2008/01/31 by S. Frey, Leonid Gurvits, Frey, S. +8
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Radio Astronomy Observations and Technology #astro-ph
paper · pdf · doi:10.48550/arxiv.0801.4864
3 pages; proceedings of the symposium "Approaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technology" (ISAS/JAXA, Sagamihara, Japan, 3-7 Dec 2007). Astronomical Society of the Pacific Conference Series, eds. Hagiwara Y., Fomalont E.B., Tsuboi M., Murata Y., in press
arxiv created 2008/01/31 · openalex publication_date 2008/01/31 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We studied the radio structure of high-redshift (z>3) quasars with VSOP at 1.6 and 5 GHz. These sources are the most distant objects ever observed with Space VLBI, at rest-frame frequencies up to ~25 GHz. Here we give an account of the observations and briefly highlight the most interesting cases and results. These observations allowed us, among other things, to estimate the mass of the central black holes powering these quasars, to identify large misalignments between the milli-arcsecond (mas) and sub-mas scale radio structures, and to detect apparent superluminal motion at sub-mas scale.