Table 2
Observed data used in the WASP-43b retrieval setups described in this work.
| Observation type | Phase (°) | Centred on | Instrument |
|---|---|---|---|
| Phase | 45 | Nightside | HST WFC3/Spitzer IRAC |
| Phase | 67.5 (a) | Nightside | HST WFC3/Spitzer IRAC |
| Phase | 90 (b) | Evening | HST WFC3/Spitzer IRAC |
| Phase | 112.5 (a) | Dayside | HST WFC3/Spitzer IRAC |
| Phase | 135 (c) | Dayside | HST WFC3/Spitzer IRAC |
| Phase | 157.5 | Dayside | HST WFC3/Spitzer IRAC |
| Phase | 180 | Dayside | HST WFC3/Spitzer IRAC |
| Phase | 202.5 | Dayside | HST WFC3/Spitzer IRAC |
| Phase | 225 (c) | Dayside | HST WFC3/Spitzer IRAC |
| Phase | 247.5 (a) | Dayside | HST WFC3/Spitzer IRAC |
| Phase | 270 | Morning | HST WFC3/Spitzer IRAC |
| Phase | 315 | Nightside | HST WFC3/Spitzer IRAC |
| Transmission | – | Terminators (combined) | HST WFC3 |
Notes. All phase data from HST are from Stevenson et al. (2014). The phase data observed using Spitzer are from Stevenson et al. (2017) and were independently reduced by two different sources: Stevenson et al. (2017) or Mendonça et al. (2018a). We use slightly different phases in this work for these two cases, as detailed in the footnote of this table. Transmission HST data are from Kreidberg et al. (2014). HST WFC3 refers to the Hubble Space Telescope Wide Field Camera 3, and IRAC to the Infrared Array Camera on board Spitzer. (a) This phase was used in retrieval setups using the Mendonça et al. (2018a) Spitzer points only. (b) This phase considers HST WFC3 data only for the retrieval cases using the Mendonça et al. (2018a) Spitzer points. (c) This phase was used in retrieval setups using the Stevenson et al. (2017) Spitzer points only.
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