voccdb.epn_core: Resource Record Summary

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Resource Record Summary

Specialized Resource (CatalogResource):
Predictions of stellar occultations by the main planetary satellites

Short name: voccdb.epn_core IVOA Identifier: ivo://padc.obspm.planeto/voccdb/q/epn_corePublisher: Paris Astronomical Data Centre More Info: http://voparis-tap-planeto.obspm.fr/tableinfo/voccdb.epn_core VO Compliance: Level 2: This is a VO-compliant resource.	Status: active Registered: 2024 Jan 08 09:34:20Z
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Description

The VOccDB database provides prediction and parameters of stellar occultations by the main planetary satellites. Observations of a stellar occultations help to better determine the size and the shape of the occulting body, as well as its astrometric position at the milli-arcsecond level precision. Only the main moons of giant planets Jupiter, Saturn, Uranus and Neptune are considered in the event prediction database. Predictions are provided over period 2023-2032, up to visual magnitude 12 for the biggest satellites, and magnitude 14 for other satellites. For each stellar occultation event prediction, the database provides circumstances and observational data, date and timing of the occultation, star position and magnitude, excepted duration, etc.

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About the Resource Providers

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Status of This Resource

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What This Resource is About

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Available Service Interfaces

[+]	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://voparis-tap-planeto.obspm.fr/tapX(version 1.1 compatible)

Developed with the support of the National Science Foundation
under Cooperative Agreement AST0122449 with the Johns Hopkins University
The NAVO project is a member of the International Virtual Observatory Alliance

This NAVO Application is hosted by the Space Telescope Science Institute

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