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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. -
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_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_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_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 -
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. -
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. -
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 -
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. -
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
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