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Astroparticle_16
https://people.ast.cam.ac.uk/~gpe/Astroparticle_16.pdf13 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! -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120327.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120327.txt27 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 -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120926.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120926.txt5 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. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120430.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120430.txt24 Aug 2012: transfer over the Internet some 24 hours later. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_121031.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_121031.txt5 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 -
Domain walls, cosmic strings and monopoles, dark matter ...
https://people.ast.cam.ac.uk/~gpe/Astroparticle_11.pdf27 Feb 2012: 2/20/12 Astroparticle 24. Bulk region. Co-annihilation region. Focus point region. -
Astroparticle_14
https://people.ast.cam.ac.uk/~gpe/Astroparticle_14.pdf12 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 -
Draft version December 10, 2012Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/bmkb12.pdf10 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. -
Searching for Saturn's Irregular Satellite Swarm with Spitzer
https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf29 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 -
Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed ...
https://people.ast.cam.ac.uk/~wyatt/jw12.pdf19 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 -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/bksm12.pdf5 Oct 2012: β Uma PACS 70/160 1342220802/3 2011-04-29. PACS 100/160 1342197015/6 2010-05-24. SPIRE 1342195687 2010-04-29. ... PSF fit500 4.24.9 0.420.01 3.84.9 PSF fit. -
mnr_21298_LR
https://people.ast.cam.ac.uk/~wyatt/wksm12.pdf7 Nov 2012: 24.8 2,14.8 1 arcsec, 75 4.5 at 160 μm. ... Photometry on the 24 μm image was used in the spectral energydistribution (SED) modelling. -
1 A SELF-CONSISTENT MODEL OF THE CIRCUMSTELLAR DEBRIS CREATED ...
https://people.ast.cam.ac.uk/~wyatt/jlcm12.pdf23 Oct 2012: which could be readily detectable around other stars by Spitzer 24 μm surveys for 25 Myr after. ... SiO h (24). which occurs with a rate coefficient m3 s-1 (Andreazza et al. -
arX iv:1 211. 4898 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/lmsk12.pdf24 Nov 2012: Finally, we used the SPIRE 3σ upper limits as a constraint toreject any model with a flux density of the dust emission largerthan 24 mJy at 250µm. ... The upper inset zooms on the IRS wavelengths and displays spectra asSν(λ/24)2 on a linear scale -
Dynamical effects of stellar massloss on a Kuiperlike belt
https://people.ast.cam.ac.uk/~wyatt/bmw11.pdf22 May 2012: However, the lowest mass planets scatter test particles moreweakly and thus fewer test particles end up with e > eSD = 0.24,our definition of the scattered disc and MSD is low -
Observing Kepler stars with WISE
https://people.ast.cam.ac.uk/~wyatt/kw12.pdf7 Jul 2012: Also shown is the sensitivity with MIPS at 24 and 70µm to55 Cancri, a typical nearby star at 12pc withKs 4.2 (grey lines). -
mnr_20522_LR
https://people.ast.cam.ac.uk/~wyatt/vw12.pdf30 Oct 2012: 2009), with q 24 au and a 796 au, and 2000 OO67 (Veillet, Doressoundiram &. Marsden 2001; Millis et al. 2002), with q 21 au and a 552 au.The perihelia and -
cv.dvi
https://people.ast.cam.ac.uk/~gpe/cv.pdf24 Jan 2012: CURRICULUM VITAE. FULL NAME: George Petros EFSTATHIOUNATIONALITY: BritishDATE OF BIRTH: 2nd Sept 1955. QUALIFICATIONS. Dates Academic Institution Degree. 10/73 to 7/76 Keble College, Oxford. B.A. in Physics10/76 to 9/79 Department of Physics, Ph.D. -
arX iv:1 201. 1911 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwsd12.pdf12 Jan 2012: 8 arcminaway to the SE (PA = 120) that is visible at 24, 70, and100µm. -
The Astrophysical Journal, 701:2019–2032, 2009 August 20…
https://people.ast.cam.ac.uk/~wyatt/lcwm09.pdf1 Aug 2012: edu. Received 2008 November 24; accepted 2009 June 16; published 2009 August 7. ... This agrees well with the200 K temperature of the large, cool grain dust grains fromthis work, and with Wyatt et al.’s (2007b) Spitzer 24/70 μmbased estimate of 4–5
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