PADC TAP Server on voparis-tap-planeto.obspm.fr Public Tables

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Matched: 25

TablenameInfoTable desc.Res desc.
apis.epn_coreTable InfoEpnCore table for APIS service Planetary aurorae are powerful emissions radiated from auroral regions of magnetized planets by accelerated charged particles, in a wide range of wavelengths (from radio to X-rays). The UV range in particular is adequate to measure collisionaly excited transitions of H and H2, the dominant species in the upper atmosphere of giant planets, produced by precipitating auroral particles, and benefits a good angular resolution. Auroral UV observations therefore provide a rich source of informations on planetary atmospheres and magnetospheres. They also offer a unique diagnostic to remotely probe the solar wind activity throughout the heliosphere.
basecom.epn_coreTable InfoN/A Since 1973, the 18-cm lines of the OH radical have been systematically observed in a number of comets with the Nançay radio telescope. This allowed an evaluation of the cometary water production rates and their evolution with time, as well as a study of several physical processes: the excitation mechanisms of the OH radio lines, the expansion of the cometary atmospheres, their anisotropy in relation with non-gravitational forces, the Zeeman effect in relation with the cometary magnetic field. The Nançay observations of 53 cometary apparitions between 1982 and 2009 are now organized in this database.
bdip.epn_coreTable InfoPlanetary Images Database One Century of Planetary Images ------------------------------- The database of planetary images (BDIP) comes from the digitization of photographs collected and preserved by the Center for Photographic Documentation of the planets held by the IAU at the Meudon Observatory in 1961 under the the curation of J.H. Focas (IAUC, 12th General Assembly, Report 1964). A similar center was established at the Lowell Observatory in Arizona, under the responsibility of W.A. Baum. The photographs were duplicated between the two centers. Approximately 8400 photographs of Mars, Venus, Mercury, Jupiter and Saturn, acquired between 1890 and 1977, are kept at LESIA. They remain available for research on justified request. The digitization of these planetary photographs was performed by scanning between 1998 and 2000 by the staff of the Documentation Center (R. Boyer, E. Neyvoz et al), in the framework of a project proposed to the Scientific Council of the Paris Observatory by P. Drossart. Care was taken to preserve the best possible definition and photometric linearity of photographs during the scanning procedure. Storage was done using different image formats (JPEG, GIF and TIFF ie, lossy, lossless and uncompressed). Improved techniques for mass storage and network distribution today allow us to provide access to the highest definition images, thereby facilitating research on the evolution of planets, at asecular time scale. Scientific interest ------------------- The scientific interest of the photographic database mainly concerns planetary atmospheric evolution of Mars, Jupiter, Saturn and Venus. The evolution of the Martian storms, or the polar caps on Mars, the survey of storms observed on Saturn, or features like the Great Red Spot of Jupiter or oval white spots are among the subjects which triggered on photographs. Such studies can be refined today thanks to digital pictures (Sanchez-Lavega and Battaner, A and A Suppl. Ser., 64, 287, 1986). Some images of Mercury are also available.
bdip.observatoriesTable InfoObservatory names One Century of Planetary Images ------------------------------- The database of planetary images (BDIP) comes from the digitization of photographs collected and preserved by the Center for Photographic Documentation of the planets held by the IAU at the Meudon Observatory in 1961 under the the curation of J.H. Focas (IAUC, 12th General Assembly, Report 1964). A similar center was established at the Lowell Observatory in Arizona, under the responsibility of W.A. Baum. The photographs were duplicated between the two centers. Approximately 8400 photographs of Mars, Venus, Mercury, Jupiter and Saturn, acquired between 1890 and 1977, are kept at LESIA. They remain available for research on justified request. The digitization of these planetary photographs was performed by scanning between 1998 and 2000 by the staff of the Documentation Center (R. Boyer, E. Neyvoz et al), in the framework of a project proposed to the Scientific Council of the Paris Observatory by P. Drossart. Care was taken to preserve the best possible definition and photometric linearity of photographs during the scanning procedure. Storage was done using different image formats (JPEG, GIF and TIFF ie, lossy, lossless and uncompressed). Improved techniques for mass storage and network distribution today allow us to provide access to the highest definition images, thereby facilitating research on the evolution of planets, at asecular time scale. Scientific interest ------------------- The scientific interest of the photographic database mainly concerns planetary atmospheric evolution of Mars, Jupiter, Saturn and Venus. The evolution of the Martian storms, or the polar caps on Mars, the survey of storms observed on Saturn, or features like the Great Red Spot of Jupiter or oval white spots are among the subjects which triggered on photographs. Such studies can be refined today thanks to digital pictures (Sanchez-Lavega and Battaner, A and A Suppl. Ser., 64, 287, 1986). Some images of Mercury are also available.
crism_speclib.epn_coreTable InfoN/A This service provides access to the spectral library in support of the CRISM experiment on Mars Reconnaissance Orbiter. This is a redesigned version of the library once distributed by the PDS Geosciences node, with data files provided as VOTable (the native version was available at: http://pds-geosciences.wustl.edu/mro/mro-m-crism-4-speclib-v1/mrocr_90xx/ Reference: Murchie et al (2007) Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on Mars Reconnaissance Orbiter (MRO). JGR Planets, 112:E05S03
dynastvo.epn_coreTable InfoN/AThis database displays calculated orbital parameters for small bodies
exoplanet.epn_coreTable InfoEncyclopedia of extrasolar planetEncyclopedia of extrasolar planet
hst_planeto.epn_coreTable InfoN/A HST observations of planets, dwarf planets, and satellites, extracted from the CADC database catalogue (with daily updates). Data are linked to the CADC repository, with file names common to all HST archives. Both calibrated and derived products are included. The main target is identified. Physical ephemeris and thumbnails are provided when available. Files and previews are not accessible during the proprietary period.
iks.epn_coreTable InfoN/A Measurements of comet Halley in the spectral channel of IKS on board the Vega-1 spacecraft. Data are retrieved from the PDS Small Bodies Node data set (2011 reformatted version) and updated. The data set consists in 101 tables providing the radiance spectrum of comet Halley from various distances, plus two composite spectra. For details and further references, see: Combes M. et al., 1988, The 2.5-12 micron Spectrum of Comet Halley from the IKS-VEGA Experiment, Icarus, 76, 404-436 [1988Icar...76..404C]
m4ast.epn_coreTable Infocompiled database for asteroid spectra in the visible and NIR regionscompiled database for asteroid spectra in the visible and NIR regions
meteor_showers.epn_coreTable InfoN/A 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
moonsprop.epn_coreTable InfoN/A This service provides the physical and dynamical characteristics of natural satellites in the Solar System: size, mass, rotational properties, magnitude and albedo, orbital elements. These quantities are taken from various publications listed under the bib_reference parameter. These data will be updated as new values are published.
planets.epn_coreTable InfoN/A Main characteristics of Solar System planets. Data are included in the table, which includes non-standard EPN-TAP parameters. Data are retrieved from Archinal et al 2018 (IAU report 2015, 2018CeMDA.130...22A) [radii] and Cox et al 2000 (Allen's astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric distances, and rotation periods].
spectro_asteroids.epn_coreTable InfoN/A This service provides a compilation of spectra of asteroids in the visible and NIR range. It is composed of various libraries distributed as VizieR catalogues. Reformatted VOtable or fits versions are provided with thumbnails. Ephemeris data are retrieved from Miriade (IMCCE) for the reference date when possible.
spectro_planets.epn_coreTable InfoN/A This service provides a compilation of global spectra of planets and satellites in the visible and NIR range, for quick reference purpose. It is made from various libraries, including the Tohoku-Hiroshima-Nagoya Planet Spectra Library (Lundock et al 2009) and spectra from a USGS web site (R. Clark). Reformatted VOtable versions are provided together with links to the original data.
tap_schema.columnsTable InfoColumns in tables available for ADQL querying. PADC TAP Server on voparis-tap-planeto.obspm.fr's Table Access Protocol (TAP) service with table metadata.
tap_schema.groupsTable InfoColumns that are part of groups within tables available for ADQL querying. PADC TAP Server on voparis-tap-planeto.obspm.fr's Table Access Protocol (TAP) service with table metadata.
tap_schema.key_columnsTable InfoColumns participating in foreign key relationships between tables available for ADQL querying. PADC TAP Server on voparis-tap-planeto.obspm.fr's Table Access Protocol (TAP) service with table metadata.
tap_schema.keysTable InfoForeign key relationships between tables available for ADQL querying. PADC TAP Server on voparis-tap-planeto.obspm.fr's Table Access Protocol (TAP) service with table metadata.
tap_schema.schemasTable InfoSchemas containing tables available for ADQL querying. PADC TAP Server on voparis-tap-planeto.obspm.fr's Table Access Protocol (TAP) service with table metadata.
tap_schema.tablesTable InfoTables available for ADQL querying. PADC TAP Server on voparis-tap-planeto.obspm.fr's Table Access Protocol (TAP) service with table metadata.
titan_profiles.epn_coreTable InfoEPNcore table for temperature, pressure and element abundance profiles in Titan's atmosphere. This database contains vertical profiles of temperature and composition in Titan's atmosphere at several altitudes below 750 km. These profiles were retrieved from the infrared spectra acquired by the Composite Infrared Spectrometer (CIRS) aboard the Cassini spacecraft. The retrieval method and the description of the used dataset are detailed by Vinatier et al. (2010), and completed in Mathé et al. (2020), and Vinatier et al. (2020). References ---------- - Vinatier et al. (**2010**) Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission: I. Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles. *Icarus*, 206(2), 559-570. `doi:10.1016/j.icarus.2009.08.013 <https://doi.org/10.1016/j.icarus.2009.08.013>`_ - Mathé et al. (**2020**) Seasonal changes in the middle atmosphere of Titan from Cassini/CIRS observations: Temperature and trace species abundance profiles from 2004 to 2017. *Icarus*, 344, 113547. `doi:10.1016/j.icarus.2019.113547 <https://doi.org/10.1016/j.icarus.2019.113547>`_ - Vinatier et al. (**2020**), Temperature and chemical species distributions in the middle atmosphere observed during Titan's late northern spring to early summer. A&A 641, A116; `doi:10.1051/0004-6361/202038411 <https://doi.org/10.1051/0004-6361/202038411>`_
tnosarecool.epn_coreTable InfoN/A This service lists TNO thermal properties as derived mostly from Spitzer and Herschel observations.
vims_satellites.epn_coreTable InfoN/A The Visual and Infrared Mapping Spectrometer (VIMS) instrument onboard the Cassini spacecraft observed the system of Saturn, acquiring spectral cubes in the range 0.4-5.2 microns. This service focuses on Saturn satellites, and provides access to calibrated and ancillary data, computed as described here: https://vims.univ-nantes.fr/info/isis-calibration. It also provides direct links to a larger web site with previews.
vvex.epn_coreTable InfoIR spectroscopy of Venus VIRTIS/Venus Express demonstrator service: imaging spectroscopy of Venus in the visible and the near infrared. ** Assessment version from PI team database - some values currently missing ** This lists all calibrated files for the total mission and the three channels M-vis, M-IR and H. Files are described according to the PI team database, with links to the PSA: https://archives.esac.esa.int/psa/ftp/VENUS-EXPRESS/VIRTIS/VEX-V-VIRTIS-2-3-V3.0/. See Piccioni et al, 2007, VIRTIS: The Visible and Infrared Thermal Imaging Spectrometer, ESA SP 1295.
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