Table 1.

Table showing best-fitting model parameters, RCF, metallicity (M/H), C/O ratio, internal temperature (T|$_{\rm int}$|⁠) from the self-consistent atmosphere model grid for each planet using their HST and/or Spitzer observations. The best-fitting model reduced |$\chi ^2_{\rm red}$| value is also shown.

PlanetRCFM/H (x solar)C/OT|$_{\rm int}$| (K)|$\chi ^2_{\rm red}$|
WASP-0181.20.630.554001.28
WASP-1211.00.630.84001.56
WASP-0770.80.0630.011001.37
WASP-0430.80.010.12001.61
WASP-0170.82.52.01001.1
WASP-0191.01000.011000.025
PlanetRCFM/H (x solar)C/OT|$_{\rm int}$| (K)|$\chi ^2_{\rm red}$|
WASP-0181.20.630.554001.28
WASP-1211.00.630.84001.56
WASP-0770.80.0630.011001.37
WASP-0430.80.010.12001.61
WASP-0170.82.52.01001.1
WASP-0191.01000.011000.025
Table 1.

Table showing best-fitting model parameters, RCF, metallicity (M/H), C/O ratio, internal temperature (T|$_{\rm int}$|⁠) from the self-consistent atmosphere model grid for each planet using their HST and/or Spitzer observations. The best-fitting model reduced |$\chi ^2_{\rm red}$| value is also shown.

PlanetRCFM/H (x solar)C/OT|$_{\rm int}$| (K)|$\chi ^2_{\rm red}$|
WASP-0181.20.630.554001.28
WASP-1211.00.630.84001.56
WASP-0770.80.0630.011001.37
WASP-0430.80.010.12001.61
WASP-0170.82.52.01001.1
WASP-0191.01000.011000.025
PlanetRCFM/H (x solar)C/OT|$_{\rm int}$| (K)|$\chi ^2_{\rm red}$|
WASP-0181.20.630.554001.28
WASP-1211.00.630.84001.56
WASP-0770.80.0630.011001.37
WASP-0430.80.010.12001.61
WASP-0170.82.52.01001.1
WASP-0191.01000.011000.025
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close