We present the catalog of Radio sources associated with Optical Galaxies and having Unresolved or Extended morphologies I (ROGUE I), consisting of 32,616 spectroscopically selected galaxies. It is the largest handmade catalog of this kind, obtained by cross-matching galaxies from the Sloan Digital Sky Survey (SDSS) Data Release 7 and radio sources from both the First Images of Radio Sky at Twenty Centimetre (FIRST) survey and the NRAO Very Large Array Sky Survey, without imposing a limit on the radio flux densities. The catalog provides a visual classification of radio and optical morphologies of galaxies presenting a FIRST core within 3'' of the optical position. The radio morphological classification is performed by examining the radio–op...
We discuss the optical and radio properties of similar to30,000 FIRST (radio, 20 cm, sensitive to 1 ...
An investigation into the environments of a large number of radio galaxies is described. T...
A new sample of very large angular size radio sources has been selected from the 1.4 GHz VLA surveys...
We present the catalogue of Radio sources associated with Optical Galaxies and having Unresolved or ...
We constructed and presented in the first paper of this series a new sample of 84 large angular size...
Celem pracy jest poszukiwanie rozciągłych struktur radiowych wokół zwartych obiektów z katalogu ROGU...
International audienceBasing our analysis on ROGUE I, a catalog of over 32,000 radio sources associa...
We present results from the first 12 months of operation of Radio Galaxy Zoo, which upon completion ...
We present an analysis of the properties of optical counterparts of radio sources down to 1 mJy. Opt...
We present results from the first twelve months of operation of Radio Galaxy Zoo, which upon complet...
We discuss the optical and radio properties of ~30,000 FIRST (radio, 20 cm, sensitive to 1 mJy) sour...
Restricted Access.This is the second in a series of papers discussing the radio, optical, and near-I...
This is the second in a series of papers discussing the radio, optical, and near-IR properties of a ...
The noise level in the central part of the field is 11 Jy. From these data we have extracted a catal...
Restricted Access.This is the first in a series of papers discussing the properties of a complete se...
We discuss the optical and radio properties of similar to30,000 FIRST (radio, 20 cm, sensitive to 1 ...
An investigation into the environments of a large number of radio galaxies is described. T...
A new sample of very large angular size radio sources has been selected from the 1.4 GHz VLA surveys...
We present the catalogue of Radio sources associated with Optical Galaxies and having Unresolved or ...
We constructed and presented in the first paper of this series a new sample of 84 large angular size...
Celem pracy jest poszukiwanie rozciągłych struktur radiowych wokół zwartych obiektów z katalogu ROGU...
International audienceBasing our analysis on ROGUE I, a catalog of over 32,000 radio sources associa...
We present results from the first 12 months of operation of Radio Galaxy Zoo, which upon completion ...
We present an analysis of the properties of optical counterparts of radio sources down to 1 mJy. Opt...
We present results from the first twelve months of operation of Radio Galaxy Zoo, which upon complet...
We discuss the optical and radio properties of ~30,000 FIRST (radio, 20 cm, sensitive to 1 mJy) sour...
Restricted Access.This is the second in a series of papers discussing the radio, optical, and near-I...
This is the second in a series of papers discussing the radio, optical, and near-IR properties of a ...
The noise level in the central part of the field is 11 Jy. From these data we have extracted a catal...
Restricted Access.This is the first in a series of papers discussing the properties of a complete se...
We discuss the optical and radio properties of similar to30,000 FIRST (radio, 20 cm, sensitive to 1 ...
An investigation into the environments of a large number of radio galaxies is described. T...
A new sample of very large angular size radio sources has been selected from the 1.4 GHz VLA surveys...