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Extend photometric system

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This commit is contained in:
Lukas Klass 2020-04-22 11:01:33 +02:00
parent c2a7f97ec4
commit cec9c7930a
2 changed files with 17 additions and 14 deletions
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10
esbo_etc/classes/optical_component/Filter.py
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@ -11,10 +11,12 @@ class Filter(AHotOpticalComponent):
A class to model a filter component and its thermal emission. The model can be created from a file, the name of
a band or a custom spectral range.
"""
_band = dict(U=dict(cwl=366 * u.nm, bw=68 * u.nm), B=dict(cwl=438 * u.nm, bw=98 * u.nm),
V=dict(cwl=545 * u.nm, bw=89 * u.nm), R=dict(cwl=641 * u.nm, bw=220 * u.nm),
I=dict(cwl=798 * u.nm, bw=240 * u.nm), J=dict(cwl=1220 * u.nm, bw=300 * u.nm),
H=dict(cwl=1630 * u.nm, bw=400 * u.nm), K=dict(cwl=2190 * u.nm, bw=600 * u.nm))
_band = dict(U=dict(cwl=365 * u.nm, bw=68 * u.nm), B=dict(cwl=440 * u.nm, bw=98 * u.nm),
V=dict(cwl=550 * u.nm, bw=89 * u.nm), R=dict(cwl=700 * u.nm, bw=220 * u.nm),
I=dict(cwl=900 * u.nm, bw=240 * u.nm), J=dict(cwl=1250 * u.nm, bw=300 * u.nm),
H=dict(cwl=1650 * u.nm, bw=400 * u.nm), K=dict(cwl=2200 * u.nm, bw=600 * u.nm),
L=dict(cwl=3600 * u.nm, bw=1200 * u.nm), M=dict(cwl=4800 * u.nm, bw=800 * u.nm),
N=dict(cwl=10200 * u.nm, bw=2500 * u.nm))
@u.quantity_input(temp=[u.Kelvin, u.Celsius], obstructor_temp=[u.Kelvin, u.Celsius])
def __init__(self, parent: IRadiant, transmittance: Union[SpectralQty, Callable[[u.Quantity], u.Quantity]],

21
esbo_etc/classes/target/BlackBodyTarget.py
View File

@ -10,16 +10,17 @@ 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
# band_sfd = {"U": 1790*u.Jansky, "B": 4063*u.Jansky, "V": 3636*u.Jansky, "R": 3064*u.Jansky,
# "I": 2416*u.Jansky, "J": 1590*u.Jansky, "H": 1020*u.Jansky, "K": 640*u.Jansky}
_band = dict(U=dict(wl=366 * u.nm, sfd=4.175e-11 * u.W / (u.m ** 2 * u.nm)),
B=dict(wl=438 * u.nm, sfd=6.32e-11 * u.W / (u.m ** 2 * u.nm)),
V=dict(wl=545 * u.nm, sfd=3.631e-11 * u.W / (u.m ** 2 * u.nm)),
R=dict(wl=641 * u.nm, sfd=2.177e-11 * u.W / (u.m ** 2 * u.nm)),
I=dict(wl=798 * u.nm, sfd=1.126e-11 * u.W / (u.m ** 2 * u.nm)),
J=dict(wl=1220 * u.nm, sfd=3.15e-12 * u.W / (u.m ** 2 * u.nm)),
H=dict(wl=1630 * u.nm, sfd=1.14e-12 * u.W / (u.m ** 2 * u.nm)),
K=dict(wl=2190 * u.nm, sfd=3.96e-13 * u.W / (u.m ** 2 * u.nm)))
_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,