Celestial reference frame (CRF) from VIE2022 VLBI solution

DOI

Celestial reference frame estimated from Very Long Baseline Interferometry (VLBI) technique measurements (1979.6 - 2023.0). VLBI global solution of S/X + VGOS 24h sessions.

GENERATION TIME:  2023-07-28T02:41:15 DATA START:  1979-08-03T00:00:00 DATA END:  2022-12-30T00:00:00 ANALYSIS CENTER:  VIE (TU Wien, Austria) CONTACT:   VIE Analysis Center (vlbi_contact@tuwien.ac.at) SOFTWARE:  VieVS v3.2 TECHNIQUE:  VLBI   FREQUENCY BANDS: S/X + VGOS FORMAT: ICRF DESCRIPTION:  CRF from the VLBI global solution S/X + VGOS, updated with additional VGOS sessions. Source positions are in the J2000 frame, but at the 2015.0 galactic aberration epoch. Reported source position errors are inflated with scaling factors:  1.5 RA,  1.5 De, and a RA/Dec noise floor 30/ 30 micro-arc-sec is applied.

Identifier
DOI https://doi.org/10.48436/264xv-kff41
Related Identifier IsVersionOf https://doi.org/10.48436/tjvn3-j8w08
Metadata Access https://researchdata.tuwien.ac.at/oai2d?verb=GetRecord&metadataPrefix=oai_datacite&identifier=oai:researchdata.tuwien.ac.at:264xv-kff41
Provenance
Creator Krasna, Hana (ORCID: 0000-0001-8660-649X)
Publisher TU Wien
Contributor Krasna, Hana; Böhm, Johannes; Böhm, Sigrid; Baldreich, Leo; Gruber, Jakob Franz; Hellerschmied, Andreas; Jaron, Frederic; Kern, Lisa; Mayer, David; Nothnagel, Axel; Panzenböck, Olivia; Wolf, Helene
Publication Year 2023
Rights Creative Commons Attribution 4.0 International; https://creativecommons.org/licenses/by/4.0/legalcode
OpenAccess true
Contact tudata(at)tuwien.ac.at
Representation
Resource Type Dataset
Version 2.0.0
Discipline Other