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

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Planet/star Flux Ratio (10 -3 ) Croll+2011 Cowan+2012 Campo+2011 Madhusudhan+2011 Madhusudhan+2011 12
Campo+2011 Cowan+2012 4.5µm Eclipses of <strong>WASP</strong>-<strong>12b</strong>: 0.382 ± 0.019 % 0.39 ± 0.03 % (very prolate planet) Or 0.50 ± 0.04 % (non-prolate planet) 13
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: Planet/star Flux Ratio (10 -3 ) Cro
Page 15 and 16: A fainter star very close to WASP-1
Page 17 and 18: IRTF/SpeX K-band imaging shows that
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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