PoWR: Resource Record Summary

Resource Record Summary

Data Service:
PoWR

Short name: PoWR IVOA Identifier: ivo://org.gavo.dc/gvo/data/PoWR/powr.ipapPublisher: The GAVO DC team More Info: http://dc.zah.uni-heidelberg.de/gvo/data/PoWR/powr.ipap/info VO Compliance: Level 2: This is a VO-compliant resource.	Status: active Registered: 2013 Mar 14 13:25:52Z
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Description

Theoretical spectral energy distributions (SEDs) from expanding NLTE model atmospheres for hot stars.

About the Resource Providers

This section describes who is responsible for this resource

Publisher: The GAVO DC team

Creator: Wolf-Rainer Hamann

Contact Information:

X GAVO Data Center Team
Email: gavo at ari.uni-heidelberg.de
Address: Mönchhofstrasse 12-14
D-69120 Heidelberg

Status of This Resource

This section provides some status information: the resource version, availability, and relevant dates.

Version: n/a
Availability: This is an active resource.

This resource was registered on: 2013 Mar 14 13:25:52Z
This resource description was last updated on: 2022 Mar 23 13:13:05Z

What This Resource is About

This section describes what the resource is, what it contains, and how it might be relevant.

Resource Class: DataService: This resource is a service that provides access to data.

Resource type keywords: Simulation	Subject keywords: stellar-atmospheres radiative-transfer
Intended audience or use: University: This resource provides information appropriate for use in university education. Research: This resource provides information appropriate for supporting scientific research.
More Info: http://dc.zah.uni-heidelberg.de/gvo/data/PoWR/powr.ipap/info

	Custom Service
	This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource. VO Compliance: Level 2: This is a VO-compliant resource. Available endpoints for this service interface: Interactive web page: http://www.astro.physik.uni-potsdam.de/~PoWR