Add EPN-TAP data files.

Nathanael Jourdane
1 parent ec577a2d
Showing 4 changed files with 423 additions and 0 deletions Show diff stats
generic_data/EpnTapData/EpnTapProductTypes.json
generic_data/EpnTapData/EpnTapServices.json
generic_data/EpnTapData/EpnTapTargetClasses.json
generic_data/EpnTapData/EpnTapTargetNames.json
@@ -0,0 +1,15 @@
+[
+{"id": "al", "name": "All types"},
+{"id": "im", "name": "Image"},
+{"id": "ma", "name": "Map"},
+{"id": "sp", "name": "Spectrum"},
+{"id": "ds", "name": "Dynamic spectrum"},
+{"id": "sc", "name": "Spectral cube"},
+{"id": "pr", "name": "Profile"},
+{"id": "vo", "name": "Volume"},
+{"id": "mo", "name": "Movie"},
+{"id": "cu", "name": "Cube"},
+{"id": "ts", "name": "Time series"},
+{"id": "ca", "name": "Catalogue"},
+{"id": "ci", "name": "Catalogue item"}
+]
@@ -0,0 +1,366 @@
+[
+{
+"short_name": "AMDA",
+"res_title": "CDPP AMDA DataBase",
+"ivoid": "ivo://cdpp/amda",
+"access_url": "http://cdpp-epntap.cesr.fr/__system__/tap/run/tap",
+"table_name": "amdadb.epn_core",
+"content_type": "archive",
+"res_description": "The CDPP (Centre de Données de la Physique des Plasmas) was created in 1998 jointly by CNES and INSU. The CDPP is the French national data centre \n                        for natural plasmas of the solar system. The CDPP assures the long term preservation of data obtained primarily from instruments built using French \n                        resources, and renders them readily accessible and exploitable by the international community. The CDPP also provides services to enable on-line data \n                        analysis (AMDA), 3D data visualization in context (3DView), and a propagation tool which bridges solar perturbations to in-situ measurements. \n                        The CDPP is involved in the development of interoperability, participates in several Virtual Observatory projects, and supports data distribution for\n                        scientific missions (Solar Orbiter, JUICE).",
+"creator seq": "Centre de Données de la Physique des Plasmas",
+"content_level": "university#research",
+"reference_url": "http://amda.cdpp.eu",
+"created": "2014-11-06T17:00:00",
+"updated": "2014-11-13T17:00:00"
+},
+{
+"short_name": "APIS",
+"res_title": "Auroral Planetary Imaging and Spectroscopy",
+"ivoid": "ivo://vopdc.obspm/lesia/apis/epn",
+"access_url": "http://voparis-tap.obspm.fr/__system__/tap/run/tap",
+"table_name": "apis.epn_core",
+"content_type": "archive",
+"res_description": "The Auroral Planetary Imaging and Spectroscopy (APIS) service provides an open and interactive access to processed auroral observations of the outer planets and their satellites. Such observations are of interest for a wide community at the interface between planetology and magnetospheric and heliospheric physics. APIS consists of (i) a high level database, built from planetary auroral observations acquired by the Hubble Space Telescope (HST) since 1997 with its mostly used Far-UltraViolet spectro-imagers, (ii) a dedicated search interface aimed at browsing efficiently this database through relevant conditional search criteria and (iii) the ability to interactively work with the data online through plotting tools developed by the Virtual Observatory (VO) community, such as Aladin and Specview. This service is VO compliant and can therefore also been queried by external search portals of the VO community. The diversity of available data and the capability to sort them out by relevant physical criteria shall in particular facilitate statistical studies, on long-term scales and/or multi-instrumental multi-spectral combined analysis.",
+"creator seq": "L. Lamy",
+"content_level": "general#university#research#amateur",
+"reference_url": "http://lesia.obspm.fr/apis/",
+"created": "2012-06-06T00:00:00",
+"updated": "2016-05-04T00:00:00"
+},
+{
+"short_name": "BASECOM",
+"res_title": "The Nançay Cometary Database",
+"ivoid": "ivo://vopdc.obspm/lesia/basecom/epn",
+"access_url": "http://voparis-tap.obspm.fr/__system__/tap/run/tap",
+"table_name": "basecom.epn_core",
+"content_type": "archive",
+"res_description": "Since 1973, the 18-cm lines of the OH radical have been systematically observed\n         in a number of comets with the Nançay radio telescope. This allowed an evaluation of the\n         cometary water… production rates and their evolution with time, as well as a study of\n         several physical processes: the excitation mechanisms of the OH radio lines, the expansion\n         of the cometary atmospheres, their anisotropy in relation with non-gravitational forces,\n         the Zeeman effect in relation with the cometary magnetic field. The Nançay observations of\n         53 cometary apparitions between 1982 and 2009 are now organized in this\n         database.",
+"creator seq": "J. Crovisier",
+"content_level": "general#university#research#amateur",
+"reference_url": "http://www.lesia.obspm.fr/planeto/cometes/basecom/",
+"created": "2009-08-07T00:00:00",
+"updated": "2013-11-26T00:00:00"
+},
+{
+"short_name": "BDIP",
+"res_title": "Base de Données d\u0027Images Planetaires",
+"ivoid": "ivo://vopdc.obspm/lesia/bdip/epn",
+"access_url": "http://voparis-tap.obspm.fr/__system__/tap/run/tap",
+"table_name": "bdip.epn_core",
+"content_type": "archive",
+"res_description": "The database of planetary images (BDIP) comes from the digitization of\n         photographs collected and preserved by the Center for Photographic Documentation of the\n         planets held by the IAU at the Meudon Observatory in 1961 under the the curation of J.H.\n         Focas (IAUC, 12th General Assembly, Report 1964). A similar center was established at the\n         Lowell Observatory in Arizona, under the responsibility of W.A. Baum. The photographs were\n         duplicated between the two centers.",
+"creator seq": "F. Henry",
+"content_level": "general#university#research#amateur",
+"reference_url": "http://lesia.obspm.fr/BDIP/",
+"created": "2012-06-06T00:00:00",
+"updated": "2013-02-28T00:00:00"
+},
+{
+"short_name": "BIRA-IASB TAP",
+"res_title": "VESPA PA team server TAP service",
+"ivoid": "ivo://bira-iasb/tap",
+"access_url": "http://vespa-ae.oma.be/tap",
+"table_name": "soir.epn_core",
+"content_type": "",
+"res_description": "The VESPA PA team server\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, emptyobscore, obscore from the ivoa schema, epn_core from the soir schema.",
+"creator seq": "Loic Trompet",
+"content_level": "",
+"reference_url": "http://vespa-ae.oma.be/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2016-06-23T13:56:35"
+},
+{
+"short_name": "ExoPlanet",
+"res_title": "Extrasolar Planets Encyclopaedia",
+"ivoid": "ivo://vopdc.obspm/luth/exoplanet/epn",
+"access_url": "http://voparis-tap.obspm.fr/__system__/tap/run/tap",
+"table_name": "exoplanet.epn_core",
+"content_type": "catalog",
+"res_description": "VO-compliant and interactive encyclopaedia of extrasolar planets.",
+"creator seq": "J. Schneider",
+"content_level": "general#university#research#amateur",
+"reference_url": "http://exoplanet.eu/",
+"created": "2012-11-04T00:00:00",
+"updated": "2013-02-28T00:00:00"
+},
+{
+"short_name": "IAA and CAB TAP",
+"res_title": "Cross section values TAP service",
+"ivoid": "ivo://spectrum.iaa/tap",
+"access_url": "http://spectrum.iaa.es/tap",
+"table_name": "abs_cs.epn_core",
+"content_type": "",
+"res_description": "The Cross section values\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, emptyobscore, obscore from the ivoa schema, epn_core from the abs_cs schema.",
+"creator seq": "IAA-CSIC",
+"content_level": "",
+"reference_url": "http://spectrum.iaa.es/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2016-04-03T18:56:07"
+},
+{
+"short_name": "IKS",
+"res_title": "IR spectroscopy of comet Halley",
+"ivoid": "ivo://vopdc.obspm/lesia/iks/epn",
+"access_url": "http://voparis-tap.obspm.fr/__system__/tap/run/tap",
+"table_name": "iks.epn_core",
+"content_type": "archive",
+"res_description": "Measurements of comet Halley in the spectral channel of IKS on board the Vega-1\n         spacecraft. Data are retrieved from the PDS Small Bodies Node archive (2011 reformatted\n         version) and completed with extra information from the original team. The dataset consists\n         in 101 tables providing the calibrated radiance spectra of comet Halley as distance\n         decreases, plus two composite spectra in different spectral ranges. For details and further\n         references, see: Combes M. et al., 1988, The 2.3-12 micron Spectrum of Comet Halley from\n         the IKS-VEGA Experiment, Icarus, 76, 404-436.",
+"creator seq": "LESIA",
+"content_level": "general#university#research",
+"reference_url": "http://lesia.obspm.fr/IKS/",
+"created": "2013-10-12T00:00:00",
+"updated": "2013-11-26T00:00:00"
+},
+{
+"short_name": "LATMOS TAP",
+"res_title": "SPICAM TAP service",
+"ivoid": "ivo://latmos.ipsl/tap",
+"access_url": "http://vo.projet.latmos.ipsl.fr/tap",
+"table_name": "locdens.epn_core",
+"content_type": "",
+"res_description": "The SPICAM\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the locdens schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the mcd schema, epn_core from the ozone schema, epn_core from the spicam schema, emptyobscore, obscore from the ivoa schema.",
+"creator seq": "Zi Yin",
+"content_level": "",
+"reference_url": "http://vo.projet.latmos.ipsl.fr/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2016-04-20T11:08:34"
+},
+{
+"short_name": "LATMOS TAP",
+"res_title": "SPICAM TAP service",
+"ivoid": "ivo://latmos.ipsl/tap",
+"access_url": "http://vo.projet.latmos.ipsl.fr/tap",
+"table_name": "ozone.epn_core",
+"content_type": "",
+"res_description": "The SPICAM\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the locdens schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the mcd schema, epn_core from the ozone schema, epn_core from the spicam schema, emptyobscore, obscore from the ivoa schema.",
+"creator seq": "Zi Yin",
+"content_level": "",
+"reference_url": "http://vo.projet.latmos.ipsl.fr/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2016-04-20T11:08:34"
+},
+{
+"short_name": "LATMOS TAP",
+"res_title": "SPICAM TAP service",
+"ivoid": "ivo://latmos.ipsl/tap",
+"access_url": "http://vo.projet.latmos.ipsl.fr/tap",
+"table_name": "spicam.epn_core",
+"content_type": "",
+"res_description": "The SPICAM\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the locdens schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the mcd schema, epn_core from the ozone schema, epn_core from the spicam schema, emptyobscore, obscore from the ivoa schema.",
+"creator seq": "Zi Yin",
+"content_level": "",
+"reference_url": "http://vo.projet.latmos.ipsl.fr/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2016-04-20T11:08:34"
+},
+{
+"short_name": "M4AST",
+"res_title": "M4AST - Modeling for Asteroids",
+"ivoid": "ivo://vopdc.obspm/imcce/m4ast",
+"access_url": "http://voparis-tap.obspm.fr/__system__/tap/run/tap",
+"table_name": "m4ast.epn_core",
+"content_type": "archive",
+"res_description": "Compiled database for asteroid spectra in the visible and nir regions.",
+"creator seq": "M. Birlan",
+"content_level": "general#university#research#amateur",
+"reference_url": "http://cardamine.imcce.fr/m4ast",
+"created": "2011-11-15T00:00:00",
+"updated": "2015-11-16T00:00:00"
+},
+{
+"short_name": "Titan",
+"res_title": "Vertical Profiles in Titan Middle Atmosphere",
+"ivoid": "ivo://vopdc.obspm/lesia/titan/epn",
+"access_url": "http://voparis-tap.obspm.fr/__system__/tap/run/tap",
+"table_name": "titan.epn_core",
+"content_type": "archive",
+"res_description": "This database displays vertical profiles of temperature and composition in\n         Titan\u0027s atmosphere at nine different latitudes between 100 and 500 km. These profiles were\n         retrieved from the infrared spectra acquired by the Composite Infrared Spectrometer (CIRS)\n         aboard the Cassini spacecraft. The retrieval method and the description of the used dataset\n         is detailed by Vinatier et al., 2009, Analysis of Cassini/CIRS limb spectra of Titan\n         acquired during the nominal mission. I: Hydrocarbons, nitriles and CO2 vertical mixing\n         ratio profiles, Icarus, in press. doi:10.1016/j.icarus.2009.08.013.",
+"creator seq": "S. Vinatier",
+"content_level": "general#university#research#amateur",
+"reference_url": "http://www.lesia.obspm.fr",
+"created": "2012-06-06T00:00:00",
+"updated": "2013-09-09T00:00:00"
+},
+{
+"short_name": "Tohoku TAP",
+"res_title": "Iitate Radio Data Server TAP service",
+"ivoid": "ivo://tohoku.univ.jp/tap",
+"access_url": "http://thebe.gp.tohoku.ac.jp/tap",
+"table_name": "hisaki.epn_core",
+"content_type": "",
+"res_description": "The Iitate Radio Data Server\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the iitate schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the iitate_test schema, epn_core from the hisaki schema, epn_core from the pparc_r schema, emptyobscore, obscore from the ivoa schema.",
+"creator seq": "Atsushi Kumamoto",
+"content_level": "",
+"reference_url": "http://thebe.gp.tohoku.ac.jp/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2015-11-12T01:43:44"
+},
+{
+"short_name": "Tohoku TAP",
+"res_title": "Iitate Radio Data Server TAP service",
+"ivoid": "ivo://tohoku.univ.jp/tap",
+"access_url": "http://thebe.gp.tohoku.ac.jp/tap",
+"table_name": "iitate.epn_core",
+"content_type": "",
+"res_description": "The Iitate Radio Data Server\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the iitate schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the iitate_test schema, epn_core from the hisaki schema, epn_core from the pparc_r schema, emptyobscore, obscore from the ivoa schema.",
+"creator seq": "Atsushi Kumamoto",
+"content_level": "",
+"reference_url": "http://thebe.gp.tohoku.ac.jp/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2015-11-12T01:43:44"
+},
+{
+"short_name": "Tohoku TAP",
+"res_title": "Iitate Radio Data Server TAP service",
+"ivoid": "ivo://tohoku.univ.jp/tap",
+"access_url": "http://thebe.gp.tohoku.ac.jp/tap",
+"table_name": "iitate_test.epn_core",
+"content_type": "",
+"res_description": "The Iitate Radio Data Server\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the iitate schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the iitate_test schema, epn_core from the hisaki schema, epn_core from the pparc_r schema, emptyobscore, obscore from the ivoa schema.",
+"creator seq": "Atsushi Kumamoto",
+"content_level": "",
+"reference_url": "http://thebe.gp.tohoku.ac.jp/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2015-11-12T01:43:44"
+},
+{
+"short_name": "Tohoku TAP",
+"res_title": "Iitate Radio Data Server TAP service",
+"ivoid": "ivo://tohoku.univ.jp/tap",
+"access_url": "http://thebe.gp.tohoku.ac.jp/tap",
+"table_name": "pparc_r.epn_core",
+"content_type": "",
+"res_description": "The Iitate Radio Data Server\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the iitate schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the iitate_test schema, epn_core from the hisaki schema, epn_core from the pparc_r schema, emptyobscore, obscore from the ivoa schema.",
+"creator seq": "Atsushi Kumamoto",
+"content_level": "",
+"reference_url": "http://thebe.gp.tohoku.ac.jp/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2015-11-12T01:43:44"
+},
+{
+"short_name": "epn1 TAP",
+"res_title": "epn1 TAP service",
+"ivoid": "ivo://jacobsuni/tap",
+"access_url": "http://epn1.epn-vespa.jacobs-university.de/tap",
+"table_name": "crism.epn_core",
+"content_type": "",
+"res_description": "The epn1\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the ft schema, epn_core from the foottest schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the robbinscraterdata2 schema, epn_core from the usgs_wms schema, epn_core from the crism schema, emptyobscore, obscore from the ivoa schema, epn_core from the mars_craters schema.",
+"creator seq": "Mikhail Minin",
+"content_level": "",
+"reference_url": "http://epn1.epn-vespa.jacobs-university.de/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2016-02-29T09:44:18"
+},
+{
+"short_name": "epn1 TAP",
+"res_title": "epn1 TAP service",
+"ivoid": "ivo://jacobsuni/tap",
+"access_url": "http://epn1.epn-vespa.jacobs-university.de/tap",
+"table_name": "ft.epn_core",
+"content_type": "",
+"res_description": "The epn1\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the ft schema, epn_core from the foottest schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the robbinscraterdata2 schema, epn_core from the usgs_wms schema, epn_core from the crism schema, emptyobscore, obscore from the ivoa schema, epn_core from the mars_craters schema.",
+"creator seq": "Mikhail Minin",
+"content_level": "",
+"reference_url": "http://epn1.epn-vespa.jacobs-university.de/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2016-02-29T09:44:18"
+},
+{
+"short_name": "epn1 TAP",
+"res_title": "epn1 TAP service",
+"ivoid": "ivo://jacobsuni/tap",
+"access_url": "http://epn1.epn-vespa.jacobs-university.de/tap",
+"table_name": "mars_craters.epn_core",
+"content_type": "",
+"res_description": "The epn1\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the ft schema, epn_core from the foottest schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the robbinscraterdata2 schema, epn_core from the usgs_wms schema, epn_core from the crism schema, emptyobscore, obscore from the ivoa schema, epn_core from the mars_craters schema.",
+"creator seq": "Mikhail Minin",
+"content_level": "",
+"reference_url": "http://epn1.epn-vespa.jacobs-university.de/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2016-02-29T09:44:18"
+},
+{
+"short_name": "epn1 TAP",
+"res_title": "epn1 TAP service",
+"ivoid": "ivo://jacobsuni/tap",
+"access_url": "http://epn1.epn-vespa.jacobs-university.de/tap",
+"table_name": "usgs_wms.epn_core",
+"content_type": "",
+"res_description": "The epn1\u0027s TAP end point. The Table Access\nProtocol (TAP) lets you execute queries against our database tables,\ninspect various metadata, and upload your own data. It is thus the\nVO\u0027s premier way to access public data holdings.\n\nTables exposed through this endpoint include: epn_core from the ft schema, epn_core from the foottest schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the robbinscraterdata2 schema, epn_core from the usgs_wms schema, epn_core from the crism schema, emptyobscore, obscore from the ivoa schema, epn_core from the mars_craters schema.",
+"creator seq": "Mikhail Minin",
+"content_level": "",
+"reference_url": "http://epn1.epn-vespa.jacobs-university.de/__system__/tap/run/info",
+"created": "2009-12-01T10:00:00",
+"updated": "2016-02-29T09:44:18"
+},
+{
+"short_name": "hfc1ar",
+"res_title": "Heliophysics Feature Catalog active regions",
+"ivoid": "ivo://vopdc.obspm/lesia/hfc1ar/epn",
+"access_url": "http://voplus.obspm.fr:81/__system__/tap/run/tap",
+"table_name": "hfc1ar.epn_core",
+"content_type": "catalog",
+"res_description": "Solar active regions extracted from Heliophysics Feature Catalog.",
+"creator seq": "J. Aboudarham",
+"content_level": "general#university#research",
+"reference_url": "http://voparis-helio.obspm.fr/hfc-gui/",
+"created": "2014-04-03T00:00:00",
+"updated": "2015-11-16T00:00:00"
+},
+{
+"short_name": "hfc1t3",
+"res_title": "Heliophysics Feature Catalog type 3 radio bursts",
+"ivoid": "ivo://vopdc.obspm/lesia/hfc1t3/epn",
+"access_url": "http://voplus.obspm.fr:81/__system__/tap/run/tap",
+"table_name": "hfc1t3.epn_core",
+"content_type": "catalog",
+"res_description": "Solar type 3 bursts extracted from Heliophysics Feature Catalog.",
+"creator seq": "J. Aboudarham",
+"content_level": "general#university#research",
+"reference_url": "http://voparis-helio.obspm.fr/hfc-gui/",
+"created": "2014-04-03T00:00:00",
+"updated": "2015-11-16T00:00:00"
+},
+{
+"short_name": "nasadustcat",
+"res_title": "INAF-IAPS RDB NASA dust catalogue TAP service",
+"ivoid": "ivo://ia2.inaf.it/hosted/iaps/epn/tap/nasadustcat",
+"access_url": "http://ia2-tap.oats.inaf.it:8080/epntap",
+"table_name": "nasadustcat.epn_core",
+"content_type": "catalog",
+"res_description": "The Cosmic dust catalog is an internal resource of the SBDN, since we have internally developed original services to access this catalogs.\n\n        NASA\u0027s Cosmic dust catalog 15 and 18 have been joined to obtain this service. 467 (from catalog 15) plus 957 (from catalog 18) dust grains with their main characteristics, images and X-ray spectra are listed. Not only cosmic dust particles are listed, but also terrestrial contamination (natural), terrestrial contamination (artificial) and aluminium oxide spheres.",
+"creator seq": "IA2",
+"content_level": "research",
+"reference_url": "http://www.iasf-roma.inaf.it:8080/web/sbdn/cosmic-dust-catalog",
+"created": "2013-02-20T08:00:49",
+"updated": "2013-12-05T08:30:00"
+},
+{
+"short_name": "planets",
+"res_title": "Main characteristics of solar system planets",
+"ivoid": "ivo://vopdc.obspm/lesia/planets/epn",
+"access_url": "http://voparis-tap.obspm.fr/__system__/tap/run/tap",
+"table_name": "planets.epn_core",
+"content_type": "catalog",
+"res_description": "This service provides the most accurate values of dimensions, mass, and rotation period of solar system planets. These data are retreived from Archinal et al 2009 (IAU report, 2011CeMDA.109..101A) (radii and Cox et al 2000 (Allen\u0027s astrophysical quantities, 2000asqu.book.....C) (masses, heliocentric distances, and rotation periods).",
+"creator seq": "S. Erard",
+"content_level": "general#university#research#amateur",
+"reference_url": "http://lesia.obspm.fr",
+"created": "2015-08-16T00:00:00",
+"updated": "2016-02-05T00:00:00"
+},
+{
+"short_name": "routinejup",
+"res_title": "Jupiter Routine Observations",
+"ivoid": "ivo://vopdc.obspm/usn/dam/routinejup/epn",
+"access_url": "http://vogate.obs-nancay.fr/__system__/tap/run/tap",
+"table_name": "dam.epn_core",
+"content_type": "catalog",
+"res_description": "Dynamic Spectra of the Routine observation of Jupiter with the Nancay Decameter Array. This dataset contains two series of dynamic spectra recorded on each of the Nançay decameter sub-arrays (i.e. on Left Hand and Right Hand Polarization). The receiver is sampling from 10 MHz to 40 MHz with 75 kHz steps on the spectral axis. It records one spectrum every second on each polarization. The list of observation frequencies is provided.",
+"creator seq": "B. Cecconi",
+"content_level": "general#university#research#amateur",
+"reference_url": "http://www.obs-nancay.fr/en/index.php/instruments/decametric-array",
+"created": "2014-04-09T00:00:00",
+"updated": "2015-11-17T00:00:00"
+}
+]
@@ -0,0 +1,17 @@
+[
+{"id": "al", "name": "All targets"},
+{"id": "asteroid", "name": "Asteroid"},
+{"id": "dwarf_planet", "name": "Dwarf planet"},
+{"id": "planet", "name": "Planet spectrum"},
+{"id": "satellite", "name": "Satellite"},
+{"id": "comet", "name": "Comet"},
+{"id": "exoplanet", "name": "Exoplanet"},
+{"id": "interplanetary_medium", "name": "Interplanetary medium"},
+{"id": "ring", "name": "Ring"},
+{"id": "sample", "name": "Sample"},
+{"id": "sky", "name": "Sky"},
+{"id": "spacecraft", "name": "Spacecraft"},
+{"id": "spacejunk", "name": "Spacejunk"},
+{"id": "star", "name": "Star"},
+{"id": "calibration", "name": "Calibration"}
+]
@@ -0,0 +1,25 @@
+[
+{"n": "All"},
+{"n": "Heliosphere"},
+{"n": "Earth"},
+{"n": "Neptune"},
+{"n": "Jupiter"},
+{"n": "Tethys"},
+{"n": "Iapetus"},
+{"n": "Interstellar"},
+{"n": "Titan"},
+{"n": "Enceladus"},
+{"n": "Dione"},
+{"n": "Rhea"},
+{"n": "Mimas"},
+{"n": "Europa"},
+{"n": "Saturn"},
+{"n": "Mars"},
+{"n": "Uranus"},
+{"n": "Venus"},
+{"n": "Callisto"},
+{"n": "Ganymede"},
+{"n": "Mercury"},
+{"n": "Comet"},
+{"n": "Io"}
+]