Search Results - "Wicenec, A."
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Optimising NGAS for the MWA Archive
Published in Experimental astronomy (01-12-2013)“…The Murchison Widefield Array (MWA) is a next-generation radio telescope, generating visibility data products continuously at about 400 MB/s. Efficiently…”
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Journal Article -
2
Data modelling approaches to astronomical data: Mapping large spectral line data cubes to dimensional data models
Published in Astronomy and computing (01-01-2022)“…As a new generation of large-scale telescopes are expected to produce single data products in the range of hundreds of GBs to multiple TBs, different…”
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3
AdiosStMan: Parallelizing Casacore Table Data System using Adaptive IO System
Published in Astronomy and computing (01-07-2016)“…In this paper, we investigate the Casacore Table Data System (CTDS) used in the casacore and CASA libraries, and methods to parallelize it. CTDS provides a…”
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4
An empirical evaluation on the applicability of the DALiuGE execution framework
Published in Astronomy and computing (01-01-2022)“…The Square Kilometre Array (SKA) project is an international cooperation project to build the largest radio telescope worldwide. Data processing is one of the…”
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5
DALiuGE: A graph execution framework for harnessing the astronomical data deluge
Published in Astronomy and computing (01-07-2017)“…The Data Activated Liu1 Graph Engine – DALiuGE2– is an execution framework for processing large astronomical datasets at a scale required by the Square…”
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6
Astronomical imagery: Considerations for a contemporary approach with JPEG2000
Published in Astronomy and computing (01-09-2015)“…The new wide-field radio telescopes, such as: ASKAP, MWA, LOFAR, eVLA and SKA; will produce spectral-imaging data-cubes (SIDC) of unprecedented size—in the…”
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7
Imaging SKA-scale data in three different computing environments
Published in Astronomy and computing (01-01-2016)“…We present the results of our investigations into options for the computing platform for the imaging pipeline in the chiles project, an ultra-deep HI…”
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8
Integrating HPC into Radio-Astronomical data reduction
Published in 2011 XXXth URSI General Assembly and Scientific Symposium (01-08-2011)“…The construction of the SKA and its pathfinders puts significant computational and power consumption constraints on the design of the computer hardware…”
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Conference Proceeding -
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Virtual Observatory studies of Planetary Nebulae
Published 05-02-2009“…Starting from the Strasbourg ESO Catalogue (SEC) of Planetary Nebulae (PNe), the largest PNe compilation available with ~ 1500 objects, we undertook a…”
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10
Realisation of a low frequency SKA Precursor: The Murchison Widefield Array
Published 06-12-2012“…The Murchison Widefield Array is a low frequency (80 - 300 MHz) SKA Precursor, comprising 128 aperture array elements distributed over an area of 3 km…”
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The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
Published 29-06-2012“…The Murchison Widefield Array (MWA) is one of three Square Kilometre Array Precursor telescopes and is located at the Murchison Radio-astronomy Observatory in…”
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ESO Imaging Survey: infrared observations of CDF-S and HDF-S
Published 23-02-2006“…This paper presents infrared data obtained from observations carried out at the ESO 3.5m New Technology Telescope (NTT) of the Hubble Deep Field South (HDF-S)…”
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ESO Imaging Survey: Past Activities and Future Prospects
Published 10-12-1999“…The ESO Imaging Survey (EIS) is an ongoing project to carry out public imaging surveys to support programs on the ESO Very Large Telescope (VLT). The first…”
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14
ESO Imaging Survey. Deep Public Survey: Multi-Color Optical Data for the Chandra Deep Field South
Published 05-03-2001“…Astron.Astrophys.379:740-754,2001 This paper presents multi-passband optical data obtained from observations of the Chandra Deep Field South (CDF-S), located…”
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ESO Imaging Survey. Deep Public Survey: Infrared Data for the Chandra Deep Field South
Published 16-02-2001“…This paper presents new J and Ks near-infrared data obtained from observations of the Chandra Deep Field South (CDF-S) conducted at the ESO 3.5m New Technology…”
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ESO Imaging Survey VII. Distant Cluster Candidates over 12 square degrees
Published 31-07-1998“…In this paper the list of candidate clusters identified from the I-band data of the ESO Imaging Survey (EIS) is completed using the images obtained over a…”
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ESO Imaging Survey. AXAF Field: Deep Optical-Infrared Observations, Data Reduction and Photometry
Published 09-12-1998“…This paper presents ground-based data obtained from deep optical and infrared observations carried out at the ESO 3.5 New Technology Telescope (NTT) of a field…”
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18
ESO Imaging Survey. Hubble Deep Field South: Optical-Infrared Observations, Data Reduction and Photometry
Published 04-12-1998“…This paper presents ground-based data obtained from deep optical and infrared observations of the HST Hubble Deep Field South (HDF-S) field carried out at the…”
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ESO Imaging Survey VI. The last 12 square degrees
Published 31-07-1998“…This paper presents the I-band data obtained by the ESO Imaging Survey (EIS) over two patches of the sky, 6 square degrees each, centered at $\alpha \sim…”
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ESO Imaging Survey V. Cluster Search using Color Data
Published 15-07-1998“…This paper presents 19 additional candidate clusters detected using the galaxy catalog extracted from the I-band images taken for the ESO Imaging Survey (EIS)…”
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Journal Article