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1 - 10 of 23 search results for KaKaoTalk:PC53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 23 match some words.
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  2. Astroparticle_16

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_16.pdf
    13 Mar 2012: 3/12/12 Astroparticle 24. Exploit fact that gravity couples to all particle types! ... Assume system created in disk - get minimum lifetime for black hole, 24 Myr, and hence max curvature of ADS bulk - 80 microns!
  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: 8. VST update -------------- As noted earlier, since February 29th Internet transfers of VST data from Paranal - Garching have been using the EVALSO link and VST data is now available 24 hours
  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 one in question is at http://www.eso.org/sci/facilities/paranal/instruments/vircam/news.html and shows it was 2010-04-24/2010-05-06.
  5. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120430.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120430.txt
    24 Aug 2012: transfer over the Internet some 24 hours later.
  6. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_121031.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_121031.txt
    5 Dec 2012: wrong end time and date for an OB. An example of the latter is below 2012-08-24 VIS 179.A-2010(F) 812323 0.00 A
  7. Domain walls, cosmic strings and monopoles, dark matter   ...

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_11.pdf
    27 Feb 2012: 2/20/12 Astroparticle 24.  Bulk region.  Co-annihilation region.  Focus point region.
  8. Astroparticle_14

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_14.pdf
    12 Mar 2012: Apply local SU(5) gauge symmetry - get 24 gauge bosons: γ, W+, W-, Z, 8 gluons and 12 X,Y bosons mediating quark-lepton transitions!These violate baryon and lepton number! ... and sgn(µ) as in SUGRA!Cgrav! Coupling for decays into gravitinos! 3/2/12
  9. 10 Dec 2012: There isboth cool dust (observable to Herschel) and warm dust(evident from IRS and MIPS 24 excesses). ... In the context of the wide belt imaging model, the IRSand MIPS 24 excesses are attributed to a warm innerring.
  10. Searching for Saturn's Irregular Satellite Swarm with Spitzer

    https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf
    29 Jun 2012: However, progress will be difficult.Table 3 inJewitt & Haghighipour(2007) shows that the faintestknown irregulars at Saturn have R magnitudes of 24.5,3 and thedeepest survey for Uranian irregulars had ... 3 The faintest published survey hasR = 24.5
  11. Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/jw12.pdf
    19 Jun 2012: Byconsidering the luminosity of dust produced in collisions within the boulder-debris distributionwe find that the Moon-forming impact would have been readily detectable around other stars inSpitzer 24 µm surveys

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