Model for the relativistically-broadened emission line from an accretion disk around a black hole. 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 relline are :
| par1 | lineE: rest frame line energy (keV) |
| par2 | Index1: emissivity index for the inner disk |
| par3 | Index2: emissivity index for the outer disk |
| par4 | Rbr: break radius separating the inner and outer portions of the disk (gravitational radii) |
| par5 | a: dimensionless black hole spin |
| par6 | Incl: disk inclination angle to the line of sight (degrees) |
| par7 | Rin: inner radius of the disk in units of the radius of marginal stability |
| par8 | Rout: outer radius of the disk in units of the radius of marginal stability |
| par9 | z: redshift |
| par10 | 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 rellinelp are :
| par1 | lineE: rest frame line energy (keV) |
| par2 | h: height of the primary source (GM/c2) |
| par3 | a: dimensionless black hole spin |
| par4 | Incl: disk inclination angle to the line of sight (degrees) |
| par5 | Rin: inner radius of the disk in units of the radius of marginal stability |
| par6 | Rout: outer radius of the disk in units of the radius of marginal stability |
| par7 | z: redshift |
| 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) |
| par9 | gamma: power-law index of the primary source (E-gamma) |
| norm | flux in line (photons/cm/s) |
and the parameters for rellinelpext are :
| par1 | lineE: rest frame line energy (keV) |
| 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 | z: redshift |
| par7 | 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) |
| par8 | gamma: power-law index of the primary source (E-gamma) |
| par9 | hbase: lower height of radially extended primary source |
| par10 | htop: upper height of radially extended primary source |
| par11 | vbase: velocity of the source at hbase |
| par12 | v100: velocity of the source at 100 rg above hbase |
| norm | flux in line (photons/cm/s) |