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観測的宇宙論ジャーナルクラブ 2006年5月22日
成田 憲保
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Origin of the obliquities of the giant planets in mutual
interactions in the early Solar System
A. Brunini
Nature, vol. 440, pp.
1163, (2006)
2
A Determination of the Spin-Orbit Alignment of the
Anomalously Dense Planet Orbiting HD 149026
A. Wolf et al.
ApJ, accepted
3
Detectability of Planetary Characteristics in DiskAveraged Spectra. I: The Earth Model
G. Tinetti et al.
Astrobiology, vol. 6,
No. 1, pp. 34, (2006)
4
Vegetation signature in the observed globally-integrated
spectrum of Earth: Modeling the red-edge strength using
simultaneous cloud data and application for extrasolar
planets
P. Montanes-Rodriguez,
E. Palle, P. Goode
astro-ph/0604420
5
An extrasolar planetary system with three Neptunemass planets
C. Lovis et al.
Nature, vol. 441, pp.
305, (2006)
6
A Transiting Planet of a Sun-like Star
P. McCullough et al.
astro-ph/0605414
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Fig. 9