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Radio stars for linking celestial reference frames
Radio stars play a key role in establishing the link between optical reference frames and the conventional celestial reference frame based on extragalactic radio sources. The... -
ROSAT active galaxies identifications
Table 2 gives the 5 GHz high resolution radio source properties for the 1861 Rosat-GreenBank (RGB) sources for which subarcsecond positions and core radio flux densities were... -
ROSAT Galactic Plane Survey observations
The analysis of the part of the ROSAT all-sky survey covering the galactic plane is the scope of a dedicated project called the ROSAT Galactic Plane Survey. In order to... -
Radio continuum study of the MC
We present a new catalogue of radio sources in the Large Magellanic Cloud (LMC) based on observations at 2.30GHz with the Parkes radio telescope. A total of 119 sources have... -
SEST obs. of extragalactic radiosources
Flux densities of 155 extragalactic radio sources observed with the SEST telescope at 3mm and 1.3mm are presented. The observations were performed from October 1987 to June... -
Radio sources in fields near G160.9+2.6 (HB9)
We present a catalogue of the 408MHz and 1420MHz radio sources in the region centered near Right Ascension 4h58m and Declination 46degrees (epoch 1950), i.e. near the supernova... -
Radio continuum study of the MC
From observations with the Parkes radio telescope, we present catalogues of radio sources in the Large Magellanic Cloud at four frequencies: 1.40, 2.45, 4.75 and 8.55GHz, and an... -
Radio to X-Ray distribution of BL Lac Objects
(no description available) Cone search capability for table J/A+AS/109/267/table1 (Radio selected BL Lacs 1Jy and S4 surveys) Cone search capability for table... -
Ultra-steep spectrum radiosources
Radio sources with ultra-steep spectra (USS; spectral index <~ -1.0) have been found to be excellent tracers of galaxies at redshifts z>~2. The samples are selected from... -
Multifrequency observations of ROSAT sources
We report on results of multifrequency radio continuum observations with the Effelsberg 100-m telescope of 234 radio sources which have counterparts in the ROSAT all-sky survey.... -
Optical identification status of 1Jy catalogue
(no description available) Cone search capability for table J/A+AS/105/211/table2 (Radio data for the 1 Jy radio sources) -
4.85GHz extragalactic sources
Eleven selected regions of sky have been surveyed at an observing frequency of 4.85GHz to limiting flux densities as low as 0.01Jy. The surveys provide a sample of 118 sources... -
A LOFAR sample of OCRS in dwarf galaxies
The vast majority of extra-galactic, compact continuum radio sources are associated with star formation or jets from (super)massive black holes and, as such, are more likely to... -
HI in NGC 3100
We present Australia Compact Telescope Array (ATCA) 21-cm observations of the nearby low-excitation radio galaxy (LERG) NGC 3100. This is the brightest galaxy of a loose group... -
943MHz EMU image of the galaxy cluster A3718
Multifrequency studies of galaxy clusters are crucial for inferring their dynamical states and physics. Moreover, these studies allow us to investigate cluster-embedded sources,... -
CO(2-1) survey at 9pc resolution in SMC
We present a CO(2-1) survey at 9pc resolution obtained with the APEX telescope in the Small Magellanic Cloud (SMC). We perform a catalog of 177 molecular clouds in an extensive... -
SMACS J0723.3-7327 eROSITA and Chandra images
SMACS J0723.3-7327 is the first galaxy cluster lens observed by James Webb Space Telescope (JWST). Based on its early release observation data, several groups have reported the... -
CHANG-ES. XXVI. radio images of 5 galaxies
Galactic winds play a key role in regulating the evolution of galaxies over cosmic time. In recent years, the role of cosmic rays (CRs) in the formation of the galactic wind has... -
Abell 2256 radio images
We present the first detailed analysis of the radio halo in the merging galaxy cluster Abell 2256 using the LOw Frequency ARray, the upgraded Giant Metrewave Radio Telescope,... -
SNR CTB87 14.7GHz and 17.3GHz total intensity maps
Breaks in the radio spectra of supernova remnants (SNRs) reflect the maximum energy of either shock-accelerated electrons or - in the case of pulsar wind nebulae - of electrons...