418 datasets found

Keywords: Radio continuum emission

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  • Gould's Belt VLA survey. III. Orion region

    We present results from a high-sensitivity (60{mu}Jy), large-scale (2.26deg^2^) survey obtained with the Karl G. Jansky Very Large Array as part of the Gould's Belt Survey...
  • Star Formation in Radio Survey (SFRS): 33GHz obs.

    We present 33GHz photometry of 103 galaxy nuclei and extranuclear star-forming complexes taken with the Green Bank Telescope (GBT) as part of the Star Formation in Radio Survey...
  • Polarized DRAO sources

    The Dominion Radio Astrophysical Observatory Deep Field polarization study has been matched with the Spitzer Wide-Area Infrared Extragalactic Survey of the European Large Area...
  • VLA fluxes for AT20G radio galaxies

    We present flux densities and polarization percentages of 159 radio galaxies based on nearly simultaneous Very Large Array observations at four frequencies, 4.86, 8.46, 22.46,...
  • 1.4GHz observations of bright early-type galaxies

    We have measured the radio continuum emission of 396 early-type galaxies brighter than K=9, using 1.4GHz imagery from the NRAO Very Large Array Sky Survey, Green Bank 300ft...
  • 148GHz ACT extragalactic sources catalog

    We report on extragalactic sources detected in a 455deg^2^ map of the southern sky made with data at a frequency of 148GHz from the Atacama Cosmology Telescope (ACT) 2008...
  • Galactic Worms

    A catalog of candidates for the Galactic Worms that are possibly the walls surrounding the superbubbles is compiled; 118 isolated structures that appear both in HI and in IR (60...
  • Filling in the gaps in the 4.85GHz sky

    We describe a 4.85GHz survey of bright, flat-spectrum radio sources conducted with the Effelsberg 100m telescope in an attempt to improve the completeness of existing surveys,...
  • GRG-J2233+1315 GMRT and LOFAR images

    We present for the first time a study of peculiar giant radio galaxy (GRG) J223301+131502 using deep multi-frequency radio observations from GMRT (323, 612, and 1300MHz) and...
  • SAGAN. I. New sample & multi-wavelength studies

    We present the first results of a project called SAGAN, which is dedicated solely to the studies of relatively rare megaparsec-scale radio galaxies in the Universe, called giant...
  • Sources detected at 325 and 610 MHz in Cygnus

    Observations at the radio continuum band below the gigahertz band are key when the nature and properties of non-thermal sources are investigated because their radio radiation is...
  • F-GAMMA 2.64-43GHz radio data over 2007-2015

    The advent of the Fermi gamma-ray space telescope with its superb sensitivity, energy range, and unprecedented capability to monitor the entire 4{pi} sky within less than 2-3 h,...
  • Massive star-forming regions radio lines

    We present Australia Telescope Compact Array (ATCA) observations of the H_2_O maser line and radio continuum at 18.0GHz and 22.8GHz toward a sample of 192 massive star-forming...
  • Rotation Measure synthesis of WSRT obs.

    Rotation Measure synthesis (RM synthesis) of the Westerbork Synthesis Radio Telescope (WSRT) observations at 2m wavelength of the FAN region at l=137deg, b=+7deg shows the...
  • Bright northern radio sources with VLA/JVLA

    We report multiple epoch VLA/JVLA observations of 89 northern hemisphere sources, most with 37GHz flux density >1Jy, observed at 4.8, 8.5, 33.5, and 43.3GHz. The high...
  • Radio relics in LoTSS-DR2 and PSZ2

    It is well-established that shock waves in the intracluster medium launched by galaxy cluster mergers can produce synchrotron emission, which is visible to us at radio...
  • Integrated radio continuum spectra of galaxies

    We investigate the spectral shape of the total continuum radiation, between 74MHz and 5GHz (400-6cm in wavelength), for a large sample of bright galaxies. We take advantage of...
  • LOFAR LBA Sky Survey First Release

    The Low Frequency Array (LOFAR) is the only existing radio interferometer able to observe at ultra-low frequencies (<100MHz) with high resolution (<15-arcsec) and high...
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