ARI katkat is a catalog of star catalogues in the spirit of G. Teleki's catalog of star catalogs (`1989BOBeo.140..131T`_ and references in there). It contains 2573 catalogs suitable for astrometric usage, starting with Flamsteed (1835) and ending in the 1970ies. For almost all of them, there is a column description file (as PDF, and unfortunately sometimes in German) and the digitized content. .. _1989BOBeo.140..131T: http://ads.g-vo.org/abs/1989BOBeo.140..131T
EPN-TAP access to rasdaman M3 database.
CRISM data from Planet Server 2: http://access.planetserver.eu/
This catalogue is a simulation of the Gaia DR2 stellar content using Galaxia (a tool to sample stars from a Besancon-like Milky Way model), 3d dust extinction maps and the latest PARSEC Isochrones. It is mimicking the Gaia DR2 data model and an apparent magnitude limit of g=20,7. Extinctions and photometry in different bands have also been included in a supplementary table as well as uncertainty estimates using a scaled nominal error model.
This web application is a compilation of all the published data collected by the U.S. Geological Survey (USGS) St. Petersburg Coastal and Marine Science Center. Data includes sediment, drill, and coral cores and samples, bathymetry data extents, seismic data extents, seismic tracklines, bathymetry tracklines, interferometric swath bathymetry digital elevation models (DEMs), single-beam and swath bathymetry combination DEMs, single-beam bathymetry DEMs, and side-scan sonar mosaics.
A catalogue of E(V-I) extinction values is presented for 3174 (LMC) and 693 (SMC) fields within the Magellanic Clouds. The extinction values were computed by determining the (V-I) colour difference of the red clump from Optical Gravitational Microlensing Experiment (OGLE III) observations in the V and I bands and theoretical values for unreddend red clump colours.
Differences between USNO-B and PPMXL in positions and proper motions, on an all-sky one-degree grid. At each gridpoint we give the differences X(PPMXL)- X(USNO-B1.0) averaged over all stars in a sqrt(2)/2-degrees environment around the gridpoint given. The corrections given here should bring USNO-B based astrometry to the ICRS.
A Duna-Ipoly National Park Directorate's (DINPI) species occurrence database.
Interpretive data release for Oregon OCS Seafloor Mapping: Selected Lease Blocks Relevant to Renewable EnergyGuy R. Cochrane
This data release includes the results of analysis of video data conducted by Oregon State University and the geo-habitat interpretation of multibeam echo sounder (MBES) data conducted by the USGS. The data were collected in 2014 and were published in Cochrane and others (2015). This data release accompanies report that describes the project and results in detail (Cochrane and others, 2017). All the data are provided as geographic information system (GIS) files that contain both...
A time integrated search for point sources of cosmic neutrinos was performed using the data collected from January 2007 to November 2012 by the ANTARES neutrino telescope. This dataset includes a total of 5921 events obtained during the effective livetime of 1338 days.
OpenNGC is a database containing positions and main data of NGC (New General Catalogue) and IC (Index Catalogue) objects. It has been built by merging data from NED, HyperLEDA, SIMBAD, and several databases available at HEASARC. In this VO publication, we have changed most of the column names, mostly to make them work as ADQL column names without resorting to delimited identifiers. The mapping should be obvious.
This service publishes plate scans of the Palomar-Leiden Troian surveys conducted between 1960 and 1977. The surveys led to the discovery of more than 2,000 asteroids (1,800 with orbital information), with another 2,400 asteroids, including 19 Trojans, found after further analysis of the plates. Note that because of the large size of the plates, in this service each original plate is contained in two parts, marked with "_1" and "_2", respectively. The central parts of...
Department of Infectious Diseases, Imperial College London running two high performance clusters on a Microsoft HPC platform
3D visualization and virtual reality Center based in the School of Energy Resources, supporting teaching and research at the University of Wyoming, and offering professional technology services and digital asset creation to the wider community. The $3M technology infrastructure includes a 3D CAVE, virtual reality head mounted displays, and augmented reality devices.
This service provides oscillator strengths and transition probabilities. Mainly based on experimental energy levels, these were calculated with the pseudo-relativistic Hartree-Fock method including core-polarization corrections.
The Cheyenne system delivers supercomputing capabilities that are central to fulfilling NCAR's mission, including support for climate modeling, weather forecasting, and other critical research in the atmospheric, oceanic, and related sciences. Cheyenne is a 5.34-petaflops SGI ICE XA cluster with 4,032 dual-socket nodes, each with Intel Xeon E5-2697V4 (Broadwell) 2.3-GHz, 18-core processors, for a total of 145,152 processor cores. The system has DDR4-2400 memory, with 3,168 nodes having 64 GB and 864 nodes having 128...
Justin updated this on 4/4 at 2:46 PM
USGS DOI Tool Production Environment29
Zentrum für Astronomie der Universität Heidelberg14
National Center for Atmospheric Research (NCAR)3
Imperial College London1
Istituto Nazionale di Geofisica e Vulcanologia1
King's College London1
Landcare Research New Zealand Ltd1
UTA Institute of Classical Archaeology1