You signed in with another tab or window. Reload to refresh your session.You signed out in another tab or window. Reload to refresh your session.You switched accounts on another tab or window. Reload to refresh your session.Dismiss alert
It would be nice to have the built-in functionality to feed in a filter bandpass (wavelength & transmission) and either A_V or E(B-V) to get the total extinction for a given extinction law.
The situation that made me think of this: going from E(B-V) of galactic foreground to the extinction in each of my filters.
The text was updated successfully, but these errors were encountered:
One complication, the effective extinction in a filter depends on the spectrum of the star. But I agree, still would be useful.
Of course, right now all the extinction curves in the optical/NIR are based on filter photometry to derive the extinction curves. So, just getting the extinction at the nominal filter wavelength will give you what you want. This will change in the near future for the optical with new work (Fitzpatrick, Massa, Gordon, in prep). And hopefully in the NIR and MIR soon too (Gordon et al. in prep). Just gotta get the work done. :-)
It would be nice to have the built-in functionality to feed in a filter bandpass (wavelength & transmission) and either A_V or E(B-V) to get the total extinction for a given extinction law.
The situation that made me think of this: going from E(B-V) of galactic foreground to the extinction in each of my filters.
The text was updated successfully, but these errors were encountered: