VLBI observations of several quasars and BL Lacertae objects were carried out at 1.66 GHz in November-December 1999 using six antennas (Medvezh'i Ozera, Svetloe, Pushchino, Noto, FlartRAO, and Shanghai). Maps of six sources (0420+022, 0420-014, 1308+326, 1345+125, 1803+784, and DA 193) obtained with milliarcsecond resolution are presented and discussed, together with their broadband (1-22 GHz) spectra obtained on the RATAN-600 radio telescope at epochs close to those of the VLBI observations. Comparison of the VLBI maps with maps of these sources obtained on standard VLBI networks and with the RATAN-600 quasisimultaneous total-flux measurements indicates the reliability of the results obtained on this Low Frequency VLBI Network and the ...
We investigated the archival ground-based VLBI images of the extragalactic radio sources included in...
The nature of jets in active galactic nuclei (AGNs) in the early Universe and their feedback to the ...
A patch of sky in the SDSS Stripe 82 was observed at 1.6 GHz with Very Long Baseline Interferometry ...
In November 1999 we carried out VLBI observations of several quasars and BL Lacertae objects at 1.66...
We present observational results for extragalactic radio sources with milliarcsecond components, obt...
We report on an ongoing effort to image active galactic nuclei simultaneously observed at 2.3 and 8....
© ESO, 2014. Aims. We present a new catalogue of the RATAN-600 multi-frequency measurements for BL L...
We present the results of bi-monthly VLBA observations at 7mm in 1998-1999 of 15 radio-bright AGNs. ...
Context. Radio-loud active galactic nuclei in the early Universe are rare. The quasars J0906+6930 at...
We have observed a sample of 15 bright active galactic nuclei (AGN) three times during 1992-1996 usi...
A patch of sky in the SDSS Stripe 82 was observed at 1.6 GHz with Very Long Baseline Interferometry ...
We discuss the results of two sessions of observations at the Low-Frequency VLBI Network (LFVN), car...
Context. Gigahertz peaked spectrum (GPS) radio sources are a class of extragalactic radio sources ch...
High-redshift radio sources provide plentiful opportunities for studying the formation and evolution...
A patch of sky in the SDSS Stripe 82 was observed at 1.6 GHz with Very Long Baseline Interferometry ...
We investigated the archival ground-based VLBI images of the extragalactic radio sources included in...
The nature of jets in active galactic nuclei (AGNs) in the early Universe and their feedback to the ...
A patch of sky in the SDSS Stripe 82 was observed at 1.6 GHz with Very Long Baseline Interferometry ...
In November 1999 we carried out VLBI observations of several quasars and BL Lacertae objects at 1.66...
We present observational results for extragalactic radio sources with milliarcsecond components, obt...
We report on an ongoing effort to image active galactic nuclei simultaneously observed at 2.3 and 8....
© ESO, 2014. Aims. We present a new catalogue of the RATAN-600 multi-frequency measurements for BL L...
We present the results of bi-monthly VLBA observations at 7mm in 1998-1999 of 15 radio-bright AGNs. ...
Context. Radio-loud active galactic nuclei in the early Universe are rare. The quasars J0906+6930 at...
We have observed a sample of 15 bright active galactic nuclei (AGN) three times during 1992-1996 usi...
A patch of sky in the SDSS Stripe 82 was observed at 1.6 GHz with Very Long Baseline Interferometry ...
We discuss the results of two sessions of observations at the Low-Frequency VLBI Network (LFVN), car...
Context. Gigahertz peaked spectrum (GPS) radio sources are a class of extragalactic radio sources ch...
High-redshift radio sources provide plentiful opportunities for studying the formation and evolution...
A patch of sky in the SDSS Stripe 82 was observed at 1.6 GHz with Very Long Baseline Interferometry ...
We investigated the archival ground-based VLBI images of the extragalactic radio sources included in...
The nature of jets in active galactic nuclei (AGNs) in the early Universe and their feedback to the ...
A patch of sky in the SDSS Stripe 82 was observed at 1.6 GHz with Very Long Baseline Interferometry ...