: 24 µm, indicative of warm dust in the inner system analogous to that produced. ... 16 –. wavelength (13 at 70 µm, plus HD 69830 at only 24 µm).
  6. New Page 1

    https://people.ast.cam.ac.uk/~cdm/cdm_CV_130509.htm
    14 May 2009: Taught the Introductory Astrophysics Lecture course, 24 lectures, 1998-2001 inclusive, and Topics in Contemporary Astrophysics, 2002-6 and 2008-present. ... Ph.D Awarded: 24.4.87. 8. Student: C A Haniff, Admission Date: 1.10.84, Title: High resolution
  7. Mon. Not. R. Astron. Soc. 000, 000–000 (2009) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/bwmm09.pdf
    19 Jun 2009: Recentsurveys have shown that 4% of stars exhibit 24 µm excess and 16% exhibit 70 µmexcess. ... Thisrun starts with an initial disc mass of 35 M and has 24 Mat the time of the LHB.
  8. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/wbpc09.pdf
    25 Oct 2009: Rewriting equation 23 gives. Mlate = [1.471011 Imax/K]M 4/3? q13/3t1[(1e)13/3S(e)]1, (24).
  9. lecture7_debrisdiskmod

    https://people.ast.cam.ac.uk/~wyatt/lecture7_debrisdiskmod.pdf
    12 Feb 2009: The largest fragment in a collision, flr = Mlr/M is given by Q < QD flr = 1 – 0.5 (Q/QD) Q > QD flr = 0.5(QD/Q)1.24.
  10. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_091119.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_091119.txt
    30 Nov 2009: within 24 hours of the final bit of data being taken.
  11. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090715.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090715.txt
    20 Jul 2009: 7. VISTA update Raw data has been received via Garching for up to and including June 24.

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