| basecom.epn_core | Table Info | 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. | 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. |
| bass2000.epn_core | Table Info | Solar survey archive: Images, movies of full Sun from groundbased
instruments: Spectroheliographs of Meudon and Coimbra, RadioHeliograph
and Decametric Array of Nancay, CLIMSO, USET | BASS2000 archives and distributes groundbased solar observations
provided by various instruments: the RadioHeliographe and Decametric
Array of Nancay, Spectroheliographes of Meudon and Coimbra, CLIMSO,
the Coronographe of Pic du Midi, the Uccle Solar Equatorial Table
(USET). It is also WDC-Solar Activity, Regular Member of ICSU World
Data system. |
| cadc.epn_core | Table Info | TBD. | TBD. |
| cadc_test3.epn_core | Table Info | TBD. | TBD. |
| cadc_test6.epn_core | Table Info | TBD. | TBD. |
| cadc_test7.epn_core | Table Info | TBD. | TBD. |
| cta.vo_obscore | Table Info | CTA run obscore | fill in |
| das2meudon.epn_core | Table Info | Obs. Paris Das2 Server service catalog | Obs. Paris Das2 Server service catalog |
| das2meudon_datalink.epn_core | Table Info | Das2 Server Meudon database. | Das2 Server Meudon database. |
| das2uiowa.epn_core | Table Info | Das2 Server at University of Iowa database. | Das2 Server at University of Iowa database. |
| dfbs.frames | Table Info | The Digitized First Byurakan Survey (DFBS) is the digitized version of
the famous Markarian survey, called also the First Byurakan Survey
(FBS). | The Digitized First Byurakan Survey (DFBS) is the digitized version of
the famous Markarian survey, called also the First Byurakan Survey
(FBS). |
| exotopo.epn_core | Table Info | DESCRIPTION | DESCRIPTION |
| expres.epn_core | Table Info | ExPRES Simulation service catalog | ExPRES Simulation service catalog |
| herschel.epn_core | Table Info | Solar System observations observed with the ESA/Herschel space
observatory. The current data has been extracted from the Herschel
ESDC search interface (http://archives.esac.esa.int/hsa/whsa/#search),
with the AQDL search query set to `global_science_area LIKE 'Solar
System'`. | Solar System observations observed with the ESA/Herschel space
observatory. The current data has been extracted from the Herschel
ESDC search interface (http://archives.esac.esa.int/hsa/whsa/#search),
with the AQDL search query set to `global_science_area LIKE 'Solar
System'`. |
| hess.vo_lightcurve | Table Info | HESS lightcurves | fill in |
| hess.vo_obscore | Table Info | HESS obscore | fill in |
| hess.vo_spectrum | Table Info | HESS spectra | fill in |
| hess2.data | Table Info | N/A | N/A |
| hess_dr.vo_obscore | Table Info | ObsCore description of event lists for observations in the H.E.S.S.
DL3 public test data release 1 | The release consists of event lists and instrument response functions
for observations of various well-known gamma-ray sources (the Crab
nebula, PKS 2155-304, MSH 15-52, RX J1713.7-3946) as well as
observations of empty fields for background modeling. |
| hess_ssa.data | Table Info | ___ | ___ |
| hst_planeto.epn_core | Table Info | HST observations of planets, dwarf planets, and satellites, extracted
from the CADC database catalogue (regularly updated). 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. | HST observations of planets, dwarf planets, and satellites, extracted
from the CADC database catalogue (regularly updated). 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_core | Table Info | 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] | 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] |
| iks2.epn_core | Table Info | 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] | 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] |
| irtf_juno.epn_core | Table Info | NASA IRTF NIR Jupiter Observations in suport of the NASA/JUNO
mission. | NASA IRTF NIR Jupiter Observations in suport of the NASA/JUNO
mission. |
| ivoa.ObsCore | Table Info | The IVOA-defined obscore table, containing generic metadata for
datasets within this datacenter. | Definition and support code for the ObsCore data model and table. |
| Tablename | Info | Table desc. | Res desc. |
|---|
| luckystar.epn_core | Table Info | Draft version from catalogue date found here:
http://occultations.ct.utfpr.edu.br/results/ | Draft version from catalogue date found here:
http://occultations.ct.utfpr.edu.br/results/ |
| lunar_crater_database.epn_core | Table Info | Catalog of lunar impact craters, with properties, from Losiak et al,
2009 A New Lunar Impact Crater Database, 2009LPI....40.1532L.
Available at
https://www.lpi.usra.edu/lunar/surface/Lunar_Impact_Crater_Database_v08Sep2015.xls | Catalog of lunar impact craters, with properties, from Losiak et al,
2009 A New Lunar Impact Crater Database, 2009LPI....40.1532L.
Available at
https://www.lpi.usra.edu/lunar/surface/Lunar_Impact_Crater_Database_v08Sep2015.xls |
| pds_speclib.epn_core | Table Info | This service provides a VO version of the PDS spectral library,
distributed by the PDS Geosciences node:
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 | This service provides a VO version of the PDS spectral library,
distributed by the PDS Geosciences node:
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 |
| planets.epn_core | Table Info | Main characteristics of planets. Data are included in the table,
therefore most relevant parameters are non-standard in EPN-TAP. 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]. | Main characteristics of planets. Data are included in the table,
therefore most relevant parameters are non-standard in EPN-TAP. 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]. |
| planets2.epn_core | Table Info | Demonstration service of EPN-TAP v1: main characteristics of planets.
Data are included in the table, therefore most relevant parameters are
non-standard in EPN-TAP. Data are retrieved from Archinal et al 2009
(IAU report, 2011CeMDA.109..101A) [radii] and Cox et al 2000 (Allen's
astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric
distances, and rotation periods]. | Demonstration service of EPN-TAP v1: main characteristics of planets.
Data are included in the table, therefore most relevant parameters are
non-standard in EPN-TAP. Data are retrieved from Archinal et al 2009
(IAU report, 2011CeMDA.109..101A) [radii] and Cox et al 2000 (Allen's
astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric
distances, and rotation periods]. |
| profils.epn_core | Table Info | temperature pressure and element abundancy in planetary atmosphere. | |
| pspecf.epn_core | Table Info | %this should be a paragraph or two (take care to mention salient
terms)% | %this should be a paragraph or two (take care to mention salient
terms)% |
| sbnaf.epn_core | Table Info | blabla | blabla |
| spectro.epn_core | Table Info | Murchie et al (2007) Compact Reconnaissance Imaging Spectrometer for
Mars (CRISM) on Mars Reconnaissance Orbiter (MRO). JGR Planets,
112:E05S03. | Murchie et al (2007) Compact Reconnaissance Imaging Spectrometer for
Mars (CRISM) on Mars Reconnaissance Orbiter (MRO). JGR Planets,
112:E05S03. |
| spectro_asteroids.epn_core | Table Info | 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. | 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_core | Table Info | 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. | 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. |
| spectro_planets2.epn_core | Table Info | 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.
Version with parameters retreived from ephemeris. | 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.
Version with parameters retreived from ephemeris. |
| spectro_planets3.epn_core | Table Info | 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.
Ephemeris data are retrieved from Miriade (IMCCE) for the reference
date (but some spectra are actually composite); C1/C2 provide location
of disk center; s_region provides the visible hemisphere (not
necessarily illuminated). | 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.
Ephemeris data are retrieved from Miriade (IMCCE) for the reference
date (but some spectra are actually composite); C1/C2 provide location
of disk center; s_region provides the visible hemisphere (not
necessarily illuminated). |
| tap_schema.columns | Table Info | Columns in tables available for ADQL querying. | PADC TAP Server on voparis-cdpp-new.obspm.fr's Table Access Protocol (TAP) service with
table metadata. |
| tap_schema.groups | Table Info | Columns that are part of groups within tables available for ADQL
querying. | PADC TAP Server on voparis-cdpp-new.obspm.fr's Table Access Protocol (TAP) service with
table metadata. |
| tap_schema.key_columns | Table Info | Columns participating in foreign key relationships between tables
available for ADQL querying. | PADC TAP Server on voparis-cdpp-new.obspm.fr's Table Access Protocol (TAP) service with
table metadata. |
| tap_schema.keys | Table Info | Foreign key relationships between tables available for ADQL querying. | PADC TAP Server on voparis-cdpp-new.obspm.fr's Table Access Protocol (TAP) service with
table metadata. |
| tap_schema.schemas | Table Info | Schemas containing tables available for ADQL querying. | PADC TAP Server on voparis-cdpp-new.obspm.fr's Table Access Protocol (TAP) service with
table metadata. |
| tap_schema.tables | Table Info | Tables available for ADQL querying. | PADC TAP Server on voparis-cdpp-new.obspm.fr's Table Access Protocol (TAP) service with
table metadata. |
| titan.epn_core | Table Info | temperature pressure and element abundancy in planetary atmosphere. | |
| tnosarecool.epn_core | Table Info | This service lists TNO thermal properties as derived mostly from
Spitzer and Herschel observations | This service lists TNO thermal properties as derived mostly from
Spitzer and Herschel observations. |
| vims.epn_core | Table Info | TBD ex: The Visual and Infrared Mapping Spectrometer (VIMS)
instrument onboard the Cassini spacecraft successfully imaged its
surface in the atmospheric windows, taking hyperspectral images in the
range 0.4 5.2 microns. | TBD ex: The Visual and Infrared Mapping Spectrometer (VIMS)
instrument onboard the Cassini spacecraft successfully imaged its
surface in the atmospheric windows, taking hyperspectral images in the
range 0.4 5.2 microns. |
| vims_satellites.epn_core | Table Info | TBD ex: The Visual and Infrared Mapping Spectrometer (VIMS)
instrument onboard the Cassini spacecraft successfully imaged its
surface in the atmospheric windows, taking hyperspectral images in the
range 0.4 5.2 microns. | TBD ex: The Visual and Infrared Mapping Spectrometer (VIMS)
instrument onboard the Cassini spacecraft successfully imaged its
surface in the atmospheric windows, taking hyperspectral images in the
range 0.4 5.2 microns. |
| vvex.epn_core | Table Info | IR spectroscopy of Venus | VIRTIS/Venus Express demonstrator service: imaging spectroscopy of
Venus in the visible and the near infrared. This lists all the
calibrated files from the nominal mission for the three channels
M-vis, M-IR and H. Files are described according to the extended index
in the PSA archive, with links to the PSA:
ftp://psa.esac.esa.int/pub/mirror/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. |
| vvex_db.epn_core | Table Info | IR 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. |
| Tablename | Info | Table desc. | Res desc. |
|---|
| vvex_db0.epn_core | Table Info | IR 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. |
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