relconv, relconv_lp, relconv_lp_ext: convolve with relativistic accretion disk line profile with different geometries

Convolves with one the family of relline line profiles. The basic code is described in Dauser et al. (2010) and the extension to lamp post geometries in Dauser et al. (2013).

The parameters for relconv are :

par1 | Index1: emissivity index for the inner disk |

par2 | Index2: emissivity index for the outer disk |

par3 | Rbr: break radius separating the inner and outer portions of the disk (gravitational radii) |

par4 | a: dimensionless black hole spin |

par5 | Incl: disk inclination angle to the line of sight (degrees) |

par6 | Rin: inner radius of the disk in units of the radius of marginal stability |

par7 | Rout: outer radius of the disk in units of the radius of marginal stability |

par8 | limb: limb-darkening/-brightening law with 0=isotropic, 1=darkening (flux 1+2.06mu), 2=brightening (flux ln(1+1/mu)) where mu=cos(emission angle) |

norm | flux in line (photons/cm/s) |

The parameters for relconvlp are :

par1 | h: height of the primary source (GM/c2) |

par2 | a: dimensionless black hole spin |

par3 | Incl: disk inclination angle to the line of sight (degrees) |

par4 | Rin: inner radius of the disk in units of the radius of marginal stability |

par5 | Rout: outer radius of the disk in units of the radius of marginal stability |

par6 | limb: limb-darkening/-brightening law with 0=isotropic, 1=darkening (flux 1+2.06mu), 2=brightening (flux ln(1+1/mu)) where mu=cos(emission angle) |

par7 | gamma: power-law index of the primary source (E-gamma) |

norm | flux in line (photons/cm/s) |

and the parameters for relconvlpext are :

par1 | a: dimensionless black hole spin |

par2 | Incl: disk inclination angle to the line of sight (degrees) |

par3 | Rin: inner radius of the disk in units of the radius of marginal stability |

par4 | Rout: outer radius of the disk in units of the radius of marginal stability |

par5 | limb: limb-darkening/-brightening law with 0=isotropic, 1=darkening (flux 1+2.06mu), 2=brightening (flux ln(1+1/mu)) where mu=cos(emission angle) |

par6 | gamma: power-law index of the primary source (E-gamma) |

par7 | hbase: lower height of radially extended primary source |

par8 | htop: upper height of radially extended primary source |

par9 | vbase: velocity of the source at hbase |

par10 | v100: velocity of the source at 100 rg above hbase |

norm | flux in line (photons/cm/s) |