Photometric system extended

This commit is contained in:
Lukas Klass 2020-04-22 11:02:32 +02:00
parent cec9c7930a
commit f0cba7ee92
2 changed files with 2 additions and 1 deletions

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@ -11,6 +11,7 @@ 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 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. a band or a custom spectral range.
""" """
# Bands from Handbook of Space Astronomy and Astrophysics p. 139
_band = dict(U=dict(cwl=365 * u.nm, bw=68 * u.nm), B=dict(cwl=440 * u.nm, bw=98 * 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), 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), I=dict(cwl=900 * u.nm, bw=240 * u.nm), J=dict(cwl=1250 * u.nm, bw=300 * u.nm),

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@ -9,7 +9,7 @@ class BlackBodyTarget(ATarget):
""" """
This class models the spectral flux density of a star of given magnitude using as black body radiator 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 # 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)), _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)), 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)), V=dict(wl=550 * u.nm, sfd=3.64e-11 * u.W / (u.m ** 2 * u.nm)),