Subject: stars / Capability Type: VOSI Availability - STScI NAVO Directory Search Results

ID:: ivo://asu.cas.cz/extract_jul16/q/ssa
Title:: DK-154 objects
Short Name:: DK-154 LCs
Date:: 19 May 2017 01:42:07
Publisher:: Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
Description:: DK-154 SSAP interpreted lightcurves

ID:: ivo://asu.cas.cz/extract_apr18/q/ssa
Title:: DK-154 objects
Short Name:: DK-154 LCs
Date:: 18 Apr 2018 11:50:00
Publisher:: Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
Description:: DK-154 SSAP interpreted lightcurves

ID:: ivo://asu.cas.cz/extract_jan18/q/ssa
Title:: DK-154 objects
Short Name:: DK-154 LCs
Date:: 08 Jan 2018 15:30:12
Publisher:: Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
Description:: DK-154 SSAP interpreted lightcurves

ID:: ivo://asu.cas.cz/extract_dec17/q/ssa
Title:: DK-154 objects
Short Name:: DK-154 LCs
Date:: 08 Jan 2018 15:30:12
Publisher:: Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
Description:: DK-154 SSAP interpreted lightcurves

ID:: ivo://asu.cas.cz/extract_jan16/q/ssa
Title:: DK-154 objects
Short Name:: DK-154 LC
Date:: 30 Nov 2017 09:39:26
Publisher:: Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
Description:: SSAP interpreted lightcurves

ID:: ivo://org.gavo.dc/gdr2dist/q/cone
Title:: Estimated distances to 1.33 billion stars in Gaia DR2
Short Name:: gdr2dist scs
Date:: 27 Dec 2024 08:31:05
Publisher:: The GAVO DC team
Description:: This catalogue provides distances estimates (and uncertainties therein) for 1.33 billion stars over the whole sky brighter than about G=20.7. These have been estimated using the parallaxes (and their uncertainties) from Gaia DR2. A Bayesian procedure was used involving a prior with a single parameter L(l,b), which varies smoothly with Galactic longitude and latitude according to a Galaxy model. The posterior is summarized with a point estimate (usually the mode) and a confidence interval (usually the 68% highest density interval). The estimation procedure is described in detail in the `accompanying paper`_, which also analyses the catalogue content. .. _accompanying paper: http://www.mpia.de/homes/calj/gdr2_distances.html

ID:: ivo://org.gavo.dc/gaia/q2/dr2lcone
Title:: Gaia DR2-light Cone Search
Short Name:: GDR2light SCS
Date:: 27 Dec 2024 08:31:02
Publisher:: The GAVO DC team
Description:: This schema contains data re-published from the official Gaia mirrors (such as ivo://uni-heidelberg.de/gaia/tap) either to support combining its data with local tables (the various Xlite tables) or to make the data more accessible to VO clients (e.g., epoch fluxes). Other Gaia-related data is found in, among others, the gdr2dist, gdr3mock, gdr3spec, gedr3auto, gedr3dist, gedr3mock, and gedr3spur schemas.

ID:: ivo://org.gavo.dc/gaia/q2/ssa
Title:: Gaia DR2 light curves SSA
Short Name:: GDR2 TS SSAP
Date:: 27 Dec 2024 08:31:02
Publisher:: The GAVO DC team
Description:: This service exposes about 0.5 million light curves of stars classified as variable by the Gaia analysis system through the VO SSAP protocol. The lightcurves are published per-band and are also available through obscore.

ID:: ivo://xaovo/gaia/q3/cone
Title:: Gaia DR3 Lite Cone Search
Short Name:: DR3 lite Cone
Date:: 25 Jun 2024 10:32:03
Publisher:: Xinjiang Astronomical Observatory,CAS
Description:: This schema contains data re-published from the official Gaia mirrors (such as ivo://uni-heidelberg.de/gaia/tap) either to support combining its data with local tables (the various Xlite tables) or to make the data more accessible to VO clients (e.g., epoch fluxes).

ID:: ivo://org.gavo.dc/gaia/q3/cone
Title:: Gaia DR3 Lite Cone Search
Short Name:: DR3 lite Cone
Date:: 27 Dec 2024 08:31:03
Publisher:: The GAVO DC team
Description:: This schema contains data re-published from the official Gaia mirrors (such as ivo://uni-heidelberg.de/gaia/tap) either to support combining its data with local tables (the various Xlite tables) or to make the data more accessible to VO clients (e.g., epoch fluxes). Other Gaia-related data is found in, among others, the gdr3mock, gdr3spec, gedr3auto, gedr3dist, gedr3mock, and gedr3spur schemas.

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