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dc.contributor.authorFEY, A. L.,
dc.contributor.authorGORDON, D.,
dc.contributor.authorJACOBS, C. S.,
hal.structure.identifierCardiology Division [Cardio Div - BEIJING]
dc.contributor.authorMA, C.,
hal.structure.identifierLaboratoire de Chimie Appliquée de l'État Solide [LCAES]
dc.contributor.authorGAUME, R. A.,
dc.contributor.authorARIAS, E. F.,
dc.contributor.authorBIANCO, G.,
dc.contributor.authorBOBOLTZ, D. A.,
dc.contributor.authorBOCKMANN, S.,
dc.contributor.authorBOLOTIN, S.,
hal.structure.identifierM2A 2016
dc.contributor.authorCHARLOT, P.
hal.structure.identifierM2A 2016
dc.contributor.authorCOLLIOUD, A.
dc.contributor.authorENGELHARDT, G.,
dc.contributor.authorGIPSON, J.,
hal.structure.identifierLaboratoire d'Hydrologie et de Géochimie de Strasbourg [LHyGeS]
dc.contributor.authorGONTIER, A.-M.,
dc.contributor.authorHEINKELMANN, R.,
dc.contributor.authorKURDUBOV, S.,
hal.structure.identifierScience et Technologie du Lait et de l'Oeuf [STLO]
dc.contributor.authorLAMBERT, S.,
dc.contributor.authorLYTVYN, S.,
dc.contributor.authorMACMILLAN, D. S.,
hal.structure.identifierPulkovo Observatory
dc.contributor.authorMALKIN, Z.,
dc.contributor.authorNOTHNAGEL, A.,
dc.contributor.authorOJHA, R.,
dc.contributor.authorSKURIKHINA, E.,
dc.contributor.authorSOKOLOVA, J.,
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorSOUCHAY, J.,
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorSOVERS, O. J.,
dc.contributor.authorTESMER, V.,
dc.contributor.authorTITOV, O.,
hal.structure.identifierLaboratoire Matériaux et Phénomènes Quantiques [MPQ (UMR_7162)]
dc.contributor.authorWANG, G.,
dc.contributor.authorZHAROV, V.,
dc.date.issued2016-01
dc.description2016yCat..51500058F - VizieR On-line Data Catalog: J/AJ/150/58. Originally published in: 2015AJ....150...58F
dc.description.abstractEnWe present the second realization of the International Celestial Reference Frame (ICRF2) at radio wavelengths using nearly 30 years of Very Long Baseline Interferometry observations. The earliest observations used are from 1979 August and the latest are from 2009 March. ICRF2 consists of accurate positions of 295 new "defining" sources and positions of 3119 additional compact radio sources to densify the frame. ICRF2 has more than 5 times as many sources as ICRF1 (Ma et al. 1997, cat. I/251), is roughly 5-6 times more accurate, and is nearly twice as stable in the orientation of its axes.(3 data files).
dc.language.isoen
dc.typeAutre document
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
hal.identifierhal-01272526
hal.version1
hal.popularnon
dc.title.itVizieR Online Data Catalog: VLBI ICRF2 (Fey+, 2015)
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01272526v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2016-01&rft.au=FEY,%20A.%20L.,&GORDON,%20D.,&JACOBS,%20C.%20S.,&MA,%20C.,&GAUME,%20R.%20A.,&rft.genre=unknown


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