The environment and host haloes of the brightest z~6 Lyman-break galaxies
Monthly Notices of the Royal Astronomical Society Oxford University Press 477:3 (2018) 3760-3774
Abstract:
By studying the large-scale structure of the bright high-redshift Lyman-break galaxy (LBG) population it is possible to gain an insight into the role of environment in galaxy formation physics in the early Universe. We measure the clustering of a sample of bright ($-22.7Revival of the Magnetar PSR J1622-4950: Observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR
ASTROPHYSICAL JOURNAL 856:2 (2018) ARTN 180
RFI flagging implications for short-duration transients
Astronomy and Computing Elsevier 23 (2018) 103-114
Tracking of an electron beam through the solar corona with LOFAR
Astronomy and Astrophysics EDP Sciences 611 (2018) A57
Abstract:
The Sun's activity leads to bursts of radio emission, among other phenomena. An example is type-III radio bursts. They occur frequently and appear as short-lived structures rapidly drifting from high to low frequencies in dynamic radio spectra. They are usually interpreted as signatures of beams of energetic electrons propagating along coronal magnetic field lines. Here we present novel interferometric LOFAR (LOw Frequency ARray) observations of three solar type-III radio bursts and their reverse bursts with high spectral, spatial, and temporal resolution. They are consistent with a propagation of the radio sources along the coronal magnetic field lines with nonuniform speed. Hence, the type-III radio bursts cannot be generated by a monoenergetic electron beam, but by an ensemble of energetic electrons with a spread distribution in velocity and energy. Additionally, the density profile along the propagation path is derived in the corona. It agrees well with three-fold coronal density model by (1961, ApJ, 133, 983).Tracking of an electron beam through the solar corona with LOFAR
ASTRONOMY & ASTROPHYSICS 611 (2018) ARTN A57