A Survey of Close, Young Stars with the Simultaneous Differential Imager (SDI) at the VLT and MMT

Details A Survey of Close, Young Stars with the Simultaneous Differential Imager (SDI) at the VLT and MMT A Survey of Close, Young Stars with the Simultaneous Differential Imager (SDI) at the VLT and MMT

2006-01-03

arxiv.org/abs/astro-ph/0601062v1

Astronomy and Astrophysics

Astrophysics

7 pages, 3 figures, 1 table. Presented at IAU Colloquium 200, Direct Imaging of Exoplanets: Science and Techniques. For high r

Scientific paper

We discuss the preliminary results of a survey of young (<300 Myr), close (<50 pc) stars with the Simultaneous Differential Extrasolar Planet Imager (SDI) implemented at the VLT and the MMT. SDI uses a double Wollaston prism and a quad filter to take 4 identical images simultaneously at 3 wavelengths surrounding the 1.62 um methane bandhead found in the spectrum of cool brown dwarfs and gas giants. By performing a difference of images in these filters, speckle noise from the primary can be significantly attenuated, resulting in photon noise limited data. In our survey data, we achieved H band contrasts >25000 (5 sigma Delta F1(1.575 um) > 10 mag, Delta H > 11.5 mag for a T6 spectral type) at a separation of 0.5" from the primary star. With this degree of attenuation, we should be able to image (5 sigma detection) a 2-4 Jupiter mass planet at 5 AU around a 30 Myr star at 10 pc. We are currently completing our survey of young, nearby stars. We have obtained complete datasets for 35 stars in the southern sky (VLT) and 7 stars in the northern sky (MMT). We believe that our SDI images are the highest contrast astronomical images ever made from ground or space for methane rich companions.

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