J/A+A/422/1109: Resource Record Summary

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Resource Record Summary

Catalog Service:
SnII Lifetimes and oscillator strengths

Short name: J/A+A/422/1109 IVOA Identifier: ivo://CDS.VizieR/J/A+A/422/1109 DOI (Digital Object Identifier): 10.26093/cds/vizier.34221109 Publisher: CDSivo://CDS[Pub. ID] More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/422/1109 VO Compliance: Level 2: This is a VO-compliant resource.	Status: active Registered: 2004 Sep 12 17:13:24Z
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Description

Oscillator strengths calculated for 101 lines of Sn II arising from auto-ionized levels are displayed in column three of Table A1, while columns one and two give the transitions and corresponding wavelengths, respectively. In the second column of Table A2, we present the radiative lifetimes calculated for 13 levels of Sn II. Two levels correspond to 5s2 4f 2F5/2 5s2 4f 2F7/2 for both theoretical and experimental values obtained by other authors. In the other columns of Table 2 we present these values. A good agreement exists between our work and the experimental values. The eleven remaining values correspond to the levels labeled by Moore as 1{deg} at 11{deg} and whose identification is based on the IC 5p3-5s5p5d-5s5p6s.

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About the Resource Providers

This section describes who is responsible for this resource

Publisher: CDSivo://CDS[Pub. ID]

Creators:

Colon C.Alonso Medina A.

Contact Information:

X CDS support team
Email: cds-question at unistra.fr
Address: CDS
Observatoire de Strasbourg
11 rue de l'Universite
F-67000 Strasbourg
France

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 service provides only public data.

Relevant dates for this Resource:

Updated: 2004 Sep 12 17:14:12Z
Created: 2004 Sep 12 17:13:24Z

This resource was registered on: 2004 Sep 12 17:13:24Z
This resource description was last updated on: 2021 Oct 21 00:00:00Z

What This Resource is About

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

Resource Class: CatalogService: This resource is a service that provides access to catalog data. You can extract data from the catalog by issuing a query, and the matching data is returned as a table.

Resource type keywords: Catalog	Subject keywords: Atomic physics
Intended audience or use: Research: This resource provides information appropriate for supporting scientific research.
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/422/1109	Literature Reference: 2004A&A...422.1109C
Related Resources: Other Related Resources TAP VizieR generic service(IsServedBy) ivo://CDS.VizieR/TAP [Res. ID]

	Data Coverage Information
	This section describes the data's coverage over the sky, frequency, and time.

	Rights and Usage Information
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Available Service Interfaces

	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://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/422/1109

	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: URL-based interface: http://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/422/1109

	Table Access Protocol - Auxiliary ServiceXX
	This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data. VO Compliance: Level 2: This is a VO-compliant resource. Available endpoints for the standard interface: http://tapvizier.cds.unistra.fr/TAPVizieR/tap

Developed with the support of the National Science Foundation
under Cooperative Agreement AST0122449 with the Johns Hopkins University
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This NAVO Application is hosted by the Space Telescope Science Institute

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