Content Level: General / Validation Level: 2 - STScI NAVO Directory Search Results

ID:: ivo://pds-ppi/vex_aspera4_els_derived/ppi/epn_core
Title:: VEx ASPERA-4 ELS Background Derived Data Collection
Short Name:: vex_aspera4_els_
Date:: 25 Apr 2025 01:59:18
Publisher:: Planetary Data System
Description:: This collection contains the derived data products for the Venus Express Electron Spectrometer Background Data Bundle.

ID:: ivo://pds-ppi/vex_aspera4_els_eng/ppi/epn_core
Title:: VEx ASPERA-4 ELS Background Engineering Data Collection
Short Name:: VEX-ASPERA4-ENG
Date:: 15 Dec 2022 19:26:13
Publisher:: Planetary Data System
Description:: This collection contains the engineering data for the Venus Express Electron Spectrometer Background Data Bundle.

ID:: ivo://pds-ppi/vex_aspera4_els_raw/ppi/epn_core
Title:: VEx ASPERA-4 ELS Background Raw Data Collection
Short Name:: vex_aspera4_els_
Date:: 25 Apr 2025 02:02:07
Publisher:: Planetary Data System
Description:: This collection contains the raw data products for the Venus Express Electron Spectrometer Background Data Bundle.

ID:: ivo://padc.obspm.planeto/meteor_showers/q/epn_core
Title:: VOEvent meteor shower service
Short Name:: Meteor Showers
Date:: 16 Jul 2024 13:55:03
Publisher:: Paris Astronomical Data Centre
Description:: The ephemeris were produced by simulating the ejection of meteoroids from the sunlit hemisphere of cometary nuclei, typically from 0 to 3 au, followed by the propagation of orbits of meteoroids in the Solar System, taking into account the gravity of the Sun, the 8 planets, Pluto, and the Moon, as well as the radiation pressure and the Poynting-Robertson drag. Note that asteroid parent bodies were considered as active (i.e. comet-like bodies) even if they are not active today. The showers are predicted when a planet enters a large enough set of meteoroids, at a distance less than typically 0.01 au. See Vaubaillon J., Colas F., Jorda L. 2005 A new method to predict meteor showers. I. Description of the model, Astronomy and Astrophysics, Volume 439/2 p.751-760, as well as: Vaubaillon J. 2017 A confidence index for forecasting of meteor showers, Planetary and Space Science, Volume 143 p.78-82

ID:: ivo://vopdc
Title:: VO-Paris Data Center Naming Authority
Short Name:: PADC Authority
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre
Description:: This naming authority is the root of the naming of the resources from VO-Paris Data Center and partners

ID:: ivo://vopdc/registry
Title:: VO-Paris Data Center Publishing Registry
Short Name:: PADC Registry
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre
Description:: This registry provides access to resources from VO-Paris Data Center and partners.

ID:: ivo://vopdc.obspm/portal
Title:: VO-Paris Data Discovery Portal
Short Name:: PADC Portal
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre
Description:: The Paris Astronomical Data Centre Portal provides an easy way to access to all VO data available at Paris Observatory.

ID:: ivo://vopdc.obspm/gepi/vopsat
Title:: VO Paris Southern Atlas
Short Name:: VOPSAT
Date:: 10 Jan 2017
Publisher:: Paris Astronomical Data Centre - GEPI
Description:: VOPSAT is a set of southern sky digital surveys based on ESO-R, SRC-J and POSS1-E atlases. The plates have been digitized with the MAMA microdensitometer with a resolution of 0.7 arc-sec. Pixel resampling will allow mosaicing neighbouring Schmidt fields up to hundreds of square degrees.

ID:: ivo://vopdc.obspm/imcce/miriade
Title:: VO Solar System Object Ephemeris Generator
Short Name:: Miriade
Date:: 03 Feb 2017
Publisher:: Paris Astronomical Data Centre - IMCCE
Description:: The Miriade project aims to provide a VO-compliant suite of services to compute positional and physical ephemerides of known solar system bodies as seen from any location on Earth as well as various location in space (HST, SPITZER, Gaia, etc.)

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