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
The dilution- corrected planetary spectrum is very nearly a blackbody: A high C/O ratio cannot be defended when a two-parameter (blackbody) model fits as well as do many-parameter (radiative-transfer) models. chi^2 k BIC Blackbody ~15 2 19 C/O > 1 ~10 >10 >32 Crossfield et al., submitted 24
A high C/O ratio cannot be defended when a two-parameter (blackbody) model fits as well as do many-parameter (radiative-transfer) models. chi^2 k BIC Blackbody ~25 2 29 C/O > 1 ~10 >10 >32 25
- 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 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: The similarly hot (~3200 K) planet
- 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
The dilution-<br />
corrected planetary<br />
spectrum is very<br />
nearly a blackbody:<br />
A high C/O ratio cannot be defended<br />
when a two-parameter (blackbody) model fits as well<br />
as do many-parameter (radiative-transfer) models.<br />
chi^2 k BIC<br />
Blackbody ~15 2 19<br />
C/O > 1 ~10 >10 >32<br />
Crossfield et al., submitted<br />
24
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