Nine-hour X-ray quasi-periodic eruptions from a low-mass black hole galactic nucleus

(2019)

Authors:

G Miniutti, RD Saxton, M Giustini, KD Alexander, RP Fender, I Heywood, I Monageng, M Coriat, AK Tzioumis, AM Read, C Knigge, P Gandhi, ML Pretorius, B Agís-González

Accretion and outflow in V404 Cyg

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 488:1 (2019) 1356-1365

Authors:

J Casares, T Muñoz-Darias, D Mata Sánchez, PA Charles, MAP Torres, M Armas Padilla, RP Fender, J García-Rojas

TeraHertz Exploration and Zooming-in for Astrophysics (THEZA): ESA Voyage 2050 White Paper

(2019)

Authors:

Leonid I Gurvits, Zsolt Paragi, Viviana Casasola, John Conway, Jordy Davelaar, Heino Falcke, Rob Fender, Sándor Frey, Christian M Fromm, Cristina García Miró, Michael A Garrett, Marcello Giroletti, Ciriaco Goddi, José-Luis Gómez, Jeffrey van der Gucht, José Carlos Guirado, Zoltán Haiman, Frank Helmich, Elizabeth Humphreys, Violette Impellizzeri, Michael Kramer, Michael Lindqvist, Hendrik Linz, Elisabetta Liuzzo, Andrei P Lobanov, Yosuke Mizuno, Luciano Rezzolla, Freek Roelofs, Eduardo Ros, Kazi LJ Rygl, Tuomas Savolainen, Karl Schuster, Tiziana Venturi, Martina Wiedner, J Anton Zensus

A new sample of southern radio galaxies: host-galaxy masses and star-formation rates

Monthly Notices of the Royal Astronomical Society Oxford University Press 489:3 (2019) 3403-3411

Authors:

T Marubini, Matthew Jarvis, S Fine, T Mauch, K McAlpine, M Prescott

GREENBURST: A commensal Fast Radio Burst search back-end for the Green Bank Telescope

Publications of the Astronomical Society of Australia Cambridge University Press 36 (2019) e032

Authors:

MP Surnis, D Agarwal, Lorimer, X Pei, G Foster, A Karastergiou, G Golpayegani, RJ Maddalena, S White, Wesley Armour, J Cobb, MA McLaughlin, DHE Macmahon, APV Siemion, D Werthimer, CJ Williams

Abstract:

We describe the design and deployment of GREENBURST, a commensal Fast Radio Burst (FRB) search system at the Green Bank Telescope. GREENBURST uses the dedicated L-band receiver tap to search over the 960$-$1920 MHz frequency range for pulses with dispersion measures out to $10^4$ pc cm$^{-3}$. Due to its unique design, GREENBURST will obtain data even when the L-band receiver is not being used for scheduled observing. This makes it a sensitive single pixel detector capable of reaching deeper in the radio sky. While single pulses from Galactic pulsars and rotating radio transients will be detectable in our observations, and will form part of the database we archive, the primary goal is to detect and study FRBs. Based on recent determinations of the all-sky rate, we predict that the system will detect approximately one FRB for every 2$-$3 months of continuous operation. The high sensitivity of GREENBURST means that it will also be able to probe the slope of the FRB source function, which is currently uncertain in this observing band.