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Open AccessJournal ArticleDOI

Considerations for a Multi-beam Multi-purpose Survey with FAST

TLDR
In this paper, the authors devised a survey plan to utilize the full sensitivity of FAST, while minimizing the complexities in operation the system and taking continuous data streams while the surface shape and the focal cabin stay fixed.
Abstract
Having achieved 'first-light' right before the opening ceremony on September 25, 2016, the Five-hundred-meter Aperture Spherical radio Telescope (FAST) is being busily commissioned Its innovative design requires ~1000 points to be measured and driven instead of just the two axes of motion, eg Azimuth and Elevation for most of the conventional antennae, to realize pointing and tracking We have devised a survey plan to utilized the full sensitivity of FAST, while minimizing the complexities in operation the system The 19-beam L band focal plan array will be rotated to specific angles and taking continuous data streams while the surface shape and the focal cabin stay fixed Such a survey will cover the northern sky in about 220 full days Our aim is to obtain data for pulsar search, HI (neutral hydrogen) galaxies, HI imaging, and radio transients, simultaneously, through multiple backends These data sets could be a significant contribution to all related fields in radio astronomy and remain relevant for decades

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Journal ArticleDOI

WALLABY – an SKA Pathfinder H i survey

B. S. Koribalski, +81 more
TL;DR: The Widefield ASKAP L-band Legacy All-sky Blind Survey (wallaby) as discussed by the authors is a next-generation survey of neutral hydrogen (H i) in the Local Universe, which uses the widefield, high-resolution capability of the Australian Square Kilometer Array Pathfinder (ASKAP), a radio interferometer consisting of 36 dishes equipped with Phased-Array Feeds.
Journal ArticleDOI

The fundamental performance of FAST with 19-beam receiver at L band

TL;DR: In this paper, the Five-hundred-meter Aperture Spherical radio Telescope (FAST) passed national acceptance and is taking pilot cycle of 'Shared-Risk' observations.
Journal ArticleDOI

On the FRB luminosity function - - II. Event rate density

TL;DR: In this article, the authors measured the FRB luminosity function using 46 known FRBs and found that the expected FRB event rate density at the upper cut-off luminosity is 2.9.
Journal ArticleDOI

FRB Energetics and detectability from high redshifts

TL;DR: In this paper, the authors estimate the upper limit redshifts of known FRBs using the dispersion measure (DM) - redshift ($z) relation and derive the upper- limit peak luminosity and energy of FRBs within the observational band.
References
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Journal ArticleDOI

The five-hundred-meter aperture spherical radio telescope (fast) project

TL;DR: Wang et al. as discussed by the authors proposed the Five Hundred Meter Aperture Spherical Radio Telescope (FAST) to build the largest single-dish radio telescope in the world.
Journal ArticleDOI

The VLA Galactic Plane Survey

TL;DR: The VLA Galactic Plane Survey (VGPS) is a survey of H I and 21 cm continuum emission in the Galactic plane between longitude 18° and 67° with latitude coverage from | b| < 13 to |b| < 23 as discussed by the authors.
Journal ArticleDOI

The Southern Galactic Plane Survey: H I Observations and Analysis

TL;DR: The Southern Galactic Plane Survey (SGPS) as mentioned in this paper is a large-scale project to image at arcminute resolution the H I spectral line and 21 cm continuum emission in parts of the plane of the Milky Way.
Journal ArticleDOI

The parkes Southern pulsar Survey — I. Observing and data analysis systems and initial results

TL;DR: The Australia Telescope National Facility (ATN), CSIRO, PO Box 76, Epping NSW 2121, Australia Wuffield Radio Astronomy Laboratories, University of Manchester, lodrell Bank, Macclesfield, Cheshire SKII 9DL 3Istituto di Radioastronomia del CNR, Via Gobetti 101, 40129 Bologna, Italy as discussed by the authors, Via Archirafi 36, 90123 Palermo, Italy
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