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1 - 10 of 26 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 26 match some words.

  1. Results that match 1 of 2 words

  2. Domain walls, cosmic strings and monopoles, dark matter   ...

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_11.pdf
    27 Feb 2012:  Many such phase transitions possible as Universe evolves. 2/20/12! Astroparticle! ... 2φx2. = dVdφ. 2/20/12 Astroparticle 7. From eq. of motion we get!

  3. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120327.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120327.txt
    27 Apr 2012: SC - encouraged the LTO4 suppliers by pointing out that 1723 single LTO4 tapes were divisible into boxes of 20 aka mod(1723,20)=3 MJI - attended and duly reported back on ... Measuring this effect is also compounded by 10-20% of the frames having rather

  4. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120926.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120926.txt
    5 Dec 2012: The normal variation is /-5% so being conservative in searching yields only 3 suspicious examples: -0.05 in g #10 for feb2012 0.06 in r #20 for dec2011 0.19 ... in NB #10 for dec2011 The one puzzling thing found was no offset for u_SDSS_flat_20120414.fit

  5. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_121128.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_121128.txt
    5 Dec 2012: JPE forwarded a warning about VIRCAM warming up at around 20:51 UT on the night of 1st November and was probably in this state for much of the night. ... the scaling of the pickup pattern varies from detector to detector by about 20-30% but other than

  6. Astroparticle_16

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_16.pdf
    13 Mar 2012: unphysical decays, or jump to final stage of decay! 3/12/12 Astroparticle 20. ... Assume 20% error on cross-section! 3/12/12 Astroparticle 22. •Number of dimensions and Planck mass can be obtained in a correlated way!

  7. The Astrophysical Journal, 701:2019–2032, 2009 August 20…

    https://people.ast.cam.ac.uk/~wyatt/lcwm09.pdf
    1 Aug 2012: The Astrophysical Journal, 701:2019–2032, 2009 August 20 doi:10.1088/0004-637X/701/2/2019C 2009. The American Astronomical Society. ... the strongest IRS spectralsensitivity to the 0.1–20 μm particle size range), with particlesize effects on the

  8. Question_solutions

    https://people.ast.cam.ac.uk/~gpe/Question_solutions.pdf
    16 Mar 2012: ˜ χ 20 ˜ l l 2 and work in slepton rest frame. ... The four vectors are:. ˜ χ 20 (E 2, p2 )˜ l (m ˜ l ,0).

  9. Astroparticle_14

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_14.pdf
    12 Mar 2012: ˜ χ 20 ˜   ˜ χ 1. 0 ˜ G γUse decay chains to get more information:! ... Mass lepton pair γ. Mllγmax = M. ˜ χ 20. 2 M˜ χ 1.

  10. arX iv:1 208. 1759 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwsp12.pdf
    9 Oct 2012: The images showsignificant residuals for changes of 10-20 in both inclinationand PA, giving an indication of their uncertainties. ... 10. 0. 10. 20. δ of. fset. ("). -4.00. -2.67. -1.33.

  11. ms_v2.dvi

    https://people.ast.cam.ac.uk/~wyatt/rcmw12.pdf
    22 May 2012: ime. 4m. 8m. Counts Time. 0 10 20 30 40 50Exozodi Brightness / Solar System Brightness. ... 20 –. Fig. 4.— Simulated high-contrast imaging of exozodi thermal emission with a ground-based ELT.Left: Amodel for a face-on debris disk aroundτ Ceti, a

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