fluxcompensator.utils.pseudo.Pseudo

class fluxcompensator.utils.pseudo.Pseudo(wav, val, origin=None, units=None, distance=None, x_min=None, x_max=None, y_min=None, y_max=None, lon_min=None, lon_max=None, lat_min=None, lat_max=None, pix_area_sr=None, ap_min=None, ap_max=None)

Mimics the properties of an ModelOutput array.

Parameters:

wav : numpy.ndarray

  • SyntheticCube like: The 1D wavelength of val cube in microns.
  • SyntheticImage like: The 0D wavelength of val image in microns.
  • SyntheticSED like: The 1D wavelengths of val vector in microns.
  • SyntheticFlux like: The 0D wavelength of val scalar in microns.

val : numpy.ndarray

  • SyntheticCube like: The 3D array cube with shape (x, y, wav).
  • SyntheticImage like: The 2D array image with shape (x, y).
  • SyntheticSED like: The 1D array vector with shape like wav.
  • SyntheticFlux like: The 0D array scalar with shape like wav.

units : str

Unit of val array at input. Valid options are:

  • 'ergs/cm^2/s'
  • 'ergs/cm^2/s/Hz'
  • 'Jy'
  • 'mJy'
  • 'MJy/sr' (not for SyntheticSED)

distance : str

Distance to the observed object in cm.

x_min : float

Physical offset from axis origin in FOV in cm.

x_max : float

Physical offset from axis origin in FOV in cm.

y_min : float

Physical offset from axis origin in FOV in cm.

y_max : float

Physical offset from axis origin in FOV in cm.

lon_min : float

Minimal longitudinal angle.

lon_max : float

Maximal longitudinal angle.

lat_min : float

Minimal latitudinal angle.

lat_max : float

Maximal latitudinal angle.

pix_area_sr : float

Pixel area per sr.

ap_min : float

Minimal aperture of the telescope. Default is None.

ap_max : float

Maximal aperture of the telescope. Default is None.
Returns:

cube : Pseudo like ModelOutput 3D

3D val array with ModelOutput properties.

sed : Pseudo like ModelOutput 1D

1D val array with ModelOutput properties.