ESBO-ETC/esbo_etc/classes/target/BlackBodyTarget.py

from ..target.ATarget import ATarget
from ..SpectralQty import SpectralQty
import astropy.units as u
from astropy.modeling.models import BlackBody
from ...lib.logger import logger
from ..Entry import Entry
from typing import Union


class BlackBodyTarget(ATarget):
    """
    This class models the spectral flux density of a star of given magnitude using as black body radiator
    """
    # Bands from Handbook of Space Astronomy and Astrophysics p. 139
    _band = dict(U=dict(wl=365 * u.nm, sfd=4.27e-11 * u.W / (u.m ** 2 * u.nm)),
                 B=dict(wl=440 * u.nm, sfd=6.61e-11 * u.W / (u.m ** 2 * u.nm)),
                 V=dict(wl=550 * u.nm, sfd=3.64e-11 * u.W / (u.m ** 2 * u.nm)),
                 R=dict(wl=700 * u.nm, sfd=1.74e-11 * u.W / (u.m ** 2 * u.nm)),
                 I=dict(wl=900 * u.nm, sfd=8.32e-12 * u.W / (u.m ** 2 * u.nm)),
                 J=dict(wl=1250 * u.nm, sfd=3.18e-12 * u.W / (u.m ** 2 * u.nm)),
                 H=dict(wl=1650 * u.nm, sfd=1.18e-12 * u.W / (u.m ** 2 * u.nm)),
                 K=dict(wl=2200 * u.nm, sfd=4.17e-13 * u.W / (u.m ** 2 * u.nm)),
                 L=dict(wl=3600 * u.nm, sfd=4.17e-13 * u.W / (u.m ** 2 * u.nm)),
                 M=dict(wl=4800 * u.nm, sfd=4.17e-13 * u.W / (u.m ** 2 * u.nm)),
                 N=dict(wl=10200 * u.nm, sfd=4.17e-13 * u.W / (u.m ** 2 * u.nm)))

    @u.quantity_input(wl_bins='length', temp=[u.Kelvin, u.Celsius], mag=u.mag)
    def __init__(self, wl_bins: u.Quantity, temp: u.Quantity = 5778 * u.K,
                 mag: u.Quantity = 0 * u.mag, band: str = "V", size: str = "Point"):
        """
        Initialize a new black body point source

        Parameters
        ----------
        wl_bins : length-Quantity
            Wavelengths used for binning
        temp : Quantity in Kelvin / Celsius
            Temperature of the black body
        mag : Quantity in mag
            Desired apparent magnitude of the point source
        band : str
            Band used for fitting the planck curve to a star of 0th magnitude. Can be one of [U, B, V, R, I, J, H, K].
        size : str
            The size of the target. Can be either point or extended

        Returns
        -------
        """
        if band.upper() not in self._band.keys():
            logger.error("Band has to be one of '[" + ", ".join(list(self._band.keys())) + "]'")
        # Create blackbody model with given temperature
        bb = BlackBody(temperature=temp, scale=1 * u.W / (u.m ** 2 * u.nm * u.sr))

        # Calculate the correction factor for a star of 0th magnitude using the spectral flux density
        # for the central wavelength of the given band
        factor = self._band[band.upper()]["sfd"] / (bb(self._band[band.upper()]["wl"]) * u.sr) * u.sr
        # Calculate spectral flux density for the given wavelengths and scale it for a star of the given magnitude
        sfd = bb(wl_bins) * factor * 10 ** (- 2 / 5 * mag / u.mag)

        # Initialize super class
        super().__init__(SpectralQty(wl_bins, sfd), wl_bins, size)

    @staticmethod
    def check_config(conf: Entry) -> Union[None, str]:
        """
        Check the configuration for this class

        Parameters
        ----------
        conf : Entry
            The configuration entry to be checked.

        Returns
        -------
        mes : Union[None, str]
            The error message of the check. This will be None if the check was successful.
        """
        mes = conf.check_quantity("temp", u.K)
        if mes is not None:
            return mes
        mes = conf.check_quantity("mag", u.mag)
        if mes is not None:
            return mes
        mes = conf.check_selection("band", ["U", "B", "V", "R", "I", "J", "H", "K", "L", "M", "N"])
        if mes is not None:
            return mes
        mes = conf.check_selection("size", ["point", "extended"])
        if mes is not None:
            return mes