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SEEDS: Strategic Explorations of Exoplanets and Disks with Subaru

Published online by Cambridge University Press:  06 January 2014

Motohide Tamura
Affiliation:
Dept. of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan email: motohide.tamura@nao.ac.jp / motohide.tamura@astron.s.u-tokyo.ac.jp
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Abstract

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SEEDS is the first Subaru Strategic Program, whose aim is to conduct a direct imaging survey for giant planets as well as protoplanetary/debris disks at a few to a few tens of AU region around 500 nearby solar-type or more massive young stars devoting 120 Subaru nights for 5 years. The targets are composed of five categories spanning the ages of ~1 Myr to ~1 Gyr. Some RV-planet targets with older ages are also observed. The survey employs the new high-contrast instrument HiCIAO, a successor of the previous NIR coronagraph camera CIAO for the Subaru Telescope. We describe the outline of this survey and present its first three years of results. The survey has published ~20 refereed papers by now. The main results are as follows: (1) detection and characterization of the most unequivocal and lowest-mass planet via direct imaging. (2) detection of a super-Jupiter around the most massive star ever imaged, (3) detection of companions around a retrograde exoplanet system, which supports the Kozai mechanism for the origin of retrograde orbit (not in this proceedings, but see Narita et al. 2010, 2012). We also report (4) the discovery of unprecedentedly detailed structures of more than a dozen of protoplanetary disks and some debris disks. The detected structures such as wide gaps and spirals arms of a Solar-system scale could be signpost of planet.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

References

Brandt, T. D.et al. 2013a, ApJ, 764, 183CrossRefGoogle Scholar
Brandt, T. D.et al. 2013b, ApJ in pressGoogle Scholar
Carson, J.et al. 2013, ApJ, 763, L32CrossRefGoogle Scholar
Dong, R.et al. 2012a, ApJ, 750, 161Google Scholar
Dong, R.et al. 2012b, ApJ, 760, 111Google Scholar
Follette, K.et al. 2013, ApJ, 767, 10CrossRefGoogle Scholar
Grady, C.et al. 2013, ApJ, 762, 48Google Scholar
Hashimoto, J.et al. 2011, ApJ, 729, L17Google Scholar
Hashimoto, J.et al. 2012, ApJ, 758, L19CrossRefGoogle Scholar
Hodapp, K.et al. 2006, Proc. SPIE, 6269, 62693VCrossRefGoogle Scholar
Janson, M.et al. 2011, ApJ, 728, 85Google Scholar
Janson, M.et al. 2013, ApJ, in pressGoogle Scholar
Kusakabe, N.et al. 2012, ApJ, 753, 153Google Scholar
Kuzuhara, M.et al. 2013, ApJ, in pressGoogle Scholar
Mayama, S.et al. 2012, ApJ, 760, L26CrossRefGoogle Scholar
Muto, T.et al. 2012, ApJ, 748, L22CrossRefGoogle Scholar
Narita, N.et al. 2010, PASJ, 62, 779CrossRefGoogle Scholar
Narita, N.et al. 2012, PASJ, 64, 124Google Scholar
Tamura, M.et al. 2006, Proc. SPIE, 6269, 62690VCrossRefGoogle Scholar
Takami, M.et al. 2013, ApJ, 772, 145CrossRefGoogle Scholar
Tanii, R.et al. 2012, PASJ, 64, 124CrossRefGoogle Scholar
Thalmann, C.et al. 2012, ApJ, 707, L123Google Scholar
Thalmann, C.et al. 2010, ApJ, 718, L87CrossRefGoogle Scholar
Thalmann, C.et al. 2011, ApJ, 743, L6Google Scholar
Thalmann, C.et al. 2013, ApJ, 763, L29CrossRefGoogle Scholar
Yamamoto, K.et al. 2013, PASJ, in pressGoogle Scholar