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hal.structure.identifierSupélec Sciences des Systèmes [E3S]
dc.contributor.authorJACOBS, Christopher S.,
dc.contributor.authorARIAS, F.,
dc.contributor.authorBOEHM, J.,
dc.contributor.authorBOLOTIN, S.,
hal.structure.identifierM2A 2014
dc.contributor.authorBOURDA, G.
hal.structure.identifierM2A 2014
dc.contributor.authorCHARLOT, P.
dc.contributor.authorDE WITT, A.,
dc.contributor.authorFEY, A.,
hal.structure.identifierLaboratoire de Chimie Appliquée de l'État Solide [LCAES]
dc.contributor.authorGAUME, R.,
hal.structure.identifierFlinders Medical Centre
dc.contributor.authorGORDON, D.,
dc.contributor.authorHEINKELMANN, R.,
dc.contributor.authorKURDUBOV, S.,
hal.structure.identifierParis-Jourdan Sciences Economiques [PSE]
hal.structure.identifierParis School of Economics [PSE]
dc.contributor.authorLAMBERT, S.,
hal.structure.identifierLaboratoire de synthèse organique [DCSO]
dc.contributor.authorMA, C.,
hal.structure.identifierPulkovo Observatory
dc.contributor.authorMALKIN, Z.,
dc.contributor.authorNOTHNAGEL, A.,
dc.contributor.authorSEITZ, M.,
dc.contributor.authorSKURIKHINA, E.,
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorSOUCHAY, J.,
dc.contributor.authorTITOV, O.,
dc.date.issued2014-10
dc.date.conference2013-09-16
dc.description.abstractEnICRF-3 seeks to improve upon the highly successful ICRF-2. Our goals are to improve the precision, spatial and frequency coverage relative to the ICRF-2 by 2018. This date is driven by the desire to create radio frames that are ready for comparison with the Gaia optical frame.Several specific actions are underway. A collaboration has started to improve at S/X-band precision of the VLBA Calibrator Survey's ~2200 sources which are typically 5 times less precise than the rest of the ICRF-2. S/X-band southern precision improvements are underway with observations using southern antennas such as the AuScope and HartRAO, S. Africa.We also seek to improve radio frequency coverage with X/Ka and K-band work. An X/Ka frame of 654 sources now has full sky coverage from the addition of a 2nd southern station in Argentina which should strengthen the southern hemisphere in general. A K-band collaboration has formed with similar coverage and southern precision goals.On the analysis front, special attention is being given to combination techniques both of VLBI frames and of multiple data types. Consistency of the CRF with the TRF and EOP is another area of concern. Comparison of celestial frame solutions from various groups is underway in order to identify and correct systematic errors.Finally, work is underway to identify and pinpoint sources bright enough in both radio and optical to allow for a robust frame tie between VLBI and Gaia optical frames.
dc.language.isoen
dc.subject.enCelestial Reference Frame
dc.subject.enICRF
dc.subject.enICRF-3
dc.subject.enastrometry
dc.subject.enVLBI
dc.subject.enS/X-band
dc.subject.enK-band
dc.subject.enX/Ka-band
dc.subject.enActive Galactic Nuclei
dc.title.enThe ICRF-3: Proposed Roadmap to the Next Generation International Celestial Reference Frame
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.page1
bordeaux.conference.titleProceedings of Reference Frames for Astrometry and Geodesy 2014, 34 pp.
bordeaux.countryFR
bordeaux.conference.cityParis
bordeaux.peerReviewedoui
hal.identifierhal-01110513
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01110513v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2014-10&rft.spage=1&rft.epage=1&rft.au=JACOBS,%20Christopher%20S.,&ARIAS,%20F.,&BOEHM,%20J.,&BOLOTIN,%20S.,&BOURDA,%20G.&rft.genre=unknown


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