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  1. The birth of a telescope 30 times larger than Earth

    Dec 8, 2011 · The detection was made on 15 November 2011, with observations performed at a wavelength of 18 centimeters and targeting bright and extremely compact radio emission from …

  2. The successful detection of interference fringes demonstrates the overall excellent status of the complex system and reflects the birth of the new international ground-to-space very long …

  3. The detection was made on 15 November 2011, with observations performed at a wavelength of 18 centimeters and targeting bright and extremely compact radio emission from the distant …

  4. First fringes for the RadioAstron project were already detected using the Effelsberg 100 m telescope and the ASC correlator in 2011 and presented in an earlier press release.

  5. en meter dish in a highly elliptical orbit with an eight to nine day period. RadioAstron works together with Earth based radio telescopes to give interferometer baselines extending up to …

  6. The aim of the RadioAstron project was to make it possible to obtain a record-high angular resolution of a few micro-arcseconds, orders of magnitude higher resolution than was …

  7. Russian RadioAstron (Spectr-R) update - NASASpaceFlight.com

    Jun 30, 2013 · The RadioAstron survey of active galactic nuclei in all frequency bands continues. The record is being set so far by a detection of the active galaxy OJ287 at 6 cm with the SRT …

  8. Interference signal from the quasar 0212+735 on a 8,100 km projected baseline between RadioAstron and the 100-m MPIfR radio telescope near Effelsberg, Germany, observed on …

  9. Residual fringe rate vs delay diagram showing the interferometric fringe signal from the quasar 0212+735 on a 100,000 km baseline between RadioAstron and the 100m radio telescope in …

  10. The birth of a Radio Telescope 30 times larger than Earth

    Artist's impression of Spektr-R, the 10-meter space-borne antenna of the RadioAstron project. Credit: Lavochkin Association.