Advancing Astrophysics with the Square Kilometre Array

By S. Blyth, van der Thijs Hulst, Marc A. W. Verheijen, B. Catinella, Filippo Fraternali, M. Haynes, K. Hess, B. Koribalski, C. Lagos, M. Meyer and 5 more. 2015

561 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/2424334a5ee594c9b34aa8f46c7b5d259abf6623

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Citations in the corpus

The astrophysics of nanohertz gravitational waves (2018, background): “In the future, it is expected that new facilities such asMeerKAT and the SquareKilometreArraywill increase the sensitivity of PTAs manifold through extensive pulsar searching and timing programs (e. g., Janssen et al. 2015).”
One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering (2019, background): “2018) or SKA (Testi et al. 2015) will be quite powerful in this regard, although these long wavelength observations will get significant contamination from free-free emission from the star or jet.”
Diffuse Radio Emission from Galaxy Clusters (2019, methodology): “2), do not show the presence of a radio halo (Bonafede et al. 2017). This absence of a radio halo might be related to early or late phase mergers, and the timescale of halo formation and disappearance. Although, these results are not yet statistically significant given the small sample size. Cassano”
The Dark Energy Survey: more than dark energy - an overview (2016, background): “…volume radio survey offers potentially novel synergies, including the comparison of shape measurements made in the optical and radio wavelengths (Brown et al. 2014), large numbers of spectroscopicquality redshifts from the H I survey (Abdalla et al. 2015), and potentially the use of radio…”
Design and characterization of the Large-aperture Experiment to Detect the Dark Age (LEDA) radiometer systems (2017, methodology): “Motivated by limitations of single-antenna experiments, LEDA is a multi-antenna experiment, co-installed on the Long Wavelength Array stations at Owens Valley Radio Observatory (OVRO-LWA, 37.24◦N, 118.28◦W), and the National Radio Astronomy Observatory in Socorro, New Mexico (LWA1, 34.07◦N, 107.63◦W”
The Giant Radio Array for Neutrino Detection (GRAND): Science and design (2018, background): “Direct imaging of ionized regions [206] and statistical studies of brightness fluctuations in the 21-cm spectrum using interferometry [207–214] could measure the 21-cm cosmic signal with high sensitivity, though they are regarded as challenging observations.”
Cosmology with a SKA HI intensity mapping survey (2015, background): “2009; Rao et al. 2006; Martin et al. 2010; Lah et al. 2007; Zwaan et al. 2005; Khandai et al. 2011), partially based on the compilation in Duffy et al. (2012). DLA observations are shown in blue, cross-correlations in orange, other observations in red, and simulations in green.”
Fundamental physics with the Square Kilometre Array (2018, methodology): “Chapman et al. (2015) compared foreground subtraction methods and found that GMCA proves the most robust to realistic foreground spectra.”
CMB anomalies after Planck (2015, methodology): “by means of the square kilometre array (SKA; [190]), will map all galaxies containing neutral hydrogen out to a redshift of a few.”