Australian square kilometre array pathfinder: I. system description
In this paper, we describe the system design and capabilities of the Australian Square
Kilometre Array Pathfinder (ASKAP) radio telescope at the conclusion of its construction …
Kilometre Array Pathfinder (ASKAP) radio telescope at the conclusion of its construction …
The Evolutionary Map of the Universe pilot survey
We present the data and initial results from the first pilot survey of the Evolutionary Map of
the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array …
the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array …
Galaxy And Mass Assembly (GAMA): assimilation of KiDS into the GAMA database
ABSTRACT The Galaxy And Mass Assembly Survey (GAMA) covers five fields with highly
complete spectroscopic coverage (> 95 per cent) to intermediate depths (r< 19.8 or i< 19.0 …
complete spectroscopic coverage (> 95 per cent) to intermediate depths (r< 19.8 or i< 19.0 …
Deep ASKAP EMU Survey of the GAMA23 field: properties of radio sources
G Gürkan, I Prandoni, A O'Brien, W Raja… - Monthly Notices of …, 2022 - academic.oup.com
ABSTRACT We present the Australian Square Kilometre Array Pathfinder (ASKAP)
observations of the Galaxy and Mass Assembly (GAMA)-23h field. The survey was carried …
observations of the Galaxy and Mass Assembly (GAMA)-23h field. The survey was carried …
Deep investigation of neutral gas origins (DINGO): H i stacking experiments with early science data
J Rhee, M Meyer, A Popping, S Bellstedt… - Monthly Notices of …, 2023 - academic.oup.com
We present early science results from Deep Investigation of Neutral Gas Origins (DINGO),
an i survey using the Australian Square Kilometre Array Pathfinder (ASKAP). Using ASKAP …
an i survey using the Australian Square Kilometre Array Pathfinder (ASKAP). Using ASKAP …
The ASKAP-EMU Early Science Project: 888 MHz radio continuum survey of the Large Magellanic Cloud
CM Pennock, JT Van Loon, MD Filipović… - Monthly Notices of …, 2021 - academic.oup.com
We present an analysis of a new 120 deg2 radio continuum image of the Large Magellanic
Cloud (LMC) at 888 MHz with a bandwidth of 288 MHz and beam size of 13 9× 12 1 from the …
Cloud (LMC) at 888 MHz with a bandwidth of 288 MHz and beam size of 13 9× 12 1 from the …
Connecting MeerKAT radio continuum properties to GAMA optical emission-line and WISE mid-infrared activity
HFM Yao, ME Cluver, TH Jarrett… - The Astrophysical …, 2022 - iopscience.iop.org
The identification of active galactic nuclei (AGNs) in large surveys has been hampered by
seemingly discordant classifications arising from differing diagnostic methods, usually …
seemingly discordant classifications arising from differing diagnostic methods, usually …
The SAMI galaxy survey: impact of black hole activity on galaxy spin–filament alignments
S Barsanti, M Colless, F D'Eugenio, S Oh… - Monthly Notices of …, 2023 - academic.oup.com
The activity of central supermassive black holes might affect the alignment of galaxy spin
axes with respect to the closest cosmic filaments. We exploit the Sydney–AAO Multi-object …
axes with respect to the closest cosmic filaments. We exploit the Sydney–AAO Multi-object …
FLASH early science – discovery of an intervening H i 21-cm absorber from an ASKAP survey of the GAMA 23 field
We present early science results from the First Large Absorption Survey in H i (FLASH), a
spectroscopically blind survey for 21-cm absorption lines in cold hydrogen (H i) gas at …
spectroscopically blind survey for 21-cm absorption lines in cold hydrogen (H i) gas at …
DEVILS/MIGHTEE/GAMA/DINGO: the impact of SFR time-scales on the SFR-radio luminosity correlation
RHW Cook, LJM Davies, J Rhee… - Monthly Notices of …, 2024 - academic.oup.com
The tight relationship between infrared luminosity (L TIR) and 1.4 GHz radio continuum
luminosity (L 1.4 GHz) has proven useful for understanding star formation free from dust …
luminosity (L 1.4 GHz) has proven useful for understanding star formation free from dust …