Re-evaluating the Very Hot Gas Giant WASP-12b

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Step 2: IRTF/SpeX Imaging of <strong>WASP</strong>-12 and Bergfors-2. 16
IRTF/SpeX K-band imaging shows that Bergfors-2 is redder than <strong>WASP</strong>-12 Δi = 4.0 mag Bergfors et al. 2011 ΔK = 2.5 mag Eclipse dilution is greater at longer λ Crossfield et al., submitted 17
Page 1 and 2: Re-evaluating the Very Hot Gas Gian
Page 3 and 4: E Transiting Planets with Measured
Page 5 and 6: The Extreme Planet WASP-12b: Period
Page 7 and 8: Modeling of initial eclipse photome
Page 9 and 10: Step 1: Subaru/MOIRCS narrowband 2.
Page 11 and 12: Planet/star Flux Ratio (10 -3 ) Cro
Page 13 and 14: Campo+2011 Cowan+2012 4.5µm Eclips
Page 15: A fainter star very close to WASP-1
Page 19 and 20: Transit/Eclipse contamination Keck/
Page 21 and 22: Dilution-corrected planetary spectr
Page 23 and 24: The similarly hot (~3200 K) planet
Page 25 and 26: A high C/O ratio cannot be defended
Page 27 and 28: Followup observations will confirm
Page 29: Conclusions: ● An M0 dwarf is loc
Page 32 and 33: de Mooij poster; Preliminary! Swain
Page 34: Planet/Star Flux Density (10 -3 ) F

Re-evaluating the Very Hot Gas Giant WASP-12b

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