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https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_140122.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_140122.txt5 Mar 2014: the original Vega one based on ESO std fields observed each night APASSZPT= 24.147 / APASS ZP (mags) for default extinction APASSZRR= 0.012 / APASS ZP error (mags) APASSNUM= 104 / Number ... of APASS standards used NIGHTZPT= 24.155 / Average APASS ZP -
Irwin06draft.dvi
https://people.ast.cam.ac.uk/~wfcam/ukreview/Irwin06draft.pdf23 Jul 2014: 1 -2.4 3.8 4.84 18.4#2 3.7 4.2 4.87 20.5#3 -9.0 4.2 5.80 24.4#4 49.1 -
arX iv:1 402. 1184 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/dawk14.pdf10 Feb 2014: IRS pick-up camera at 16 and 22 µm and the MIPS 24 µm photometry to establish the absolute. ... and 22 µm and MIPS 24 µm broadband fluxes (listed in Table 3). -
betapic-final
https://people.ast.cam.ac.uk/~wyatt/dwra14.pdf8 Apr 2014: This was interpreted as a transition from a dust-‐producing planetesimal belt to a region dominated by submicron-‐sized grains blown out by radiation pressure (9,24). ... The dashed line is an axisymmetric model for the parent body distribution -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/fwgb14.pdf31 Jul 2014: 16 and MIPS 24 µm photometry (Farihi et al. 2008; Reach et al.2005). ... µMIPS 24 mµIRAC 8 m. Figure 1. Reduced infrared images of G29-38 taken with both Spitzer and Herschel. -
Mon. Not. R. Astron. Soc. 000, 1–22 (2013) Printed ...
https://people.ast.cam.ac.uk/~wyatt/jwbv14.pdf11 Mar 2014: which at 50AU from the Sun corresponds to σv/vk = 0.056,0.13, 0.27, 0.55, and 1.24. -
arX iv:1 312. 4531 v2 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kmlm13.pdf21 Jan 2014: Argon lamps were used for wave-length calibration. 24 images were taken with 1 second exposures. -
arX iv:1 408. 4116 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kw14.pdf22 Aug 2014: 4-35µm), three MIPS(24-160µm), and two SCUBA (450-850µm) bands. ... 2014). However, plotting their tempera-tures shows a probable correlation, with all Sun-like starshav-ing warm components<220K, but 15 out of 24 A-type starshaving warm components>220K -
arX iv:1 312. 5315 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwkd13.pdf21 Jan 2014: The expected December 2010 source position of α = 22h 48m 4.7s,δ = 24 22m 9.9s is at the centre of the images, and the PACS pointing accuracy for these ... Figure 3 shows the limits on the fractional luminosity of adisc around TW PsA given these -
Observations, Modeling and Theory of Debris Disks Brenda C. ...
https://people.ast.cam.ac.uk/~wyatt/mkwb14.pdf7 Jan 2014: 2008) and Dodson-Robinson et al. (2011)find rates of 4% at 24 µm in contrast to 16% at 70µm (Trilling et al. ... 7. 10-24. 10-22. 10-20. 10-18. 10-16. 100. 101. 102. 103. 104.
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