Gnomonic view

cosmoglobe.plot.gnomonic.gnom(input, lon=0, lat=0, comp=None, sig=0, freq=None, nside=None, size=20, sample=-1, min=None, max=None, ticks=None, rng=None, llabel=None, rlabel=None, unit=None, cmap=None, graticule=False, norm=None, cbar=True, cbar_pad=0.0, cbar_shrink=1, fwhm=<Quantity 0. arcmin>, remove_dip=False, remove_mono=False, fontsize=None, figsize=(3, 4), xsize=1000, darkmode=False, sub=None, hold=False, reuse_axes=False)[source]

Gnomonic view plotting

Parameters

  • input (ndarray, fits file path or cosmoglobe model object) – Map data input given as numpy array either 1d or index given by ‘sig’. Also supports fits-file path string or cosmoglobe model. If cosmoglobe object is passed such as ‘model’, specify comp or freq.

  • lon (float) – Longitude coordinate of the center of the figure in galactic coordinates default: 0

  • lat (float) – Latitude coordinate of the center of the figure in galactic coordinates default: 0

  • sig (str or int, optional) – Specify which signal to plot if ndim>1. default: None

  • comp (string, optional) – Component label for automatic identification of plotting parameters based on information from autoparams.json default: None

  • freq (astropy GHz, optional) – frequency in GHz needed for scaling maps when using a model object input default: None

  • nside (int, optional) – optional ud_grading of the input data default: None

  • size (float, optional) – Size of square in degrees default: 20

  • sample (float, optional) – Specify sample if passing chain default: -1

  • min (float, optional) – Min value default: None

  • max (float, optional) – Max value default: None

  • ticks (list or str, optional) – Ticks for colorbar default: None

  • rng (float, optional) – Sets this value as min and max value. If specified, overwrites autodetector. default: None

  • llabel (str, optional) – Sets the upper left title. Has LaTeX functionaliity (ex. $A_{s}$.) default: None

  • rlabel (str, optional) – Sets the upper right title. Has LaTeX functionaliity (ex. $A_{s}$.) default: None

  • unit (str, optional) – Unit label for colorbar default: None

  • cmap (str, optional) – Colormap (ex. sunburst, planck, jet). Both matplotliib and cmasher available as of now. Also supports qualitative plotly map, [ex. q-Plotly-4 (q for qualitative 4 for max color)] Sets planck as default. default: None

  • graticule (bool) – add graticule default: False

  • norm (str, matplotlib norm object, optional) –

    if norm==’linear’:

    normal

    if norm==’log’:

    Uses log10 scale Normalizes data using a semi-logscale linear between -1 and 1. Autodetector uses this sometimes, you will be warned.

    SPECIFY linthresh for linear threshold of symlog! default: None

  • cbar (bool, optional) – Toggles the colorbar cbar : True

  • cbar_pad (float, optioinal) – default: 0.04

  • cbar_shrink (float, optional) – default: 0.7

  • fwhm (astropy arcmin/rad/deg, optional) – Optional map smoothing. FWHM of gaussian smoothing in arcmin. default: 0.0

  • remove_dip (bool, optional) – If mdmask is specified, fits and removes a dipole. default: True

  • remove_mono (bool, optional) – If mdmask is specified, fits and removes a monopole. default: True

  • fontsize (int, optional) – Size of labels default: None

  • figsize (touple, optional) – size of figure default: None

  • xsize (int, optional) – width of figure in pixels default: 1000

  • darkmode (bool, optional) – turn all axis elements white for optimal dark visualization default: False

  • sub (int, scalar or sequence, optional) – Use only a zone of the current figure (same syntax as subplot). Default: None

  • hold (bool, optional) – If True, replace the current Axes by a MollweideAxes. use this if you want to have multiple maps on the same figure. Default: False

  • reuse_axes (bool, optional) – If True, reuse the current Axes (should be a MollweideAxes). This is useful if you want to overplot with a partially transparent colormap, such as for plotting a line integral convolution. Default: False

  • mask (str path or np.ndarray, optional) – Apply a mask file to data default = None

previous

Sky map

next

Histogram