Loading...
Searching...
No Matches
Class List
Here are the classes, structs, unions and interfaces with brief descriptions:
[detail level 123]
| ►NISOP | ISOP namespace is for functions related to isoparametric interpolation |
| ►NUtilities | |
| CBandInfo | Class that contains information about bands |
| CBeam | A simplified data structure for use in interface with other codes |
| CBranch | The box representing a branch of a binary tree structure. Used specifically in TreeStruct for organizing points in the grid |
| CBranchNB | Box representing a branch in a tree. It has four children. Used in TreeNBStruct which is used in TreeForce |
| CCOSMOLOGY | The cosmology and all the functions required to calculated quantities based on the cosmology |
| CCPFITS_READ | Read only fits file interface |
| CCPFITS_READ_TABLES | Read only fits file interface |
| CElliptic | Class to convert isotropic LensHalos into elliptical halos |
| CGrid | Structure to contain both source and image trees |
| CGridMap | A simplified version of the Grid structure for making non-adaptive maps of the lensing quantities (kappa, gamma, etc...) |
| CHALOCalculator | Class for calculating the properties of NFW dark matter halos at a specified redshift and mass |
| CImageInfo | Structure for storing information about images or curves |
| CInputParams | Structure for reading and writing parameters to and from a parameter file as well as a container for passing the parameters to other classes and functions |
| CKistUnit | Internal container used in Kist container class |
| CLens | A class to represents a lens with multiple planes |
| CLensHalo | A base class for all types of lensing "halos" which are any mass distribution that cause lensing |
| CLensHaloAnaNSIE | A NSIE lens with distortions in shape, substructures and stars included |
| CLensHaloDisk | Creates a exponential disk out of particles |
| CLensHaloDummy | This is a lens that does no lensing. It is useful for testing and for running refinement code on sources |
| CLensHaloFit | LensHalo class primarily used for fitting point source lenses |
| CLensHaloMassMap | A class that includes the MOKA lens map |
| CLensHaloMultiMap | A lens halo that calculates all lensing quantities on two grids - a low res long range grid and a high res short range grid. This is done to reduce the required memory required |
| CLensHaloNFW | A class for calculating the deflection, kappa and gamma caused by an NFW halos |
| CLensHaloParticles | A class that represents the lensing by a collection of simulation particles |
| CLensHaloPowerLaw | A class for calculating the deflection, kappa and gamma caused by a collection of halos with truncated power-law mass profiles |
| CLensHaloPseudoNFW | A class for calculating the deflection, kappa and gamma caused by a collection of halos with a double power-law mass profile |
| CLensHaloRealNSIE | Represents a non-singular isothermal elliptical lens |
| CLensHaloTEPL | A truncated elliptical power-law profile |
| CLensHaloTNSIE | Truncated non-singular isothermal ellipsoid |
| CLensHaloUniform | A uniform surface density and shear lens |
| CLensMap | The MOKA map structure, containing all quantities that define it |
| CLensPlane | Base class representing a plane in redshift onto which lenses are placed |
| CLensPlaneSingular | A LensPlane with a list of LensHalo's in it |
| CLensPlaneTree | A LensPlane with a TreeQuad on it to calculate the deflection caused by field lenses |
| CLinkedPoint | A point that automatically has an image point |
| CMakeParticleLenses | A class for constructing LensHalos from particles in a data file |
| CMemmoryBank | |
| CMOKAmap | The MOKA map structure, containing all quantities that define it |
| CMultiGridSmoother | Warning: Not tested yet. Class for doing adaptive smoothing using multiply resolution grids |
| CNFW_Utility | Class for calculating properties of NFW halo profile |
| CObservation | It creates a realistic image from the output of a ray-tracing simulation |
| CObsVIS | It creates a realistic image from the output of a ray-tracing simulation |
| COldImageInfo | This is an old version that should not be used anymore in favor of ImageInfo |
| CParticleType2D | Atomic data class for simulation particles of the same size and mass |
| CParticleTypeSimple | Atomic data class for simulation particles of the same size and mass |
| CPixelMap | Image structure that can be manipulated and exported to/from fits files |
| CPoint | A point on the source or image plane that contains a position and the lensing quantities |
| CPoint_2d | Class for representing points or vectors in 2 dimensions. Not that the dereferencing operator is overridden |
| CPoint_3d | Class for representing points or vectors in 3 dimensions. Not that the dereferencing operator is overridden |
| CPoint_nd | |
| CPointList | Link list for points, uses the linking pointers within the Point type unlike Kist |
| CPolar | This data class represents a postion inspherical coordinates and a polarization relative to the sphircal coordinate system |
| CQBiterator | A iterator class fore TreeStruct that allows for movement through the tree without changing anything in the tree itself |
| CQBranchNB | Box representing a branch in a tree. It has four children. Used in QTreeNB which is used in TreeQuad |
| CQTreeNB | QTreeNB: Tree structure used for force calculation with particles (i.e. stars, Nbody or halos) |
| CQuasarLF | Pointer to surface brightness function |
| CRAY | Simple representaion of a light path giving position on the image and source planes and lensing quantities |
| Csimple_analytic_lens | A simplified version of LensHaloAnaNSIE |
| CSlicer | |
| CSource | Base class for all sources |
| CSourceBLR | Base class for all sources representing the Broad Line Region (BLR) of a AGN/QSO |
| CSourceBLRDisk | A source representing a BLR with a Keplarian disk |
| CSourceBLRSph1 | A source representing a BLR with a spherical symmetry and circular orbits |
| CSourceBLRSph2 | A source representing a BLR with a spherical symmetry and random velocity dispersion |
| CSourceFunctor | Functor to turn sources into binary functions |
| CSourceMultiAnaGalaxy | Source that represents an analytic galaxy surface brightness model. It encapsulates a OverzierSource which is a model from R.Overzier et al. 2012 with a bulge and a disk |
| CSourceMultiShapelets | Class for reading in and handling an array of SourceShapelets, made on the model of SourceMultiAnaGalaxy Galaxies are read from files in a predifined directory and put into a std::vector that allows sorting in redshift and magnitude. An individual object can be get via CurrentGalaxy() or the overloaded operator [] |
| CSourceOverzier | Structure for holding parameters for one or more galaxy images according to the Overzier model |
| CSourceOverzierPlus | Adds some extra features to the SourceOverzier source like spiral arms, and randomizations |
| CSourcePixelled | Class for sources described by an array of pixels |
| CSourcePoint | A uniform surface brightness circular source |
| CSourceSersic | Class for sources described by a Sersic profile |
| CSourceShapelets | Class for sources described by shapelets |
| CSourceUniform | A uniform surface brightness circular source |
| CStarType | Atomic data class for stars with different masses |
| CSunInfo | Class that contains information about the solar SED and magnitudes |
| CTreeForce | Object used to calculate the force or deflection caused by a collection of "particles" by the tree method |
| CTreeNBStruct | TreeNBStruct: Tree structure used for force calculation with particles (i.e. stars, Nbody or halos) |
| CTreeQuadParticles | TreeQuadParticles is a class for calculating the deflection, kappa and gamma by tree method |
| CTreeSimple | A C++ class wrapper for the bianary treeNB used in the Nbody force calculation, but also useful for general purpose searches |
| ►CTreeSimpleVec | A tree for doing quick searches in multidimensional space. A pointer to an array of objects type T is provided. If they are in a vector, vector.data() can be put in the constructor. The order of objects in the array is not changed. If Mypos is not specified the method D * T::x() must exist. It is this coordinate that is used for the object's position. Another definition for the position of and object can made by specifying Mypos |
| ►CTreeStruct | Tree: Exported struct |
Generated on Fri Apr 18 2025 13:05:57 for GLAMERDOC++ by
1.13.2