The cross - correlation of the source list from the ROSAT All - Sky Survey with the 5 GHz Green Bank survey yields a list of 2127 objects. About two thirds of them are optically unidentified. The majority of the objects with known optical counterparts are quasars and radio galaxies, most of them detected in X-rays for the first time. In this paper we present a list of the previously optically identified objects with their main characteristics and discuss their general (bulk) properties. We find strong correlations between luminosities in the radio, optical, and X-ray bands which differ for quasars and radio galaxies. The fraction of flat radio spectrum sources increases with redshift and #propor to#95% of all sources above z=2 are of that t...
We discuss the optical and radio properties of similar to30,000 FIRST (radio, 20 cm, sensitive to 1 ...
Our current understanding of radio-loud active galactic nuclei (AGN) comes predominantly from studie...
The ROSAT Deep Survey includes a complete sample of 50 X-ray sources with fluxes in the $0.5 - 2$ ke...
The cross-correlation of a source list from the ROSAT All Sky Survey with the Molonglo 408 MHz surve...
We present the broad band, radio - to - X-ray, properties of a large sample of mostly previously opt...
A database of radio-quiet quasers detected with ROSAT is presented containing 846 quasars seen in th...
The beginning of X-ray astronomy is based on two accidental discoveries made in 1962. A single point...
The noise level in the central part of the field is 11 Jy. From these data we have extracted a catal...
A deep and large-area survey of the North Ecliptic Pole region was made with the ROSAT All-Sky Surve...
The ROSAT Deep Survey in the Lockman Hole contains a complete sample of 50 X-ray sources with fluxes...
The Byurakan/Hamburg/ROSAT Catalogue (BHRC) of the optical identifications of X-ray sources is prese...
We discuss the optical and radio properties of 30,000 FIRST sources positionally associated with an ...
The relationship between the radio and optical properties of quasars and the connection between thes...
We discuss the optical and radio properties of ~30,000 FIRST (radio, 20 cm, sensitive to 1 mJy) sour...
Rosat pointed observations of a complete sample of radio-selected BL Lacs (RB Ls) have been analyze...
We discuss the optical and radio properties of similar to30,000 FIRST (radio, 20 cm, sensitive to 1 ...
Our current understanding of radio-loud active galactic nuclei (AGN) comes predominantly from studie...
The ROSAT Deep Survey includes a complete sample of 50 X-ray sources with fluxes in the $0.5 - 2$ ke...
The cross-correlation of a source list from the ROSAT All Sky Survey with the Molonglo 408 MHz surve...
We present the broad band, radio - to - X-ray, properties of a large sample of mostly previously opt...
A database of radio-quiet quasers detected with ROSAT is presented containing 846 quasars seen in th...
The beginning of X-ray astronomy is based on two accidental discoveries made in 1962. A single point...
The noise level in the central part of the field is 11 Jy. From these data we have extracted a catal...
A deep and large-area survey of the North Ecliptic Pole region was made with the ROSAT All-Sky Surve...
The ROSAT Deep Survey in the Lockman Hole contains a complete sample of 50 X-ray sources with fluxes...
The Byurakan/Hamburg/ROSAT Catalogue (BHRC) of the optical identifications of X-ray sources is prese...
We discuss the optical and radio properties of 30,000 FIRST sources positionally associated with an ...
The relationship between the radio and optical properties of quasars and the connection between thes...
We discuss the optical and radio properties of ~30,000 FIRST (radio, 20 cm, sensitive to 1 mJy) sour...
Rosat pointed observations of a complete sample of radio-selected BL Lacs (RB Ls) have been analyze...
We discuss the optical and radio properties of similar to30,000 FIRST (radio, 20 cm, sensitive to 1 ...
Our current understanding of radio-loud active galactic nuclei (AGN) comes predominantly from studie...
The ROSAT Deep Survey includes a complete sample of 50 X-ray sources with fluxes in the $0.5 - 2$ ke...