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HAT P 12b: A Low Density Sub Saturn Mass Planet Transiting a Metal Poor K Dwarf

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Figure 1. Unbinned light curve of HAT-P-12 including all 2927 instrumental I-band 5.5 minute cadence measurements obtained with the HAT-5 (Arizona) telescope of HATNet (see the text for details), and folded with the period of P = 3.2130598 days (which is t
Figure 2. Top: RV measurements from Keck for HAT-P-12, along with an orbital fit, shown as a function of orbital phase, using our best-fit period (see Section 3)
Figure 4. Stellar isochrones from Baraffe et al. (1997, 1998) for metallicity [Fe/H] = −0.29 and ages 0.2, 0.5, 1.0, 2.0, 3.0, 4.0, 5.0, and 6.0 Gyr
Table 4 Blend Configurations
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