31,478 datasets found

The Mars Crater Catalog by S.J. Robbins was generated from THEMIS Daytime IR and Viking MDIM 2.1 global mosaics of Mars. Craters were selected using 5 points along the rim. The...

The publishing registry for the PADC TAP Server on voparis-tap-astro.obspm.fr.

Lunar crater catalogue

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...

Mercury crater catalogue

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...

Catalogue of USGS Astrogeology WMS Map Layers

"The growth of the Tharsis volcanic complex on Mars during Noachian/Hesperian era induced a reorientation of the spin axis of the planet (true polar wander). This service gives...

The GEOPS/IPSL DaCHS Server's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own...

"The data consists in topographic maps of synthetic 3D bodies generated by a 3 parameters statistical model : the fractionally integrated flux (FiF) (Lavallee, D., Lovejoy, S.,...

The publishing registry for the GEOPS/IPSL DaCHS Server.

Spitzer Taurus access

The Wisconsin Ultraviolet Photo-Polarimeter Experiment (WUPPE) was the spectropolarimetry component of the three ASTRO instruments that flew on Space Shuttle missions in...

The ERO programme is an initiative of ESA and the Euclid Science Team: it includes one day of observations, taken before the start of the nominal survey, to showcase the...

The Euclid Q1 data release encompasses ?65 deg2 and contains the VIS and NIR data of one pass on each of the three Euclid deep fields (EDF-North, EDF-South, and EDF-Fornax), as...

In the austral winters of 2016 and 2017, we used the AST3-II telescope located at the Chinese Kunlun station at Dome A, Antarctica to survey a group of selected fields near the...

The KiDZ data are complementary to the main Kilo-Degree (KIDS) survey, and specifically target fields with extensive deep spectroscopy. They are primarily intended for the...

The ERO programme is an initiative of ESA and the Euclid Science Team: it includes one day of observations, taken before the start of the nominal survey, to showcase the...

In the austral winters of 2016 and 2017, we used the AST3-II telescope located at the Chinese Kunlun station at Dome A, Antarctica to survey a group of selected fields near the...

The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in. Original acknowledgement...