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    GLAMERDOC++
    
   Gravitational Lensing Code Library 
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A source representing a BLR with a Keplarian disk. More...
#include <source.h>


Public Member Functions | |
| PosType | SurfaceBrightness (const PosType *y) const | 
| PosType | getTotalFlux () const | 
  Public Member Functions inherited from SourceBLR | |
| void | printSource () | 
| virtual PosType | getRadius () const | 
| PosType | getDlDs () const | 
  Public Member Functions inherited from Source | |
| Source (PosType r, Point_2d x, PosType z, PosType SBlimit, PosType zero_point) | |
| shell constructor  | |
| Source (const Source &s) | |
| Source & | operator= (const Source &s) | 
| double | SBlimit_magarcsec (double limit) | 
| convert mag/arcsec^2 to flux units  | |
| PosType | getSBlimit () | 
| Gets sb_limit in erg/cm^2/sec/rad^2/Hz.  | |
| PosType | getSBlimit_magarcsec () | 
| Gets sb_limit in mag/arcsec^2.  | |
| PosType | getZ () const | 
| Redshift of source.  | |
| void | setZ (PosType my_z) | 
| PosType | getRadius () const | 
| Radius of source in radians.  | |
| void | setRadius (PosType my_radius) | 
| Reset the radius of the source in radians.  | |
| Point_2d | getTheta () const | 
| position of source in radians  | |
| void | getTheta (PosType *x) const | 
| position of source in radians  | |
| void | getTheta (Point_2d &x) const | 
| position of source in radians  | |
| void | setTheta (PosType *xx) | 
| Reset the position of the source in radians.  | |
| void | setTheta (PosType my_x, PosType my_y) | 
| void | setTheta (const Point_2d &p) | 
| void | setSBlimit (float limit) | 
| Sets sb_limit in erg/cm^2/sec/rad^2/Hz.  | |
| void | setMagZeroPoint (float zeropoint) | 
| double | getMagZeroPoint () | 
| PosType | changeFilter (std::string filter_in, std::string filter_out, std::string sed) | 
| Calculates the difference in magnitude when changing the observing filter.   | |
| PosType | integrateFilter (std::vector< PosType > wavel_fil, std::vector< PosType > fil) | 
| Calculates the integral of the filter curve given as an array of (x,y) values.  | |
| PosType | integrateFilterSED (std::vector< PosType > wavel_fil, std::vector< PosType > fil, std::vector< PosType > wavel_sed, std::vector< PosType > sed) | 
| Calculates the integral of the sed multiplied by the filter curve.  | |
| double | TEST_surface_brightness (double res, int N) | 
| test if flux in pixels matches total flux  | |
| long | getID () const | 
| void | setID (long i) | 
Additional Inherited Members | |
  Static Public Member Functions inherited from Source | |
| static PosType * | getx (Source &source) | 
  Public Attributes inherited from SourceBLR | |
| PosType | source_tau | 
| lag time  | |
| PosType | source_nu | 
| frequency  | |
| float | source_nuo | 
| float | source_r_in | 
| inner radius of BLR  | |
| float | source_r_out | 
| outer radius of BLR  | |
| float | source_inclination | 
| inclination of BLR in radians, face on is  | |
| float | source_opening_angle | 
| float | source_gamma | 
| float | source_BHmass | 
| float | source_fK | 
| fraction of Keplerian velocity in random motions  | |
| bool | source_monocrome | 
| set to true to integrate over frequency  | |
  Protected Member Functions inherited from Source | |
| double | flux_to_mag (double flux) const | 
  Protected Attributes inherited from Source | |
| PosType | source_r | 
| charactoristic source size  | |
| Point_2d | source_x | 
| center of source  | |
| PosType | zsource | 
| redshift of source  | |
| PosType | sb_limit | 
| long | id | 
| double | mag_zero_point | 
A source representing a BLR with a Keplarian disk.
      
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  inlinevirtual | 
Reimplemented from SourceBLR.
      
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  virtual | 
Surface brightness of source in grid coordinates not source centered coordinates.
The units shuld be ergs / s / Hz / cm^2
Implements Source.