|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|
|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 afterwards)
Add daily cycles and planes? Add more scenarios.
|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.
|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|
|Cometary 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|
|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?||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, Christophe Ordenovich|
|Relies on TAPlib - interface study by PLS in July that year||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|
Pangaea-X 2017 data
|Various measurements on planetary analogue environment||JacobsUni|
|Finalize, ingest other data||First assessment with drone images|
|Various db from Brown University||see here http://www.planetary.brown.edu/html_pages/data.htm|
|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.|
|?||Berlin Emissivity Spectral Library||Laboratory spectroscopy of mineral samples in support of MERTIS/BepiColombo, and more||DLR, Helbert / Maturilli|
To be implemented as Europanet TNAs
To be derived from BRSL?
|Use mixin/CSV grammar|
Spectroscopy of ices and minerals
|Spectro / sample descriptors required.||To be integrated in SSHADE|
Spectroscopy of ices and minerals
|Spectro / sample descriptors required.||Includes ~ 20 evolving databases. Regular update required.|
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|
|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|
|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|
|Review and finalize |
Check consistency with CLIMSO (service includes some CLIMSO data)
|Complete draft on-line, unpublished (May 2017)|
|Radio Solar Database||Radio Solar Database||From Nançay||PADC|
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.
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.|
|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||JPL (Connell, Brooks)|
|Assessment study of EPN-TAP services and VESPA infrastructure for Cassini derived data services to come.||From Graz workshop|
|PSA||ESA's Planetary Science Archive||Madrid, ESAC|
Get parameters from files / datasets.
Start with a test on a simple dataset? AMIE / Smart-1 or Navcam / Rosetta would do - or possibly VEx for a larger service.
|v2 direct. Uses ESA non-DaCHS server (TAPlib)|
|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.|
|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.|
• Or instead, use github of OpenPlanetary
Potential issue with maintenance.
Would help wait for computing on demand system