▼CGyoto::Python::Base | Base class for classes in the Python plug-in |
CGyoto::Astrobj::Python::Standard | Coding a Gyoto::Astrobj::Standard in Python |
CGyoto::Astrobj::Python::ThinDisk | Coding a Gyoto::Astrobj::ThinDisk in Python |
CGyoto::Metric::Python | Metric coded in Python |
CGyoto::Spectrum::Python | Loader for Python classes implementing the Spectrum interface |
▼CGyoto::Screen::Coord1dSet | Set of 1-d coordinates: indices or angles |
CGyoto::Screen::Angles | 1D specifier for an arbitrary angle coordinate set |
CGyoto::Screen::Indices | 1D specifier for an arbitrary pixel coordinate set |
CGyoto::Screen::Range | 1D coordinated specifier for a range |
CGyoto::Screen::RepeatAngle | 1D specifier for an angle that is repeated |
▼CGyoto::Screen::Coord2dSet | Class to specify a set of points on the Screen |
CGyoto::Screen::Bucket | Class containing arbitrary 2D-points |
CGyoto::Screen::Empty | A dummy, empty 2D set |
CGyoto::Screen::Grid | Class containing 2D-points organized in a grid |
▼CGyoto::Functor::Double_constDoubleArray | A functor like double (func) (double const data[]) |
►CGyoto::Astrobj::Standard | Astronomical objects defined bya a potential/distance |
CGyoto::Astrobj::DeformedTorus | |
CGyoto::Astrobj::FlaredDiskSynchrotron | |
CGyoto::Astrobj::Jet | Simple jet model with thermal or kappa-distribution synchrotron emission from Pandya et al. (2016) |
►CGyoto::Astrobj::NeutronStar | Neutron star defined by its surface ; no emission |
CGyoto::Astrobj::NeutronStarAnalyticEmission | Neutron star emitting at its surface an analytic emission, typically blackbody |
CGyoto::Astrobj::NeutronStarModelAtmosphere | Neutron star emitting at its surface an emission provided by a FITS table |
CGyoto::Astrobj::OscilTorus | |
CGyoto::Astrobj::PolishDoughnut | A toroidal accretion structure |
CGyoto::Astrobj::Python::Standard | Coding a Gyoto::Astrobj::Standard in Python |
CGyoto::Astrobj::ThickDisk | A thick accretion disk described by its opening angle between the BH spin axis and the disk surface, and its inner radius |
CGyoto::Astrobj::Torus | Optically thin or thick torus in circular rotation |
►CGyoto::Astrobj::UniformSphere | Optically thick or thin, spherical objects |
CGyoto::Astrobj::FixedStar | Fixed (i.e. non-moving) star (or spherical blob) |
►CGyoto::Astrobj::Star | Mass-less, spherical object following a timelike geodesic |
CGyoto::Astrobj::Blob | Blob of plasma following a Star orbit, emitting synchrotron, with Gaussian time-evolving density and temperature |
CGyoto::Astrobj::InflateStar | An Astrobj::Star with growing size |
CGyoto::Astrobj::StarTrace | Like a Star that would be on all points of its orbit at all time |
►CGyoto::Astrobj::ThinDisk | Geometrically thin disks and rings |
CGyoto::Astrobj::DirectionalDisk | Geometrically thin disk read from FITS file |
CGyoto::Astrobj::EquatorialHotSpot | |
CGyoto::Astrobj::PageThorneDisk | Geometrically thin disk in Kerr metric |
►CGyoto::Astrobj::PatternDisk | Geometrically thin disk read from FITS file |
►CGyoto::Astrobj::PatternDiskBB | Geometrically thin disk read from FITS file with black body spectrum |
►CGyoto::Astrobj::DynamicalDisk | Geometrically thin disk read from a set of FITS files |
CGyoto::Astrobj::DynamicalDiskBolometric | Geometrically thin disk read from a set of FITS files |
CGyoto::Astrobj::Python::ThinDisk | Coding a Gyoto::Astrobj::ThinDisk in Python |
CGyoto::Astrobj::ThinDiskIronLine | |
CGyoto::Astrobj::ThinDiskPL | Geometrically thin disk with black-body emission |
CGyoto::Astrobj::XillverReflection | The illumination table specifies how the thin disk is illuminated while the reflection table deduces from that the reflected spectrum as computed by Javier Garcia's XILLVER code |
▼CGyoto::Functor::Double_Double_const | A functor like double (func) (double) const |
CGyoto::Astrobj::PolishDoughnut::intersection_t | Double intersection(double) Functor class |
CGyoto::Astrobj::PolishDoughnut::outerradius_t | Double outerradius(double) Functor class |
CGyoto::Register::Entry | Entry in a register (or a full register) |
CGyoto::Error | Class for thowing exceptions |
CGyoto::Factory | XML input/output |
CGyoto::FactoryMessenger | Factory / SmartPointee::Subcontractor_t interface |
CGyoto::Property::getter_t | Union holding an accessor to get any type |
CGyoto::Property::getter_unit_t | Union holding an accessor to get double or vector<double> with unit |
▼CGyoto::GridData2D | Class for reading data stored in a 2D grid |
CGyoto::Astrobj::FlaredDiskSynchrotron | |
CGYOTO_ARRAY< T, sz > | |
CGyoto::Worldline::IntegState | |
▼CGyoto::Hook::Listener | I might listen to a Teller |
CGyoto::Astrobj::FlaredDiskSynchrotron | |
CGyoto::Astrobj::Jet | Simple jet model with thermal or kappa-distribution synchrotron emission from Pandya et al. (2016) |
CGyoto::Astrobj::OscilTorus | |
CGyoto::Astrobj::PageThorneDisk | Geometrically thin disk in Kerr metric |
CGyoto::Astrobj::PolishDoughnut | A toroidal accretion structure |
CGyoto::Astrobj::ThickDisk | A thick accretion disk described by its opening angle between the BH spin axis and the disk surface, and its inner radius |
CGyoto::Astrobj::XillverReflection | The illumination table specifies how the thin disk is illuminated while the reflection table deduces from that the reflected spectrum as computed by Javier Garcia's XILLVER code |
CGyoto::Spectrometer::Complex | Complex spectrometer object |
►CGyoto::Worldline | Timelike or null geodesics |
CGyoto::Astrobj::EquatorialHotSpot | |
CGyoto::Astrobj::Star | Mass-less, spherical object following a timelike geodesic |
►CGyoto::Photon | A null geodesic transporting light |
CGyoto::Photon::Refined | Refine last step of integration in a Photon |
CListenerItem | Private (undocumented) class to hold listeners_ |
CNumericalMetricLorene | Class for 3+1 numerical metrics computed by LORENE. This class can handle (so far) any kind of LORENE metric, stars, collapsing stars, Kerr, boson star e.g |
▼CGyoto::Object | Object with properties |
►CGyoto::Astrobj::Generic | Base class for astronomical object |
CGyoto::Astrobj::Complex | Complex astronomical object |
►CGyoto::Astrobj::Disk3D | Geometrically thick disk read from FITS file |
CGyoto::Astrobj::DynamicalDisk3D | Geometrically thick optically thin disk read from a set of FITS files |
CGyoto::Astrobj::Standard | Astronomical objects defined bya a potential/distance |
CGyoto::Astrobj::ThinDisk | Geometrically thin disks and rings |
►CGyoto::Metric::Generic | Base class for metrics |
CGyoto::Metric::Hayward | Metric of a regular rotating black hole or naked worm-hole |
►CGyoto::Metric::KerrBL | Metric around a Kerr black-hole in Boyer-Lindquist coordinates |
CGyoto::Metric::ChernSimons | |
CGyoto::Metric::KerrKS | Metric around a Kerr black-hole in Kerr-Schild coordinates Warning: this metric is seldom used and may be buggy |
CGyoto::Metric::Minkowski | The Minkowski flat-space metric |
CGyoto::Metric::NumericalMetricLorene | |
CGyoto::Metric::Python | Metric coded in Python |
CGyoto::Metric::RezzollaZhidenko | |
CGyoto::Metric::RotStar3_1 | Numerical metric around a rotating star in 3+1 formalism |
CGyoto::Photon | A null geodesic transporting light |
CGyoto::Scenery | Ray-tracing scene |
CGyoto::Screen | The camera with which the Astrobj is observed |
►CGyoto::Spectrometer::Generic | Base class for spectrometers |
CGyoto::Spectrometer::Complex | Complex spectrometer object |
CGyoto::Spectrometer::Uniform | Uniformly spaced spectrometers |
►CGyoto::Spectrum::Generic | Spectrum emitted by an Astrobj |
CGyoto::Spectrum::BlackBody | Black Body |
CGyoto::Spectrum::KappaDistributionSynchrotron | Kappa-distribution synchrotron spectrum from Pandya et al. (2016) |
CGyoto::Spectrum::PowerLaw | I_nu=constant_*nu^exponent_ |
CGyoto::Spectrum::PowerLawSynchrotron | Powerlaw synchrotron spectrum |
CGyoto::Spectrum::Python | Loader for Python classes implementing the Spectrum interface |
CGyoto::Spectrum::ThermalBremsstrahlung | Thermal brems spectrum |
CGyoto::Spectrum::ThermalSynchrotron | Thermal synchrotron spectrum |
CGyoto::Property | Property that can be set and got using standard methods |
CGyoto::Property::setter_t | Union holding an accessor to set any type |
CGyoto::Property::setter_unit_t | Union holding an accessor to set double or vector<double> with unit |
▼CGyoto::SmartPointee | Can be pointed to by a SmartPointer |
CGyoto::Astrobj::Generic | Base class for astronomical object |
CGyoto::Astrobj::Properties | Observable properties of an Astronomical object |
CGyoto::Metric::Generic | Base class for metrics |
CGyoto::Photon | A null geodesic transporting light |
CGyoto::Scenery | Ray-tracing scene |
CGyoto::Screen | The camera with which the Astrobj is observed |
CGyoto::Spectrometer::Generic | Base class for spectrometers |
CGyoto::Spectrum::Generic | Spectrum emitted by an Astrobj |
►CGyoto::Worldline::IntegState::Generic | Current state of a geodesic integration |
CGyoto::Worldline::IntegState::Legacy | Obsolete: Home-brewed integrator |
CGyoto::SmartPointer< T > | Pointers performing reference counting |
CGyoto::SmartPointer< Gyoto::Astrobj::Generic > | |
CGyoto::SmartPointer< Gyoto::Metric::Generic > | |
CGyoto::SmartPointer< Gyoto::Metric::KerrBL > | |
CGyoto::SmartPointer< Gyoto::Metric::NumericalMetricLorene > | |
CGyoto::SmartPointer< Gyoto::Photon > | |
CGyoto::SmartPointer< Gyoto::Scenery > | |
CGyoto::SmartPointer< Gyoto::Screen > | |
CGyoto::SmartPointer< Gyoto::Spectrometer::Generic > | |
CGyoto::SmartPointer< Gyoto::Spectrum::BlackBody > | |
CGyoto::SmartPointer< Gyoto::Spectrum::Generic > | |
CGyoto::SmartPointer< Gyoto::Spectrum::KappaDistributionSynchrotron > | |
CGyoto::SmartPointer< Gyoto::Spectrum::PowerLawSynchrotron > | |
CGyoto::SmartPointer< Gyoto::Spectrum::ThermalBremsstrahlung > | |
CGyoto::SmartPointer< Gyoto::Spectrum::ThermalSynchrotron > | |
CGyoto::SmartPointer< Gyoto::Units::Converter > | |
CGyoto::SmartPointer< Gyoto::Worldline::IntegState::Generic > | |
▼CGyoto::Hook::Teller | Listen to me and I'll warn you when I change |
CGyoto::Metric::Generic | Base class for metrics |
CGyoto::Spectrometer::Generic | Base class for spectrometers |
CGyoto::Value | Container for the value of a Property |
CGyoto::WIP | Base class for work in progress |