1,151 datasets found

Keywords: radio sources

Filter Results
  • NGC 3184, 4736, 5055 and 5194 LOFAR & WSRT maps

    Radio continuum (RC) emission in galaxies allows us to measure star formation rates (SFRs) unaffected by extinction due to dust, of which the low-frequency part is...
  • Abell 1914 multiwavelength radio images

    A number of radio observations have revealed the presence of large synchrotron-emitting sources associated with the intra-cluster medium. There is strong observational evidence...
  • LoTSS/HETDEX. Optical quasars. I.

    The radio-loud/radio-quiet (RL/RQ) dichotomy in quasars is still an open question. Although it is thought that accretion onto supermassive black holes in the centre the host...
  • LOFAR Two-metre Sky Survey DR1 source catalog

    The LOFAR Two-metre Sky Survey (LoTSS) is an ongoing sensitive, high-resolution 120-168MHz survey of the entire northern sky for which observations are now 20% complete. We...
  • ATESP 5 GHz radio survey. IV.

    It is now established that the faint radio population is a mixture of star-forming galaxies and faint active galactic nuclei (AGNs), with the former dominating below...
  • SgrA* and NRAS530 86GHz images

    The compact radio source Sagittarius A (Sgr A) in the Galactic centre is the primary supermassive black hole candidate. General relativistic magnetohydrodynamical (GRMHD)...
  • Saturn lightning episodes of storm F

    The paper analyzes a lightning storm on Saturn that raged for 7.5 months at a planetocentric latitude of 35 deg. south from 27 November 2007 until 15 July 2008. The storm system...
  • High cadence polarization monitoring of OJ287

    We present a multifrequency, dense radio monitoring program of the blazar OJ287 using the 100-m Effelsberg radio telescope. The program aims to test different binary...
  • THOR survey in northern Galactic plane

    Radio continuum surveys of the Galactic plane can find and characterize HII regions, supernova remnants (SNRs), planetary nebulae (PNe), and extragalactic sources. A number of...
  • SgrA* orbital motions with GRAVITY

    We report the detection of continuous positional and polarization changes of the compact source SgrA* in high states ('flares') of its variable near- infrared emission with the...
  • 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...
  • Abell 1795 GMRT and Chandra maps

    In this paper we analyze AGN activity signatures in the rich nearby galaxy cluster Abell 1795 aiming to confirm and characterize the long-term feedback history in the system. We...
  • G328.2551-0.5321 ALMA images

    The conditions leading to the formation of the most massive O-type stars, are still an enigma in modern astrophysics. To assess the physical conditions of high-mass protostars...
  • Catalog of NLS1s galaxies in 6dFGS survey

    We present a new accurate catalog of narrow-line Seyfert 1 galaxies (NLS1s) in the southern hemisphere from the Six-degree Field Galaxy Survey (6dFGS) final data release, which...
  • CORNISH project. III. UCHII region catalogue

    A catalogue of 239 ultra-compact HII regions (UCHIIs) found in the CORNISH survey at 5GHz and 1.5-arcsec resolution in the region 10{deg}<l<65{deg}, |b|<1{deg} is...
  • Polarized point sources in LOTSS-HETDEX

    We have produced a catalog of 92 polarized radio sources at 150MHz at 4.3-arcmin resolution and 1mJy rms sensitivity, which is the largest catalog of polarized sources at such...
  • G346.056-0.021 and G346.077-0.056 radio images

    We present a multiwavelength study of two southern Galactic H II regions G346.056-0.021 and G346.077-0.056 which are located at a distance of 10.9kpc. The distribution of...
  • Cas A LOFAR and VLA images

    Cassiopeia A is one of the best-studied supernova remnants. Its bright radio and X-ray emission is due to shocked ejecta. Cas A is rather unique in that the unshocked ejecta can...
  • Cores in HII regions parameters

    High-mass stars form in much richer environments than those associated with isolated low-mass stars, and once they reach a certain mass, produce ionised (HII) regions. The...
  • 6 galaxy clusters ATCA 2.1GHz images

    A fraction of galaxy clusters host diffuse radio sources whose origins are investigated through multi-wavelength studies of cluster samples. We investigate the presence of...
You can also access this registry using the API (see API Docs).