Publisher: The GAVO DC team / Capability Type: Table Access Protocol

ID:: ivo://org.gavo.dc/mwsc/q/clu
Title:: MWSC Star Cluster Search
Short Name:: MWSC clusters
Date:: 27 Dec 2024 08:31:04
Publisher:: The GAVO DC team
Description:: MWSC presents a list of 3006 Milky Way Stellar Clusters (MWSC), found in the 2MAst (2MASS with Astrometry) catalogue. The target list was compiled on the basis of present-day lists of open, globular and candidate clusters. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, mean cluster proper motions, distances, reddenings, ages, tidal parameters, and sometimes radial velocities.

ID:: ivo://org.gavo.dc/obscode/q/query
Title:: Observatory Codes
Short Name:: obscode_web
Date:: 27 Dec 2024 08:31:05
Publisher:: The GAVO DC team
Description:: List of Observatory Codes assigned by the Minor Planet Center (MPC). The codes are used in cataloguing astrometric observations of small bodies in the solar system. A code is unique for a certain location and consists of three digits or one letter and two digits. In this representation, we give the observatory code, the geocentric coordinates, and the observatory designation.

ID:: ivo://org.gavo.dc/openngc/q/web
Title:: OpenNGC
Short Name:: openNGC
Date:: 27 Dec 2024 08:31:01
Publisher:: The GAVO DC team
Description:: 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.

ID:: ivo://org.gavo.dc/polcatsmc/q/cone
Title:: Optical Polarimetric Catalog for the SMC
Short Name:: PolCatSMC
Date:: 27 Dec 2024 08:31:13
Publisher:: The GAVO DC team
Description:: An optical polarimetric catalog for the Small Magelanic Cloud (SMC) is presented. It gives intrinsic and observed polarizations in the V-band for a total of 7207 stars located in the Northeast and Wing sections of the SMC and part of the Magellanic Bridge.

ID:: ivo://org.gavo.dc/xpparams/q/cone
Title:: Parameters of 220 million stars from Gaia BP/RP (XP) spectra
Short Name:: XP ap-pars
Date:: 27 Dec 2024 08:31:01
Publisher:: The GAVO DC team
Description:: We present astrophysical parameters of 220 million stars, based on Gaia XP spectra and near-infrared photometry from 2MASS and WISE. Instead of using ab initio stellar models, we develop a data-driven model of Gaia XP spectra as a function of the stellar parameters, with a few straightforward built-in physical assumptions. This resource is a VO re-publication of the resulting catalog of stellar parameters. For bulk downloads, the covariances, the trained model, and more, see https://zenodo.org/record/7811871.

ID:: ivo://org.gavo.dc/cs82morphoz/q/cone
Title:: Photometric redshifts in Stripe 82
Short Name:: CS82 cone
Date:: 27 Dec 2024 08:31:06
Publisher:: The GAVO DC team
Description:: This is a catalogue of photometric redshifts of galaxies in the Stripe 82 obtained when morphology (galaxy size, ellipticity, Sérsic index, and surface brightness) are included in training on galaxy samples from the SDSS and the CFHT Stripe-82 Survey (CS82). Our redshifts yield a 68th percentile error of 0.058(1 + z), and a outlier fraction of 5.2 per cent.

ID:: ivo://org.gavo.dc/auger/q/cone
Title:: Pierre Auger Observatory public data
Short Name:: auger_scs
Date:: 27 Dec 2024 08:31:06
Publisher:: The GAVO DC team
Description:: This dataset comprises the public data observed by the Pierre Auger cosmic ray observatory, which is 1% of its total data. It contains 28493 events between 0.1 and 49.7 EeV collected between 2004 and 2013.

ID:: ivo://org.gavo.dc/auger/q3/pub
Title:: Pierre Auger Observatory public DR3
Date:: 06 Sep 2024 11:23:49
Publisher:: The GAVO DC team
Description:: The Pierre Auger Open Data is the public release of 10% of the Pierre Auger Observatory cosmic-ray data published in recent scientific papers and at International conferences. The Pierre Auger Observatory, located on a vast, high-altitude plain in the Province of Mendoza in Argentina, is the world's largest cosmic ray observatory and measures the extensive air-showers produced by cosmic rays above ~1e17 eV. Here, we include data from the two surface detector (SD) setups, SD750 and SD1500, as well as the flourescence detectors (FD). For both of these, we also host the full json event descriptors. In addition there is a table of highly inclined events and the scaler readouts. See also the portal page https://opendata.auger.org.

Search