1,151 datasets found

Keywords: radio sources

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  • IC 342 multi-frequency radio polarization study

    Magnetic fields play an important role in the formation and stabilization of spiral structures in galaxies, but the interaction between interstellar gas and magnetic fields has...
  • AGN in IFRS. VLBA observations

    Infrared-faint radio sources (IFRS) form a new class of galaxies characterised by radio flux densities between tenths and tens of mJy and faint or absent infrared counterparts....
  • Radio jet emission from GeV-emitting NLSy1

    With the current study we aim at gaining understanding on the properties of radio emission and the assumed jet from four radio loud and {gamma}-ray loud Narrow Line Seyfert 1...
  • HI absorption in flux-selected radio AGNs

    We present an analysis of the HI 21cm absorption in a sample of 101 flux-selected radio AGN (S_1.4GHz_>50mJy) observed with the Westerbork Synthesis Radio Telescope (WSRT)....
  • LOFAR long baselines at 140MHz Calibrators

    An efficient means of locating calibrator sources for international LOw Frequency ARray (LOFAR) is developed and used to determine the average density of usable calibrator...
  • Multifrequency study of NL Seyfert 1 galaxies

    High-energy {gamma}-rays, which are produced by powerful relativistic jets, are usually associated with blazars and radio galaxies. In the current active galactic nuclei (AGN)...
  • M31 polarization & magnetic structure

    The Andromeda Galaxy (M31) is the nearest grand-design spiral galaxy. Thus far, most studies in the radio regime concentrated on the 10kpc ring. The central region of M31 has...
  • Spiderweb galaxy 870um and 1.4GHz images

    We present APEX LABOCA 870{mu}m observations of the field around the high-redshift radio galaxy MRC1138-262 at z=2.16. We detect 16 submillimeter galaxies (SMGs) in this...
  • NGC 7129 FIRS 2 interferometric 1-D spectrum

    NGC 7129 FIRS 2 (hereafter FIRS 2) is an intermediate-mass (2 to 8M_{sun}) protostar located at a distance of 1250pc. High spatial resolution observations are required to...
  • X-ray and radio images of SNR G351.0-5.4

    While searching the NRAO VLA Sky Survey (NVSS) for diffuse radio emission, we have serendipitously discovered extended radio emission close to the Galactic plane. The radio...
  • ATLASGAL: dust condensations in Galactic plane

    The formation processes and the evolutionary stages of high-mass stars are poorly understood compared to low-mass stars. Large-scale surveys are needed to provide an unbiased...
  • GLIMPSE/BGPS 6.7GHz methanol maser survey

    We present the results of a 6.7GHz methanol maser survey from the Effelsberg 100m radio telescope. A sample of 404 sources from the Bolocam Galactic Plane Survey (BGPS) 1.1mm...
  • Imaging GRB 980425 in millimetric and submm

    Gamma-ray bursts (GRBs) have been proposed as a tool to study star formation in the Universe, so it is crucial to investigate whether their host galaxies and immediate...
  • Fermi detection of BL Lac objects

    By cross-correlating an archival sample of 170 BL Lacs with a 2 year Fermi/LAT AGN sample, we have compiled a sample of 100 BL Lacs with Fermi detection (FBLs) and a sample of...
  • Small-diameter sources in Sino-German 6cm survey

    We have carried out the Sino-German 6cm polarisation survey of the Galactic plane at 6cm in total and polarised intensity using the Urumqi 25-m telescope of Xinjiang (formerly...
  • 43GHz observation of the blazar Mrk 421

    We report the results obtained for the AGN Markarian 421 by model-fitting the data in the visibility plane, studing the proper motion of jet components, the light curve, and the...
  • RM Synthesis of 33 sources around M31

    Low-frequency radio continuum observations are best suited to search for radio halos of inclined galaxies. Polarization measurements at low frequencies allow the detection of...
  • WMAP cosmic microwave background data

    There is currently a debate over the existence of claimed statistical anomalies in the cosmic microwave background (CMB), recently confirmed in Planck data. Recent work has...
  • Radio images of CIZA J2242.8+5301

    Giant cluster radio relics are thought to form at shock fronts in the course of collisions between galaxy clusters. Via processes that are still poorly understood, these shocks...
  • Variability of 198 extragalactic radio sources

    Combining measurements taken using the Wilkinson Microwave Anisotropy Probe (WMAP) from 2001 to 2008 with measurements taken using Planck from 2009 to 2010, we investigate the...
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