Information on Service 'PoWR'
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Further access options are discussed below
Theoretical spectral energy distributions (SEDs) from expanding NLTE
model atmospheres for hot stars.
For a list of all services and tables belonging to this service's
resource, see Information on resource 'PoWR'
Overview
You can access this service using:
-
external --
a renderer with some custom access method that should be mentioned in the service description
This service is published as follows:
- Within the
set(s) ivo_managed with the renderer
external
local means it is listed on our front page,
ivo_managed means
it has a record in the VO registry.
VOResource XML (that's something exclusively for VO nerds)
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