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https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_101027.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_101027.txt3 Dec 2010: The faulty CCD has been replaced and the whole array is co-planar to /- 20 microns. ... Approximately 20% of the band-merged VHS tile products investigated had a serious problem with the photometry due to this effect (though it is a moot point if most of -
Question_sheet
https://people.ast.cam.ac.uk/~gpe/Question_sheet_1.pdf1 Mar 2010: Consider the process. ˜ χ 20 ˜ ˜ χ 1. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100216.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100216.txt24 Mar 2010: 4. Data archives update AAT, ING, WFCAM, VISTA: all going smoothly UKIRT: JRL reported that he was still awaiting the last 20 or so nights of missing data. -
https://people.ast.cam.ac.uk/~pettini/canaries13/cupconf.sty
https://people.ast.cam.ac.uk/~pettini/canaries13/cupconf.sty5 Oct 2010: start of cupconf.sty %%%%%%%%%%%%%%%%%%%%%% % CUPconf.sty -- CUP conference proceedings style file % V0.1 released 20 September 1993, by Alison Woollatt % Copyright (1993) Cambridge University Press % This software may only be used ... 2,space}}% % -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100826.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100826.txt30 Aug 2010: Although only a few % in the Ks band the effect is approaching 15-20% in the Y and Z-bands. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100421.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100421.txt5 May 2010: 5 new BLADES (20 cores) have been acquired and added to the VISTA processing kit and SC is in the process of connecting them up and installing an operating system on -
14667ms.dvi
https://people.ast.cam.ac.uk/~wyatt/mskp10.pdf27 May 2010: For point-source mode ob-servations, seven contiguous repeat chop/nod observations wereperformed. Scan map observations had eight repeats in a singlescan direction at a rate of 20′′/s. ... 20 Dept. of Physics & Astronomy, University of California, -
CASU WFCAM/VISTA Diary Page
https://people.ast.cam.ac.uk/~wfcam/diary.html24 Mar 2010: March 2008. 18-20 March - UltraVista meeting in Leiden, MJI and JRL part attended and gave talks. -
arX iv:1 009. 0248 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf2 Sep 2010: In the general stellar population, theextrapolated planet total is 17-20 % (Cumming et al. ... 2008; Greaves & Wyatt 2010), which agreewell with the predictions of 21 and 20 % respectively. -
arX iv:1 001. 5177 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/gw10.pdf29 Jan 2010: The high-est mass appears realistic, for example it is comparable tothe 20-30 M of colliders inferred around the A-star Fomal-haut (Wyatt & Dent 2002), which hosts a bright ... 2008) estimate that 18 % of Sun-likestars host giant planets, of above about -
arX iv:1 011. 1437 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/mctw10.pdf10 Nov 2010: 0 20 40 60 80 10090. 95. 100. 105. 110. Radius! ... The expected flux density calculated withthis relation agrees with the flux density values both from ob-servations and from our model to within 20% at 0.57, 1.1, and1.6µm. -
arX iv:1 012. 3079 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/mw11.pdf15 Dec 2010: 127271 39.081915 1734.49 69459.2 20.3629 1798.92 127704 24.029317 2272.84 68903.7 13.6835 2346.56 128024 15.814919 2883.61 68472.8 9.63420 -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: SiC 11.85 1800 VISIR 124 120 23 3 7Q2 18.72 3760 VISIR 50 119 11 9 20. ... The recent 24µm and 18µmdetections presented here suggest a lower excess than that sug-gested by IRAS photometry (275 20 mJy at 25µm). -
arX iv:1 007. 4517 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/bw10.pdf27 Jul 2010: larly at 70µmFdiscF. = 1-5 (diamond:small excess), 5-20 (square:. medium excess), >20 (triangle: large excess). ... that extends down to 1010m,the contribution of particles less than 108m in size to the24µm disc flux is only 20%. -
arX iv:1 008. 0865 v2 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/cws10.pdf22 Aug 2010: 1.32 46.8 2.64 5.9 104 20 1 6HD 181327 F5/6V 1.3 51 3.1 3103 20 [86] 7,1,6,12,13 7 (Resolved -
Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 Feb 2010: This differentemphasis changes the values obtained in the formal fit at24 µm by 10–20%.3. ... For belts rmid = 20, 30, 40,50, 60, and 70 AU, dr = rmid/2, and η = 1. -
Collisional Evolution of Irregular Satellite Swarms: Detectable Dust…
https://people.ast.cam.ac.uk/~wyatt/kw11.pdf25 Nov 2010: Integrating equation (19) yields. Dc =Dmax. (1 0.4(t tnleft)/tnleft)α. (20). where α = 1/1.2. ... When there are only Nstr largest objects left, Dcbegins to decay as dictated by Equation (20).
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