397 datasets found

Keywords: interferometry

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  • P Cyg H{alpha} squared visibility

    High spatial resolution observations of the H{alpha}-emitting wind structure associated with the luminous blue variable star P Cygni were obtained with the Navy Prototype...
  • Anatomy of L1489 IRS with NOEMA I

    Over the past few years, chemical studies have revealed multiple structures in the vicinity of young stellar objects (YSOs). It has become evident that specific physical...
  • Molecular ion abundances in diffuse ISM

    The transition between atomic and molecular hydrogen is associated with important changes in the structure of interstellar clouds, and marks the beginning of interstellar...
  • GMVA 86GHz Stokes IQU images of 3C84 jet

    We report results from a deep polarization imaging of the nearby radio galaxy 3C 84 (NGC 1275). The source was observed with the Global Millimeter VLBI Array (GMVA) at 86GHz at...
  • Astrometric classification of 647 VLBI sources

    We present the result of our Allan standard deviation based classification according to their astrometric stability. The classification is divided into three categories (stable...
  • Binary stars: visual orbits & interferometry

    Knowledge of the orbits of visual binary stars has always been one of the fundamentals of astronomy. Based historically on the visual measures, nowadays the orbits rely more (or...
  • Interferometer phase calibration sources

    The catalogue contains compact radio sources with accurate positions observed with the Very Large Array (VLA). These sources are primarily intended for use as phase calibration...
  • GLEAM sources ionospheric position shifts

    Nearly 200 hours of observing with the Murchison Widefield Array (MWA) radio telescope during the Galactic and Extra-galactic All-sky MWA (GLEAM) survey were used to assemble...
  • New double stars from HST

    Data from the Hubble Space Telescope (HST) Fine Guidance Sensor (FGS) interferometers, covering 22 months of guide-star acquisition operations, have been analyzed for evidence...
  • ATCA observations of 202 compact radio sources

    The Australia Telescope Compact Array (ATCA) has been used in support of the VLBI Space Observatory Programme (VSOP) space VLBI mission, to monitor the total and polarised flux...
  • VSOP 5 GHz AGN Survey

    The VSOP mission is a Japanese-led project to image radio sources with sub-milliarcsec resolution by correlating the signal from the orbiting 8-m telescope, HALCA, with a global...
  • Speckle interferometry of binaries

    We present speckle interferometric measurements of binary stars performed during September and October of 2009 with the 2.1m telescope of the Observatorio Astronomico Nacional...
  • Speckle interferometry at OAN. III.

    We present speckle interferometric measurements of binary stars performed during August of 2010 with the 1.5m telescope and during November of 2010 with the 2.1m telescope of...
  • Speckle interferometry of Ap stars. II.

    We present the results of speckle interferometric observations of 156 stars possessing global magnetic fields, carried out with the 6-m BTA telescope of the Special...
  • Nearby multiple Speckle interferometry. V.

    The results of speckle interferometric observations of 194 binary stars performed at the BTA 6m telescope in 2002-2006 are presented in this paper. For speckle observations we...
  • Speckle interferometry of Ap stars

    We present the results of speckle interferometry of a sample of 117 chemically peculiar stars with global magnetic fields. The observations were made in December 2009 at the BTA...
  • Rapidly rotating stars

    Optical interferometry provides us with a unique opportunity to improve our understanding of stellar structure and evolution. Through direct observation of rotationally...
  • Scattering Properties of the Milky Way

    We used archival very long baseline interferometry (VLBI) data of active galactic nuclei (AGN) observed from 1.4GHz to 86GHz to measure the angular size of VLBI radio cores in...
  • Stellar parameters study with SED fit algo

    Accurately measuring stellar parameters is a key goal to increase our understanding of the observable Universe. However, current methods are limited by many factors, in...
  • alpha Leo spectro-interferometric observation

    Differential Interferometry allows to obtain the differential visibility and phase, in addition to the spectrum. The differential phase contains important information about the...
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