The Square Kilometre Array (SKA)

Research group

Research theme

Sub department

About

Related research groups

The NANOGrav 11-year Data Set: Pulse Profile Variability

The Astrophysical Journal American Astronomical Society 868:2 (2018) 122

Authors:

PR Brook, A Karastergiou, MA McLaughlin, MT Lam, Z Arzoumanian, S Chatterjee, JM Cordes, K Crowter, M DeCesar, PB Demorest, T Dolch, JA Ellis, RD Ferdman, E Ferrara, E Fonseca, PA Gentile, G Jones, ML Jones, TJW Lazio, L Levin, DR Lorimer, RS Lynch, C Ng, DJ Nice, TT Pennucci, SM Ransom, PS Ray, R Spiewak, IH Stairs, DR Stinebring, K Stovall, JK Swiggum, WW Zhu
More details from the publisher
Details from ArXiV

The Variable Pulsar Wind Nebula of PSR J1809–1917

The Astrophysical Journal American Astronomical Society 868:2 (2018) 119

Authors:

Noel Klingler, Oleg Kargaltsev, George G Pavlov, Bettina Posselt
More details from the publisher
More details

Verifying and reporting Fast Radio Bursts

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 481:2 (2018) 2612-2627

Authors:

Griffin Foster, Aris Karastergiou, Marisa Geyer, Mayuresh Surnis, Golnoosh Golpayegani, Kejia Lee, Duncan Lorimer, Danny C Price, Kaustubh Rajwade
More details from the publisher

Classification of Multiwavelength Transients with Machine Learning

(2018)

Authors:

K Sooknunan, M Lochner, Bruce A Bassett, HV Peiris, R Fender, AJ Stewart, M Pietka, PA Woudt, JD McEwen, O Lahav
More details from the publisher

The C-Band All-Sky survey (C-BASS)

Proceedings of the 53rd Rencontres de Moriond, Cosmology 2018 ARISF (2018) 137-140

Abstract:

The C-Band All-Sky survey (C-BASS) is an experiment to image the whole sky in intensity and polarization at 5 GHz. The primary aim of C-BASS is to provide low-frequency all-sky maps of the Galactic emission which will enable accurate component separation analysis of both existing and future CMB intensity and polarization imaging surveys. Here we present an overview of the experiment and an update on the current status of observations. We present simulation results showing the expected improvement in the recovery of CMB and foreground signals when including C-BASS data as an additional low-frequency channel, both for intensity and polarization. We also present preliminary results from the northern part of the sky survey.
Details from ORA
Details from ArXiV