def query(self, coords, **kwargs):
        """
        Returns E(B-V) (or a different Planck dust inference, depending on how
        the class was intialized) at the specified location(s) on the sky.

        Args:
            coords (:obj:`astropy.coordinates.SkyCoord`): The coordinates to query.

        Returns:
            A float array of the selected Planck component, at the given
            coordinates. The shape of the output is the same as the shape of the
            coordinates stored by ``coords``. If extragalactic E(B-V), tau_353
            or radiance was chosen, then the output has units of magnitudes of
            E(B-V). If the selected Planck component is temperature (or
            temperature error), then an :obj:`astropy.Quantity` is returned, with
            units of Kelvin. If beta (or beta error) was chosen, then the output
            is unitless.
        """
        return self._scale * super(PlanckQuery, self).query(coords, **kwargs)
def query ( self , coords , ** kwargs ) : return self . _scale * super ( PlanckQuery , self ) . query ( coords , ** kwargs )
Returns E(B-V) (or a different Planck dust inference, depending on how
        the class was intialized) at the specified location(s) on the sky.

        Args:
            coords (:obj:`astropy.coordinates.SkyCoord`): The coordinates to query.

        Returns:
            A float array of the selected Planck component, at the given
            coordinates. The shape of the output is the same as the shape of the
            coordinates stored by ``coords``. If extragalactic E(B-V), tau_353
            or radiance was chosen, then the output has units of magnitudes of
            E(B-V). If the selected Planck component is temperature (or
            temperature error), then an :obj:`astropy.Quantity` is returned, with
            units of Kelvin. If beta (or beta error) was chosen, then the output
            is unitless.