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Table 4

Occultation depths and mid-occultation phases of WASP-48.

Waveband (μm) From O’Rourke et al. (2014) Final MCMCs Individual MCMCs Residual permutation
Occult. depth (%) Phase of mid-occult. Occult. depth (%) Phase of mid-occult.b Occult. depth (%) Phase of mid-occult. Occult. depth (%) Phase of mid-occult.

1.6 (H) 0.047 ± 0.016 0.5010 ± 0.0013 0.050 ± 0.016 0.5003 ± 0.0006 0.050 ± 0.015 0.5030 ± 0.0069 0.057 ± 0.017 0.5009 ± 0.0063
2.1 (Ks) (Palomar) 0.109 ± 0.027 0.5010 ± 0.0013 0.136 ± 0.014a 0.5003 ± 0.0006 0.108 ± 0.026 0.5003 ± 0.0024 0.120 ± 0.024 0.5005 ± 0.0022
2.1 (Ks) (CFHT) 0.136 ± 0.014a 0.5003 ± 0.0006 0.138 ± 0.014c 0.4998 ± 0.0010c 0.135 ± 0.014 0.5002 ± 0.0009
3.6 0.176 ± 0.013 0.5001 ± 0.0026 0.176 ± 0.013 0.5003 ± 0.0006 0.177 ± 0.013 0.5001 ± 0.0007 0.180 ± 0.011 0.5004 ± 0.0010
4.5 0.214 ± 0.020 0.5013 ± 0.0015 0.213 ± 0.021 0.5003 ± 0.0006 0.213 ± 0.020 0.5023 ± 0.0012 0.224 ± 0.013 0.5005 ± 0.0006

Notes. We adopt the values in bold. (a)We fit a single model to both Ks-band data sets in each MCMC. (b)In the global MCMCs the occultation mid-phase and duration were common to each lightcurve. (c) Values were obtained from the combined posteriors of the individual MCMCs as discussed in Sect. 3.2.

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