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WFCAM simulations
https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/index.html3 Sep 2007: Passband. H. Magnitude zero-point. 24.8. Magnitudes. Sky brightness. 13.6. Mags/arcsec2. Magnitude limits. ... imcore_conf. only (Figure 23) and median magnitude difference (Figure 24) were made. -
Data Flow System Document Title: VISTA Data Reduction Library ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0010_latest.pdf7 Jun 2007: 23 2.16 Illumination Correction. 24. 3 Functional Description. 26 3.1 Recipes. ... 13 / kk leads to a relative area of. )41()31).(1( 222 rkrkrk ′′′ (2-24). -
arX iv:0 704. 0873 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf18 Apr 2007: hot Jupiter –0.08 to 0.39 1.7–5 [500–1600] 70–200 1 % 2 1 %cool Jupiter –0.44 to 0.40 0.24–1.7 [75–500] ... 200 8 % 9 (5–11) %. planet & debris –0.13 to 0.27 0.10–0.24 [30–75] 5–30 5 % 3 1 %debris –0.52 to 0.18 -
hd113766_dust_25Sep2007
https://people.ast.cam.ac.uk/~wyatt/lcwm08.pdf5 Oct 2007: excess 24 and 70 µm flux. In their follow-on study, which provided the data used in this work,. ... silicate emission features at 9.8, 11.2, 16.2, 19, 24, and 34 µm. -
842 Publications of the Astronomical Society of the Pacific, ...
https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf18 Sep 2007: stellar luminosities. TheA stars (dark blue) are a sample of 46 detected at both 24 and 70mm (Wyattet al. ... A0, 3.6–24.8 pc for G0, and 1.8–8.6 pc for M0. -
MASS AND TEMPERATURE OF THE TWA 7 DEBRIS DISK ...
https://people.ast.cam.ac.uk/~wyatt/mkw07.pdf3 Jul 2007: 1), which fits the three longest wavelength fluxes, but cannotreproduce the 24 m flux. ... 1999, ApJ, 512, 377Hildebrand, R. 1983, QJRAS, 24, 267Holland, W. S., et al. -
arX iv:0 704. 3369 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/mlpw07.pdf26 Apr 2007: 24). In Figure 4 we compare models having5 MJ between the planets with and without disc matter lo-cated inside the inner planet. ... The mass distributionfollows equation (24) and the outer disc mass is varied bychanging parameter Σ0out. -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/wcg07.pdf18 Jul 2007: L. Arnold, F. Bouchy, C. Moutou (Paris: FrontierGroup), 24. Boss A., 2002, ApJ, 567, L149Butler R. -
Submitted to ApJ, 3 January 2007, accepted 22 March ...
https://people.ast.cam.ac.uk/~wyatt/wssr07.pdf23 Mar 2007: The 150t1age line delineatingthe upper envelope of the 24 µm detections (Rieke et al. ... 4.2.1. Sample of 46 A star disks detected at 24 and 70µm. -
Microsoft PowerPoint - wyattpub
https://people.ast.cam.ac.uk/~wyatt/wyatt_kobe06.pdf24 Apr 2007: stars at 24,70,160μm• Akari (2006-) currently doing all-sky survey 2-180μm• Herschel (2008-) observations at 60-670μm• Spica (2017+) planned 5-200μm. ... Structure is wavelength dependent!850μm. (Holland et al. 2006)24 and 70μm. (Su et al.
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