Comments (5)
You're right, that is something that bothered me a couple times in the past and didn't bother to fix. I changed the code to now show proper column names. Please tell me if it's not clear to you what the names mean!
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thanks, I'm going to say
fl_obs
is confusing. I guess this means intrinsic flux right, so dust corrected? because technically observed flux is with dust.
from fastpp.
Also I think there is an issue here (assuming what I said above is correct)
In the top panel, dark blue points should match with the blue plot (intrinsic sed) and the cyan ones should match (observed sed) ( or at least vice versa if the column are jumbled).
before i go any further looking into this have you checked this before?
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Ah, I guess this is even more unclear than I thought it might :) The first column is wavelength, the second column (fl_model
) is the best fit flux, the third column (fl_obs
) is the flux of the galaxy as provided in the input catalog, and the fourth column (unc_obs
) is the uncertainty of that flux. So the last two columns are just repeating data from the input catalog, to make it easier to plot the fit and observations together. I guess I'll have to document that!
NB: there is currently no option to obtain the intrinsic (without dust) broadband fluxes, and I don't think I'll add this in the near future unless you give me a good reason to :P
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aha! got it. Yeah, the latter is not necessary, what is important to see is the photometry comparison between observations and best fit model.
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Related Issues (19)
- Adding new filters HOT 3
- Failed fit comparisons between fastpp FAST HOT 4
- Parameter estimation HOT 5
- Comparison between fastpp and FAST-IDL HOT 5
- download_bc03_ssp.sh vs what is looked for by fastpp HOT 2
- Getting error while running "make install" HOT 3
- Error with make install HOT 9
- FAST++ aborts while running with JWST filters HOT 4
- Question: How to access the scaling factor for the spectra in the grid file? HOT 7
- Higher Sig Figs in Output file HOT 2
- installation issue HOT 12
- custom SFH as a piecewise constant model HOT 6
- Segmentation fault: 11 when using a set of models HOT 6
- Unavailable library ised_exp.pr HOT 3
- computing rest-frame magnitudes HOT 2
- Investigating best-fit SEDs HOT 4
- Considering multiple metallicities HOT 5
- valid dust laws HOT 1
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