|Short Name||Name||Description||Location||Status||To do (v1 or v2)||Comments||Version_2 / updates|
|Titan||Vertical Profiles in Titan Middle Atmosphere||Atmospheric profiles of Titan (Cassini/CIRS)||PADC|
√ Check descriptions
Check/correct file names and headers!!!
Fix UCDs (coordinates at least)
|Updated to v2, to be tested again|
|VVEx||VIRTIS on Venus-Express: standard dataset||Access to spectral cubes. Venus-Express legacy||PADC|
Complete data description with geometry, enlarge to the complete dataset. Mostly intended as a demonstrator of EPN-TAP access to the PSA. In the mid-term, this will be the basis to include derived products, which are not in the PSA.
|v1 addressing part of nominal mission, limited nb of parameters|
still target_class=Star instead of star
|v2 update from Toulouse 2016 workshop - waiting to retrieve last parameters (geometry)|
|VVEx+||Enhanced VIRTIS dataset on Venus-Express||Will provide access to individual spectra. Venus-Express legacy (after discussion: same service as above, not a separated one)||PADC|
|Enlarge the above service to also provide description of VIRTIS/ VEx individual spectra with geometry parameters. Access may be a script extracting the corresponding data from the cubes (TBC). This will be a noticeable added value wrt a similar service from the PSA, only possible from the PI team.|
|abs_cs||Absorption cross sections||Absorption cross sections for gaseous species of atmospheric interest|
|√ Finalize, declare,|
add data + setup special access script (output selected species in a single table)
|First model in v2 from Toulouse 2016 VESPA workshop|
|SOIR||SOIR/SPICAV/VEx||UV / IR observations of Venus - vertical profiles||Royal Belgian Institute for Space Aeronomy / Planetary Aeronomy|
|Convert profiles to VOtable, easier to handle and visualize.||First model in v2 from Toulouse 2016 VESPA workshop|
|SPICAM||SPICAM / MEx||Vertical profiles of Mars||LATMOS|
Parameters to be updated
Reviewed, need to implement corrections
|Number of issues identified afterwards, including extra table not integrated.|
v2 direct from Toulouse 2016 workshop.
Tests during Prague workshop, 2018.
|SPICAV||SPICAV / VEx||Vertical profiles of Venus||LATMOS|
|From updated SPICAM service|
|mcd||Mars Climate Database||Sampled version through EPN-TAP||PADC + LMD|
First version on sampled data, access to vertical profiles only, reviewed.
Need to implement corrections (issues identified later on).
Add daily cycles and planes? Add more scenarios.
Second version will use datalink to provide access to continuous input parameters.
v2 installed from Toulouse 2016 VESPA workshop
|OMEGA / MEx atm db||LESIA, Melchiori|
|Exhume data, if possible||Only covers beginning of mission|
|Titan GCM db|
|Oct 2016: P. Rannou suggests to contact S. Lebonnois for his more modern 3D code.|
Only available as a code for the time being.
May be a candidate for direct code integration.
|BaseCom||The Nançay Cometary Database||Radio observation of comets from Nançay||PADC|
Restructure, clean up
|All the fits must be reconstructed from txt files; freq_min and max to be cleaned up.||Updated to v2, to be tested and refreshed|
|M4ast||Modeling for Asteroids||Asteroid spectroscopy||PADC|
|updated to v2|
|NASA dust catalog||INAF-IAPS RDB NASA dust catalogue TAP service||NASA's Cosmic dust catalogs 15 and 18||IAPS, Rome|
Restructure, Check descriptions, Update server
|v2 in progress, the open service is still an adapted v1!!!|
|IKS||IR spectroscopy of comet Halley||IR spectroscopy of 1P/Halley (IKS / Vega-1)||PADC|
√ Check descriptions,
And better thumbnails!
Descriptors updated April 2016, new web page Sept 2017.
First v2 test case (old way). Updated to mixin/grammar, Dec 2017.
|TNOsarecool||TNOs are cool||Compilation of TNOs properties + Herschel/Spitzer observations||PADC|
√ Make it consistent with M4ast, MPCOrb and DynAstVO.
Check some parameters
|Classes of small bodies still to be refined||v2 direct|
|Illu67P||Illumination maps of 67P/C-G||Shows the comet illumination for a given lat/lon of the Sun in the comet frame. Next step: shows the comet illumination for a given time||IRAP + Imperial College, London. A. Beth|
√ Finalize, add data, declare.
|Directly in v2 from Toulouse 2016 VESPA workshop|
|DynAstVO||Minor Planet parameters and orbits, with daily computation (NEO only)||IMCCE / PADC|
√ Add computed orbits as spice files, open in Cosmographia or similar.
Update in May 2018, TBC
|Spice kernels are usable in Cosmographia (manually on user's end) and 3Dview (if they are installed on the server part)|
Directly in v2 from computation results
|MPC||Minor Planets Center||Asteroid orbital and physical parameters||MPC / IAU, |
√ Provide epn_core view on existing TAP service in Heidelberg
|First experiment with EPN-TAP2 mixin||Make consistent with other small bodies services|
|CEMLS||Cometary emission line catalogue||Comet line catalogue, from observations||IAPS, Rome|
|Only provides band list with reference. Make it SLAP or LineList compliant?|
|BDIC||Base de Données d'Images Cométaires||PADC/LESIA, Henry|
|To be adapted from updated BDIP v2|
|SBNAF||Small Bodies Near and Far||Catalogue of asteroids &TNOs properties, from observations||Max Planck|
|To be reveiwed and finalized||VESPA 2018 Prague workshop|
|Comets||Base de données des observateurs de comètes||Amateur site (high level) with > 16000 images (+ some spectra included). Includes db and submission system||PADC/LESIA, Biver|
Simply write an EPN-TAP view with daily updates from existing db?
Other similar db to be studied too.
|Web version operational (http://lesia.obspm.fr/comets) Also includes links to sdd.jpl and MPC ephemeris and properties + db of observers (29 contributors). Basic table is a concatenation of target tables? Includes images + derived quantities and references.|
|MP3C||EPN-TAP access to existing MP3C||Small bodies catalogue, contains colors and spectral types||OCA Nice, M. Delbo / C. Ordenovich|
|Relies on TAPlib - interface study by PLS in July that year; then crashed due to local system.||Graz workshop, 2017|
|TNO spectra||VLT large program from ~2005||LESIA, Barucci|
|Find calibrated spectra in LESIA, evaluate|
Small Main-Belt Asteroid Spectroscopic Survey
Binzel et al VNIR spectra of asteroids
|MIT with support from PADC?|
Based on M4ast, very similar data - suggested by Mirel Birlan.
Coupled with "MIT-UH-IRTF Joint Campaign for NEO Spectral Reconnaissance" on the same site.
Plots/thumbnails have to be regenerated individually in PNG.
Physical properties of (some) NEOs
|Paris or Rome?|
Includes a (spectral) taxonomy type. Some duplication of MPC parameters (can be filtered out?)
Regularly updated on-line.
Table is easy to enter (note that Binary objects, noted B in 1rst column, have 2 entry lines; only the first one is relevant).
Each object has a detailed page with extensive biblio that cannot be included in the table - should be linked with external_link parameter)
|Mars_craters||Mars craters database||Robbin's crater database||JacobsUni|
√ Completed to entire dataset
|To be completed with revised version from GEOPS||v2 direct, with mixin|
|USGS_WMS||Planetary maps from USGS||EPN-TAP access to WMS server||JacobsUni|
√ Check data access
Add the list of planetary HiPS at CDS in this service?
|Model for GIS-VO bridge (WMS)||v2 direct, with mixin|
|CRISM||CRISM/MRO cubes||Imaging spectroscopy of Mars, WMS access||JacobsUni|
Check data access
√ Check descriptions
|Model for GIS-VO bridge (WCS) and QGIS plugins (working in May 2017)||v2 direct with mixin from Toulouse workshop, then updated|
|HRSC||HRSC / MEx images||HiRes imaging of Mars, WMS access||Frei Univ, Berlin (Sebastian Walter)|
|Finalize, ingest (many) data||Uses mixin + PDS grammar||Draft from Roscoff surface workshop|
M3 / CHANDRAYAAN-1 cubes
|Imaging spectroscopy of the Moon, WMS access||JacobsUni|
|Finalize, ingest (many) data||Partial version on-line, Jan 2018|
Pangaea-X 2017 data
|Various measurements on planetary analogue environment||JacobsUni|
|Finalize, ingest other data||First assessment with drone images, model for TA field campaign data.|
|Imaging spectroscopy of Mars||OMEGA/MEx spectral cubes in calibrated format. Non-PDS files||IAS/PSup|
|Review details, optimize format||VESPA 2018 Prague workshop|
|omega_maps||Mineralogy spectroscopy of Mars||Mineralogical maps from OMEGA analysis, fits format||IAS/PSup|
|VESPA 2018 Prague workshop|
|Dawn VIR||Imaging spectroscopy of Vesta and Ceres||Dawn/VIR spectral cubes of Vesta and Ceres||IAPS/Rome|
|Identify ivoID of provider|
|Various db from Brown University||see here http://www.planetary.brown.edu/html_pages/data.htm|
|Provide as list of catalogues?|
|IRS / Mariner 6/7 obs of Mars||Spectroscopy of Mars|
|Convert data files to integrated VOTables & add to PDS3 native format (like IKS)||Older dataset… but seems unique and only distributed on a personal web site|
|PDS spectral lib||Laboratory spectroscopy of mineral samples||Library in support of CRISM/MRO, on PDS Geosciences node||PADC / LESIA, Erard|
|√ Define (spectral) extension to describe minerals. Can be enlarged with other open mineral spectroscopy db - either in the same service or separately, this is mostly a political decision||√ To be studied with SSHADE & DLR emission database & external contributors.|
Uses mixin/CSV grammar
|Draft from Graz 2017 VESPA workshop. Assessment for other lab spectroscopy services.|
|BRSL||Berlin Reflectance Spectral Library||Laboratory spectroscopy of mineral samples in support of VIRTIS/Rosetta||DLR, Kappel / Henckel|
√ Finalize, review
Publish (issue at DLR)
|Uses mixin/CSV grammar||Draft from Graz 2017 VESPA workshop. Assessment for other lab spectroscopy services.|
|PSL||Planetary Spectroscopy Laboratory||Laboratory spectroscopy of mineral samples in support of MERTIS/BepiColombo, and more (in emission)||DLR, Helbert / Maturilli|
First Europanet TA database
Uses mixin/CSV grammar.
Uses DaCHS Docker version
|VESPA 2018 Prague workshop|
Spectroscopy of ices and minerals
|Spectro / sample descriptors required.||A set of ~ 20 evolving databases (including GhoSST). Regular update required.||VESPA 2018 Prague workshop|
Magnetospheres / radio
|AMDA||CDPP AMDA DataBase||AMDA Planetary Plasma database||CDPP, Toulouse|
√ check server
|Regular connection to APIS||Updated to v2|
|APIS||Auroral Planetary Imaging and Spectroscopy||Aurorae images/spectra data base (HST)||PADC, Paris|
√ Check descriptions
access_url should point to spectra, not to images of spectra (spectra are under native_access_url)
|Reference for EPN-TAP extension to auroral data. Get data selection from Hisaki (Nov 2017)|
updated to v2, then refreshed
|Nancay Decameter Array observation database||Jupiter decametric radio observations from Nançay.|
Part of JUNO-Ground-Radio Observation Support.
|Check descriptions |
√ update target name
(formerly JupiterDAM then NDA, then RoutineJupiter)
|Updated to v2, to be tested|
|RadioJove||Amateur radio observations of Jupiter||PADC|
|Finalize, check descriptions|
|Updated to v2|
|MDISC||Access to UCL Magnetodisc model output.||UCL, London|
|Distribute data both in matlab and netCDF format||Work on tool connection for reading / visu||First model in v2 from Toulouse 2016 VESPA workshop|
|Kronos||Cassini radio data||PADC|
|DB exists, implement as a v2 service|
|IMPEx_EPN20||Db from IMPEX simulation tree||Graz, IWF|
|√ Resurrect, update|
√ Fix data access! - some data at FMI were removed
updated to v2
Enlargement in AMDA studied during Graz meeting
|VExMAG_EPN20||Dataset from MAG/Venus-Express||Venus-Express legacy||Graz, IWF|
|√ Resurrect, update||updated to v2 from Toulouse 2016 VESPA workshop|
|IitateHF||Iitate Radio Telescope HF data of Jupiter||Part of JUNO-Ground-Radio Observation Support||Iitate / Tohoku Univ, Japan|
Data is updated every night, after daily observation
(formerly called Iitate)
Updated to v2, being tested
|Hisaki||Hisaki E-UV observations of Jupiter, Venus and more||From Hisaki JAXA mission, Exceed instrument||Tohoku Univ, Japan|
Finalize, add calibrated data
Some non-compliances to be corrected in Dec 2017
|Regularly synchronized with APIS (Nov 2017)||Test service, v2 direct|
|KHTM||MHD instabilities at 67P/C-G||IAPS, Rome, Ivanovski, Capria|
|Adapt coordinate system to something more std||First model in v2 from Toulouse 2016 VESPA workshop|
|A Transplanet model of magnetosphere-ionosphere coupling at Earth, Mars, and Jupiter (simulation runs)||IRAP, Toulouse|
|To be tested and populated||From PSWS WP, 6/2017|
MarsExpress / Marsis
|Atmosphere only||U. of Iowa, SwRI|
|Handle times series with Autoplot and das2server (with changing resolution)||VESPA 2018 Prague workshop|
|ASPERA||MarsExpress / ASPERA data||U. of Iowa, SwRI|
|Handle times series with Autoplot and das2server (with changing resolution)||VESPA 2018 Prague workshop|
|LOFAR-FR606||Coordinated Decametric observations from LOFAR station in Nançay (nb FR606)||Part of JUNO-Ground-Radio Observation Support||Nançay|
|LOFAR bis||LOFAR test service||SRC PAS, Poland|
|Graz workshop 2017|
|Space weather test service||Space weather test service||SRC PAS, Poland|
|Graz workshop 2017|
|Coordinated Decametric observations from Ukraine T-shaped Radiotelescope-2. Part of JUNO-Ground-Radio Observation Support||Institute of radio astronomy NASU / RINANU. Kharkov, Ukraine|
|Workaround solution for public data installed in Japan, still not functional.|
File formatting issue (TBC)
Still distributing raw binary data files (4000+ files, 2GB each), no previews yet.
|(to be enlarged to other instruments than UTR2 on Kharkov site)|
First model in v2 from Toulouse 2016 VESPA workshop.
Updated May 2017 with mixin/custom grammar
|LWA1||Coordinated Decametric observations from Long Wavelength Array 1||Part of JUNO-Ground-Radio Observation Support||Owens Valley, New Mexico, USA|
|Cluster data||Cluster data in CDF format, to be processed with iPECMAN tool. Requires new UCD to be defined (spectral matrix). Output (also CDF) to be visualized in Autoplot.||IAP, Prague|
|Initial setup OK, issue with DaCHS server|
|Encyclopedia of Extra-Solar Planets||Encyclopedia of Extra-Solar Planets||Compilation of published data||PADC|
|√ EPN-TAP descriptors reviewed (April 2017)||Reference for EPN-TAP extension to exoplanets and celestial objects||Updated to v2, TAP output checked.|
|Heliophysics Feature Catalog type 3 radio bursts||Solar feature catalogues (from HELIO program)||PADC|
|Check descriptions and links, fixes required||Updated to v2, to be tested|
|Heliophysics Feature Catalog active regions||Solar feature catalogues (from HELIO program)||PADC|
|Check descriptions and links, fixes required||UCD of HFC1 must be reviewed||Updated to v2, to be tested|
|Solar radio observations||Iitate / Tohoku Univ, Japan|
Populate? (expected regular updates, TBC)
|(Formerly called pparc_r)||v2 direct, to be tested|
|CLIMSO||Images of the photosphere and low corona with two coronagraphs (on H-α, He I, Fe XIII) and two telescopes (on H-α, Ca II)||IRAP, Toulouse|
|Evolving data content, seems OK||First model in v2 from Toulouse 2016 VESPA workshop, then updated|
| Final review and finalization|
First draft in May 2017.
Published May 2018
|Radio Solar Database||Radio Solar Database||From Nançay||PADC|
|Design VO interface. Make it consistent with other projects in the field|
|E-Callisto||World-wide network of Solar radio spectrographs||Windisch (Switzerland)|
|Database exists, EPNcore view to build, ~straightforward|
Generic / interdisciplinary
|BDIP||Base de Données d'Images Planétaires||Historical planetary images in Meudon (ground-based)||PADC / LESIA (Drossart, Henry, Cecconi)|
√ Rearrange data products (jpeg vs fits), add previews, + check descriptions (from local db)
Compute pointing (mostly phase) + Fix image orientation?
Enlarge contents (other existing digitized images)
Phase angle can be retrieved from Miriad.
Orientation is more difficult.
|Updated to v2, to be tested.|
Sept 2017: rebuilt with mixin / grammar, queries LESIA database in SQL during ingestion.
|Planets||Main characteristics of planets||From IAU / Allen reference data||PADC|
√ Declare properly in registry (issue with referenceURL field)
To be enlarged with satellites info (see below)?
(In Feb 2016) best model for UCDs / param (with IKS) & q.rd file.
Add datalink to Miriad (OK in test, Jan 2018)
Test service, updated to v2 in 2016.
Updated to mixin/grammar Dec 2017
|Extend "Planets" service|
Satellites info available at IMCCE, to be added.
|PVOL||Amateur imaging of giant planets + Mars/Venus||Planetary Sciences Group, UPV/EHU, Bilbao|
√ SQL trigger to handle new data coming in.
|Possible issue with corrections after ingestion, TBC||First model in v2 from Toulouse 2016 VESPA workshop|
|spectro_planets||Planetary spectra||Low res, global spectra of planets and satellites. References for ground observations, provide only 1 or 2 typical spectra/object (from selected archives). Includes historical data of interest||LESIA, Erard|
√ Identify sources; currently THN library + USGS + IRTF + JSNU + occasional LESIA data
√ Convert files to documented VOtable, not fits (for use in CASSIS) - this is tricky in some cases
√ Collect complete info from original papers
Spectral calibration unchanged, not homogeneous - but solar spectra provided also
See interoperability with Planets service.
Add ephemeris from Miriad in the table (or datalink to Miriad)
|IRTF_Orton||IR telescopic images of Jupiter||Images from IRTF, Hawaii, in support of Juno||PADC/LESIA, Cecconi|
√ Get metadata from fits headers, call Miriade to compute ephemeris
|Can be used as template for collections of poorly documented observations, will retrieve ephemeris parameters on the fly||V2 draft version|
|Cassini rings||Cassini CIRS ring data||Assessment study of EPN-TAP services and VESPA infrastructure for Cassini derived data services to come.|
Final implementation will depend on strategy at mission level
|JPL (Connell, Brooks)|
|From Graz workshop, 2017|
|PSA||ESA's Planetary Science Archive|
Complete archive implemented early 2018.
~ 18 Mfiles in 2018.
Difficult on ESA side to retrieve description parameters: PDS/EPN-TAP correspondance is very much dataset dependent.
Get parameters from files/datasets?
Big issue with RPC/LAP dataset, which is more than half the files in the archive! Very slow queries because too much granules.
|v2 direct started in 2016. Uses ESA non-DaCHS server (TAP library), apparently with modifications (new fct ivo_hashlist_has not available)|
|HST||HST planetary data||Selection of planetary data (no asteroids), calibrated + products, TBC. Link to data at CADC||PADC + CADC|
|Data selection is tricky||Include ephemeris data?|
|Herschel||ESA's Herschel archive for Solar System objects||Extract from global archive? Only standard products, ie raw and pipeline (TBC)||Madrid, ESAC|
|EPN-TAP parameters ~identified - restrained in this case||(To be done on their side)|
|T1m Pic du Midi, images||IMCCE, Colas|
Would still be very nice!
• But get data first of all!
|Ephemeris can be called during ingestion, see IRTF_Orton||Use with EPN-TAP2 mixin (fits grammar) & call ephemeris from q.rd|
|Opposition of Mars 1994||LESIA, Erard|
|May be used as a first demo of complete T1m service||Processed images from Pic du Midi, calibrated & projected|
|Opposition of Mars 1999, HST||HST images from J. Bell||Larger set available on HST site? PDS GeoScienceNode has a dataset of 1999-2001 images and cubes in fits + geometry & projected versions||LESIA|
Demo for use of images + coordinates planes
Congruence with APIS (image format with geometry)
|Titan ground based observations||Historical work from the 90s only?||LESIA, Henry|
|First, recover data on old machines (from M. Combes). |
+ Also see with Athena if she has derived data to distribute
|On-going recovery project at ObsParis|
|Stellar spectra from IRTF||Vis / NIR|
|See also at ESO + Kurucz||Support for observations, use with pipeline to scale magnitudes|
|Planetary images from OHP student's obs?|
|Not favorite: unprocessed, sparse, and planetary content is limited|
|Paris library drawings|
|(TBC)||?||Database of images and simulated data to test processing methods||IPAG, Sylvain Douté|
|Data exist, to be completed||Think about new data|
|(TBC)||?||List of codes available on-line for Planetary Science||Paris ???|
|Could be based on IDIS resource list from FP7 - has to be cleaned up and modernized though. Not EPN-TAP.|
• Or instead, use github of OpenPlanetary
Potential issue with maintenance.
Would help wait for computing on demand system