Introduction of the RV subcategory of the SEEDS project 1.57 Yasuhiro H. Takahashi GUAS/NAOJ and the RV subcategory member

What is the RV subcategory? a part of the SEEDS project – using the direct imaging method with HiCIAO instrument on board the Subaru telescope – Detail in poster by Kusakabe One of the subcategories of the NS category – Nearby Stars – stars harboring one/some planet(s) detected with the RV method – especially, we are targeting stars with the following characteristics.

Our strategy 1) Stars which have long-term trend in radial velocity – considered to be caused such RV trends by unknown planets 2) Stars which harbor inner planets having considerably high orbital eccentricity or obliquity with the spin of its host star – Planet-planet scattering (e.g., Nagasawa+ 2008) – Kozai oscillation + Tidal friction (e.g., Fabrycky & Tremaine 2007) We can possibly detect unknown outer planets by the direct imaging method! – Even if we can’t detect the outer bodies in our targets, we can impose conditions and limits on the theoretical models.

Our results Images of our targets taken by the HiCIAO instrument Typical contrast and detection limit in mass Narita et al. was published. Details in poster by Narita

Grazie!