**Porb** | Orbital period | days | |

**e** | Orbital eccentricity | - | These numbers are inhomogeneous: see 2011MNRAS.414.1278P. If an upper limit is available then the eccentricity will be given as 0.0 with the upper limit as the upper errorbar. |

**a** | Orbital semimajor axis | AU | |

**Teff** | Effective temperature of the star | Kelvin | |

**[Fe/H]** | Metal abundance of the star | Logarithmic relative to the Sun | I adopt [M/H] where a specific [Fe/H] is not available |

**M*** | Mass of the star | Msun | |

**R*** | Radius of the star | Rsun | |

**logg** | Surface gravity of the star | logarithmic in c.g.s. units | |

**ρ*** | Density of the star | ρsun | |

**Mp** | Mass of the planet | Mjup | Set to 0.0 if only an upper limit is known. The upper limit is then given as the upper errorbar. |

**Rp** | Radius of the planet | Rjup | |

**gp** | Surface gravity of the planet | m/s2 | |

**ρp** | Density of the planet | ρjup | Set to 0.0 if only an upper limit to the mass of the planet is known. The upper limit is then given as the upper errorbar. |

**Teq** | Equilibrium temperature of the planet | Kelvin | These numbers are inhomogeneous as different albedo and heat redistribution parameters are used by different people |