relative fluxes
Rob Seaman
seaman at noao.edu
Mon Jun 22 05:48:49 PDT 2009
On Jun 22, 2009, at 4:46 AM, Derriere Sebastien wrote:
> Then it hit me: that's the same as expressing a mass in Solar masses!
> ...
> So thinking of a spectra normalized to a reference, value, the unit
> could be this reference value! With Alberto's example:
> value=[anything from 0.0 to 0.06]
> unit="1.23e-4 erg/cm**2/s/Angstrom" (or whatever the reference value)
This seems like a viable solution - the question is whether this is a
problem that needs solving, its contingent priority, and whether we
yet have a complete description of the problem.
How is this used in the literature? What fraction of columns/values
in VO DBs/images/catalogs require this? Is there a need to support an
offset as well as a scaling factor?
In short, are there domain use cases for this?
> My 2cents
An even better example :-)
Rob
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