Gyoto
File List
Here is a list of all documented files with brief descriptions:
 Gyoto.hAll of Gyoto
 GyotoAstrobj.hAstronomical objects (light emitters)
 GyotoBlackBodySpectrum.hI_nu(nu, T) = cst_*2*h*nu^3/c^2/(exp(h*nu/k*T)-1.);
 GyotoBlob.hBlob of plasma following a Star orbit, emitting synchrotron, with Gaussian time-evolving density and temperature
 GyotoChernSimons.hChern-Simons 1st order perturbation to KerrBL metric
 GyotoComplexAstrobj.hCombine astronomical objects
 GyotoComplexMetric.h
 GyotoComplexSpectrometer.hCombine spectrometer objects
 GyotoConfig.hCompile-time configuration
 GyotoConverters.hGYOTO converters
 GyotoDeformedTorus.hSlender torus subject to simple time-periodic deformations
 GyotoDefs.hGyoto ubiquitous macros and typedefs
 GyotoDirectionalDisk.hGeometrically thin disk read from FITS file
 GyotoDisk3D.hA geometrically thick, optically thin disk
 GyotoDynamicalDisk.hA geometrically thin, optically thick disk, evolving dynamically
 GyotoDynamicalDisk3D.hA geometrically thick, optically thin disk, evolving dynamically, with black body emission
 GyotoDynamicalDiskBolometric.hA geometrically thin, optically thick disk, evolving dynamically
 GyotoEquatorialHotSpot.hEquatorial hot spot
 GyotoError.hError handling
 GyotoFactory.hXML I/O
 GyotoFactoryMessenger.hFactory / SmartPointee::Subcontractor_t interface
 GyotoFitsRW.hClass to read/write jnu and anu in FITS File
 GyotoFixedStar.hFixed (i.e. non-moving) star
 GyotoFlaredDiskSynchrotron.hA disk defined from a 2D grid in the equatorial plane and extrapolated in the vertical direction with H/r<<1
 GyotoFunctors.hClasses with an operator() method
 GyotoGridData2D.hBase class for reading 2D gridded data
 GyotoHayward.hMetric of a regular rotating black hole or naked worm-hole
 GyotoHooks.hTellers tell Listeners when they mutate
 GyotoInflateStar.hMass-less, spherical object following a timelike geodesic
 GyotoJet.hSimple jet model with thermal or kappa-distribution synchrotron emission from Pandya et al. (2016)
 GyotoKappaDistributionSynchrotronSpectrum.hPowerlaw synchrotron spectrum
 GyotoKerrBL.hKerrBL metric
 GyotoKerrKS.hKerrKS metric
 GyotoMetric.hBase class for metric description
 GyotoMinkowski.hThe Minkowski flat-space metric
 GyotoNeutronStar.hNeutron star defined by its surface ; no emission
 GyotoNeutronStarAnalyticEmission.hNeutron star emitting at its surface an analytic emission, typically blackbody
 GyotoNeutronStarModelAtmosphere.hNeutron star emitting at its surface an analytic emission, typically blackbody
 GyotoNumericalMetricLorene.hBase class for 3+1 numerical metrics computed by LORENE
 GyotoObject.hIntrospectable objects
 GyotoOscilTorus.hSlender torus subject to realistic Blaes 2006 oscillation modes
 GyotoPageThorneDisk.hA geometrically thin, optically thick disk
 GyotoPatternDisk.hA geometrically thin, optically thick disk
 GyotoPatternDiskBB.hA PatternDisk object with possibility to compute a black body spectrum when PatternDiskBB::emission_ does not yield directly Iν but temperature
 GyotoPhoton.hA single light ray
 GyotoPlasmoid.hPlasmoid sphere formed by magnetic reconnection following a Star orbit, emitting synchrotron, with two distributions of electrons: one thermal at "low" temperature and one kappa at "high" temperature
 GyotoPolishDoughnut.hA magnetized toroidal accretion structure
 GyotoPowerLawSpectrum.hA power law spectrum : I_nu=constant_*nu^exponent_
 GyotoPowerLawSynchrotronSpectrum.hPowerlaw synchrotron spectrum
 GyotoProperty.hIntrospectable properties
 GyotoPython.hExtending Gyoto using Python
 GyotoRegister.hGyoto registers
 GyotoRezzollaZhidenko.hSpherically-symmetric parametrized metric of Rezzolla&Zhidenko 2014 See the paper: PRD, 90, 084009 Only epsilon, a0, a1, a2, a3, b0, b1, b2, b3 are allowed non-zero
 GyotoRotStar3_1.hNumerical metric around a rotating star in 3+1 formalism
 GyotoScenery.hRay-tracing framework
 GyotoSchwarzschildHarmonic.hSchwarzschild spacetime in harmonic coordinates
 GyotoScreen.hDescription of the observer screen
 GyotoShift.hShift a metric
 GyotoSmartPointer.hReference-counting pointers
 GyotoSpectrometer.hSpectroscopic capabilities of a Screen
 GyotoSpectrum.hSpectrum of a simple object (e.g. Star)
 GyotoSphericalAccretion.hA spherically-symmetric accretion flow radially falling onto the central object
 GyotoStandardAstrobj.hAstronomical objects defined bya a potential/distance
 GyotoStar.hMass-less, spherical object following a timelike geodesic
 GyotoStarTrace.hLike a Star that would be on all points of its orbit at all time
 GyotoThermalBremsstrahlungSpectrum.hThermal brems spectrum
 GyotoThermalSynchrotronSpectrum.hThermal synchrotron spectrum
 GyotoThickDisk.hA thick accretion disk described by its inner radius and the fwhm of the Gaussian factor affecting the density out of the equatorial plane
 GyotoThinDisk.hGeometrically thin disks and rings
 GyotoThinDiskGridIntensity.hA disk defined from a 2D grid in the equatorial plane and extrapolated in the vertical direction with H/r<<1
 GyotoThinDiskIronLine.h
 GyotoThinDiskPL.hA subclass of ThinDisk emitting according to a powerlaw
 GyotoThinDiskProfile.hA subclass of ThinDisk emitting according to some specified profile that should be hardcoded in emission()
 GyotoTorus.hA simple torus
 GyotoUniformSpectrometer.hUniformly spaced spectrometers
 GyotoUniformSphere.hOptically thick or thin, spherical objects
 GyotoUtils.hGYOTO utilities
 GyotoValue.hIntrospectable value
 GyotoWIP.hWork in progress class
 GyotoWorldline.hTimelike or null geodesics
 GyotoXillverReflection.hThe 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. The metric is imposed to be Kerr for simplicity