Re-evaluating the Very Hot Gas Giant WASP-12b
Re-evaluating the Very Hot Gas Giant WASP-12b Re-evaluating the Very Hot Gas Giant WASP-12b
Modeling of initial eclipse photometry suggested that C/O ≥ 1 for WASP-12b Planet/star Flux Ratio (10 -3 ) Croll+2011 Campo+2011 Madhusudhan+2011 Madhusudhan+2011 6
Modeling of initial eclipse photometry suggested that C/O ≥ 1 for WASP-12b Planet/star Flux Ratio (10 -3 ) Croll+2011 Campo+2011 chi^2 ~ 10 Madhusudhan+2011 Madhusudhan+2011 7
- Page 1 and 2: Re-evaluating the Very Hot Gas Gian
- Page 3 and 4: E Transiting Planets with Measured
- Page 5: The Extreme Planet WASP-12b: Period
- 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 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
Modeling of initial eclipse photometry<br />
suggested that C/O ≥ 1 for <strong>WASP</strong>-<strong>12b</strong><br />
Planet/star Flux Ratio (10 -3 )<br />
Croll+2011<br />
Campo+2011<br />
Madhusudhan+2011<br />
Madhusudhan+2011<br />
6
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