PI: Debra Fischer, San Francisco State University, firstname.lastname@example.org
Address: Physics Department, 1600 Holloway, San Francisco, CA 94132, USA
CoI: Greg Laughlin, UC Santa Cruz
CoI: R. Paul Butler, Carnegie Institution, Washington D. C.
Title: N2K: Detection of Short-Period Extrasolar Planets
Abstract: The N2K program is designed to screen metal-rich stars for the presence of short-period planets with \msini comparable to or greater than Saturn. In the past year, this program has detected 4 new short period planets and there are 35 excellent planet candidates showing curvature and 3-10 sigma scatter in radial velocities. All short period candidates are followed with photometry to search for transits and one planet, HD149026b, was observed to transit its host star with a 3 mmag transit depth (1/5 the transit depth of HD209458). This transit would have likely been missed by photometric surveys, emphasizing the key role that Doppler observations from the N2K program play in transit detections. We request time to continue this program in order to obtain 3 radial velocity measurements for a set of 120 new stars.
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360