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Gyoto
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| ▼NGyoto | Namespace for the Gyoto library |
| ▼NAstrobj | Access to astronomical objects |
| ►NPython | Classes that wrap Python classes as Gyoto Astrobj implementations |
| CBlob | Blob of plasma following a Star orbit, emitting synchrotron, with Gaussian time-evolving density and temperature |
| CComplex | Complex astronomical object |
| CDeformedTorus | |
| CDirectionalDisk | Geometrically thin disk read from FITS file |
| CDisk3D | Geometrically thick disk read from FITS file |
| CDynamicalDisk | Geometrically thin disk read from a set of FITS files |
| CDynamicalDisk3D | Geometrically thick optically thin disk read from a set of FITS files |
| CDynamicalDiskBolometric | Geometrically thin disk read from a set of FITS files |
| CEquatorialHotSpot | |
| CFixedStar | Fixed (i.e. non-moving) star (or spherical blob) |
| CFlaredDiskSynchrotron | |
| CGeneric | Base class for astronomical object |
| CInflateStar | An Astrobj::Star with growing size |
| CJet | Simple jet model with thermal or kappa-distribution synchrotron emission from Pandya et al. (2016) |
| CNeutronStar | Neutron star defined by its surface ; no emission |
| CNeutronStarAnalyticEmission | Neutron star emitting at its surface an analytic emission, typically blackbody |
| CNeutronStarModelAtmosphere | Neutron star emitting at its surface an emission provided by a FITS table |
| COscilTorus | |
| CPageThorneDisk | Geometrically thin disk in Kerr metric |
| CPatternDisk | Geometrically thin disk read from FITS file |
| CPatternDiskBB | Geometrically thin disk read from FITS file with black body spectrum |
| ►CPolishDoughnut | A toroidal accretion structure |
| CProperties | Observable properties of an Astronomical object |
| CStandard | Astronomical objects defined bya a potential/distance |
| CStar | Mass-less, spherical object following a timelike geodesic |
| CStarTrace | Like a Star that would be on all points of its orbit at all time |
| CThickDisk | A thick accretion disk described by its opening angle between the BH spin axis and the disk surface, and its inner radius |
| CThinDisk | Geometrically thin disks and rings |
| CThinDiskIronLine | |
| CThinDiskPL | Geometrically thin disk with black-body emission |
| CTorus | Optically thin or thick torus in circular rotation |
| CUniformSphere | Optically thick or thin, spherical objects |
| CXillverReflection | 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 |
| ▼NFunctor | Classes with an operator() method |
| CDouble_constDoubleArray | A functor like double (func) (double const data[]) |
| CDouble_Double_const | A functor like double (func) (double) const |
| ▼NHook | Listeners attach to Tellers |
| CListener | I might listen to a Teller |
| CTeller | Listen to me and I'll warn you when I change |
| ▼NMetric | Access to metrics |
| CChernSimons | |
| CGeneric | Base class for metrics |
| CHayward | Metric of a regular rotating black hole or naked worm-hole |
| CKerrBL | Metric around a Kerr black-hole in Boyer-Lindquist coordinates |
| CKerrKS | Metric around a Kerr black-hole in Kerr-Schild coordinates Warning: this metric is seldom used and may be buggy |
| CMinkowski | The Minkowski flat-space metric |
| CNumericalMetricLorene | |
| CPython | Metric coded in Python |
| CRezzollaZhidenko | |
| CRotStar3_1 | Numerical metric around a rotating star in 3+1 formalism |
| ▼NPython | Helpers for the classes deriving from Gyoto::Python::Base |
| CBase | Base class for classes in the Python plug-in |
| ▼NRegister | Gyoto registers |
| CEntry | Entry in a register (or a full register) |
| ▼NSpectrometer | Access to spectrometers |
| CComplex | Complex spectrometer object |
| CGeneric | Base class for spectrometers |
| CUniform | Uniformly spaced spectrometers |
| ▼NSpectrum | Spectrum of a simple object (e.g. a Gyoto::Astrobj::Star) |
| CBlackBody | Black Body |
| CGeneric | Spectrum emitted by an Astrobj |
| CKappaDistributionSynchrotron | Kappa-distribution synchrotron spectrum from Pandya et al. (2016) |
| CPowerLaw | I_nu=constant_*nu^exponent_ |
| CPowerLawSynchrotron | Powerlaw synchrotron spectrum |
| CPython | Loader for Python classes implementing the Spectrum interface |
| CThermalBremsstrahlung | Thermal brems spectrum |
| CThermalSynchrotron | Thermal synchrotron spectrum |
| NUnits | Units-related classes and functions |
| CError | Class for thowing exceptions |
| CFactory | XML input/output |
| CFactoryMessenger | Factory / SmartPointee::Subcontractor_t interface |
| CGridData2D | Class for reading data stored in a 2D grid |
| CObject | Object with properties |
| ▼CPhoton | A null geodesic transporting light |
| CRefined | Refine last step of integration in a Photon |
| ▼CProperty | Property that can be set and got using standard methods |
| Cgetter_t | Union holding an accessor to get any type |
| Cgetter_unit_t | Union holding an accessor to get double or vector<double> with unit |
| Csetter_t | Union holding an accessor to set any type |
| Csetter_unit_t | Union holding an accessor to set double or vector<double> with unit |
| CScenery | Ray-tracing scene |
| ▼CScreen | The camera with which the Astrobj is observed |
| CAngles | 1D specifier for an arbitrary angle coordinate set |
| CBucket | Class containing arbitrary 2D-points |
| CCoord1dSet | Set of 1-d coordinates: indices or angles |
| CCoord2dSet | Class to specify a set of points on the Screen |
| CEmpty | A dummy, empty 2D set |
| CGrid | Class containing 2D-points organized in a grid |
| CIndices | 1D specifier for an arbitrary pixel coordinate set |
| CRange | 1D coordinated specifier for a range |
| CRepeatAngle | 1D specifier for an angle that is repeated |
| CSmartPointee | Can be pointed to by a SmartPointer |
| CSmartPointer | Pointers performing reference counting |
| CValue | Container for the value of a Property |
| CWIP | Base class for work in progress |
| ▼CWorldline | Timelike or null geodesics |
| ►CIntegState |
1.9.4