Abstract We previously reported a putative detection of radio galaxy at $z=10.15$ , selected from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey. The redshift this source, GLEAM J0917–0012, was based on three weakly detected molecular emission lines observed with Atacama Large Millimetre (ALMA). In order to confirm result, we conducted deep spectroscopic follow-...

Conventional calibration methods used in hydrological modelling are based on runoff observations at the basin outlet. However, with only often produces reasonable but poor results for other variables. Multi-variable both and remote sensing-based evapotranspiration (ET) is developed naturally, due to importance of ET its data availability. This study compares two main schemes: (1) (Scheme I) (2)...

ABSTRACT The long-period (P = 1091 s) of the recently discovered pulsar GLEAM-X J162759.5–523504.3 can be attained by neutron stars evolving with fallback discs and magnetic dipole moments a few 1030 G cm3 at ages greater than ?2 × 105 yr consistently observational upper limits to period derivative, $\dot{P}$, X-ray luminosity, LX, source. current for $\dot{P}$ allow two alternative present sta...

An evolutionary algorithm based on Evolution Strategy (ES) is presented, which includes time-related command execution and the generation of process control elements. Its concept is enlarged by problem-oriented type definitions for parameters, this has allowed a flexible implementation for different applications. The GLEAM algorithm includes new features which distinguish it from ES and GAs, am...

This paper presents results of new experiments with the Global Optimising Resource Broker and Allocator GORBA for grid systems. The scheduling algorithm is based on the Evolutionary Algorithm GLEAM (General Learning Evolutionary Algorithm and Method) and several heuristics. The task of planning grid resource allocation is compared to pure NP-complete job shop scheduling and it is shown in which...

ABSTRACT We present the results from studying 140 radio sources in GLEAM (GaLactic and Extragalactic All-sky MWA [Murchison Widefield Array]) 4-Jy (G4Jy) Sample. These were followed-up with MeerKAT to assess their morphology enable host-galaxy identification, as existing images of 25 45-arcsec resolution do not provide sufficient information. refer these MeerKAT-2019 subset. The aim is identify...

Abstract We present the South Galactic Pole (SGP) data release from GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey. These combine both years of GLEAM observations at 72–231 MHz conducted with (MWA) cover an area 5 113 $\mathrm{deg}^{2}$ centred on SGP $20^{\mathrm{h}} 40^{\mathrm{m}} < \mathrm{RA} 05^{\mathrm{h}} 04^{\mathrm{m}}$ $-48^{\circ} \mathrm{Dec} -2^{\ci...

ABSTRACT The radio pulsar GLEAM-X J162759.5–523504.3 has an extremely long spin period ($P = 1091.17\, \mbox{s}$), and yet seemingly continues to spin-down rapidly ($\dot{P} < 1.2 \times 10^{-9}\, \mbox{ss}^{-1}$). magnetic field strength that is implied, if the source a neutron star undergoing dipole braking, could exceed $10^{16}\, \mbox{G}$. This object may therefore be most magnetize...