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https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt2 Jul 2010: It's hot (JCR) pleasant (MJI) down here - upper windows can be kept open 24/7 to keep the punters happier. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100922.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100922.txt26 Oct 2010: In the K-band, for example, the surface brightness of these stripes is between 23.5 and 24 mag/sq arcsec. -
arX iv:1 009. 0248 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf2 Sep 2010: 0.088725 24.3 0.4 2.3 3.2 -0.03 0.9 -0.1. ... K-band magnitudes from2MASS were extrapolated to 24 µm based on a set of pho-. -
arX iv:1 011. 1437 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/mctw10.pdf10 Nov 2010: at 18.1µm and 0.3 mJy/pixeland 9.8 mJy/pixel at 24.5µm. ... in the 18.1-µmimage and 29.9 in the 24.5-µm image. -
14667ms.dvi
https://people.ast.cam.ac.uk/~wyatt/mskp10.pdf27 May 2010: Type A3 Va A1 V F2 VPACS OM scan point-source scanD [pc] 11.0 24.3 18.2rms100 [mJy/beam] 1.4 3.1 1.2rms160 [mJy/beam] 3.9 ... Stars mark the 100and 160µm flux densities fromHerschel. Optical data were obtainedfrom Simbad and Vizier.Spitzer 24 and 70µm -
CASU WFCAM/VISTA Diary Page
https://people.ast.cam.ac.uk/~wfcam/diary.html24 Mar 2010: 24/25th October - UK VDFS Review at Cambridge. The documents are available here. -
arX iv:1 001. 5177 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/gw10.pdf29 Jan 2010: Averag-ing the measured E70 for these 24 stars we find 0.03 0.02. ... in prep.) will present the final model parame-ters fitting both 70 and 24 µm debris statistics among theSpitzer-surveyed FGK stars. -
Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 Feb 2010: We therefore arrive at Equation(9) by focusing on the 24 µm peak excesses. ... inferred from the 24 70 µm colour assuming blackbodygrains at a single temperature, Eq. -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: Afit to the Q band excess emission and the 24 and 70µm excessreported in Su et al. ... Su et al. (2006) presented new 24 and 70µmphotometry which also confirms the excess. -
arX iv:1 008. 0865 v2 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/cws10.pdf22 Aug 2010: Forexam-ple a disc with an inner radius of 24 AU, surface density profileΣ r7/3 between 24 and 34 AU, andΣ r1.5 from 34 to 90AU can fit the
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