Results 101 to 110 of about 256,920 (281)
The Massive and Distant Clusters of WISE Survey. VIII. Radio Activity in Massive Galaxy Clusters [PDF]
We present a study of the central radio activity of galaxy clusters at high redshift. Using a large sample of galaxy clusters at $0.7
arxiv +1 more source
Abstract The use of matrix‐assisted laser desorption/ionization (MALDI) mass spectrometry for the analysis of carbohydrates and glycoconjugates is a well‐established technique and this review is the 12th update of the original article published in 1999 and brings coverage of the literature to the end of 2022.
David J. Harvey
wiley +1 more source
Radio Galaxy Zoo: host galaxies and radio morphologies derived from visual inspection [PDF]
Accepted to MNRAS, 17 pages, 13 figures, 1 table.
Julie Banfield+39 more
openaire +9 more sources
Abstract Objective This study aims to understand the utility of a stepwise technology‐based audiometry with rapid results (STARR) school screening protocol. Study Design A prospective cohort study. Setting Six elementary schools in a single school district in Minnesota.
Autefeh Sajjadi+15 more
wiley +1 more source
LUMINOSITY-LINEAR SIZE RELATION FOR GALAXIES AND QUASARS WITH STEEP RADIO SPECTRUM
Our data for sources with steep radio spectrum, detected with radio telescope UTR-2 at the decametre band give evidence on the great luminosities, linear sizes, characteristic ages of these objects.
A. P. Miroshnichenko
doaj +1 more source
Research on Morphological Detection of FR I and FR II Radio Galaxies Based on Improved YOLOv5
Recently, astronomy has witnessed great advancements in detectors and telescopes. Imaging data collected by these instruments are organized into very large datasets that form data-oriented astronomy.
Xingzhu Wang+6 more
doaj +1 more source
MRC B0319-454: Probing the large-scale structure with a giant radio galaxy [PDF]
We present an investigation of the relationships between the radio properties of a giant radio galaxy MRC B0319-454 and the surrounding galaxy distribution with the aim of examining the influence of intergalactic gas and gravity associated with the large-scale structure on the evolution in the radio morphology.
arxiv +1 more source
We present a study of the optical brightness profiles of early type galaxies, using a number of samples of radio galaxies and optically selected elliptical galaxies.
A. Capetti+60 more
core +1 more source
Why Are Radio-Galaxies Prolific Producers of Type Ia Supernovae? [PDF]
An analysis of SNIa events in early type galaxies from the Cappellaro et al (1999) database provides conclusive evidence that the rate of type Ia Supernovae (SNe) in radio-loud galaxies is about 4 times higher than the rate measured in radio-quiet ...
Bondi H.+17 more
core +2 more sources
High-Redshift Radio Galaxies [PDF]
Radio galaxies are unique cosmological probes. As with radio-loud quasars, the presence of luminous radio continuum and optical line emission enable radio galaxies to be observed and recognized at large distances, up to z = 4.2. However, unlike the situation for most quasars, their optical emission can be spatially resolved from the ground and studied ...
openaire +3 more sources