Search

3 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.

7 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).

18 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

5 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.

18 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.

3 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.

26 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.

18 Jul 2007: L. Arnold, F. Bouchy, C. Moutou (Paris: FrontierGroup), 24. Boss A., 2002, ApJ, 567, L149Butler R.

23 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.

24 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.