Spectral-Line Observations Using a Phased Array Feed on the Parkes Telescope
dc.contributor.author | Reynolds, T. | |
dc.contributor.author | Staveley-Smith, L. | |
dc.contributor.author | Rhee, J. | |
dc.contributor.author | Westmeier, T. | |
dc.contributor.author | Chippendale, A. | |
dc.contributor.author | Deng, X. | |
dc.contributor.author | Ekers, Ronald | |
dc.contributor.author | Kramer, M. | |
dc.date.accessioned | 2017-11-28T06:37:18Z | |
dc.date.available | 2017-11-28T06:37:18Z | |
dc.date.created | 2017-11-28T06:21:50Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | Reynolds, T. and Staveley-Smith, L. and Rhee, J. and Westmeier, T. and Chippendale, A. and Deng, X. and Ekers, R. et al. 2017. Spectral-Line Observations Using a Phased Array Feed on the Parkes Telescope. Publications of the Astronomical Society of Australia. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/58827 | |
dc.identifier.doi | 10.1017/pasa.2017.45 | |
dc.description.abstract |
Copyright © Astronomical Society of Australia 2017 We present first results from pilot observations using a phased array feed (PAF) mounted on the Parkes 64-m radio telescope. The observations presented here cover a frequency range from 1 150 to 1 480 MHz and are used to show the ability of PAFs to suppress standing wave problems by a factor of ~10, which afflict normal feeds. We also compare our results with previous HIPASS observations and with previous H i images of the Large Magellanic Cloud. Drift scan observations of the GAMA G23 field resulted in direct H i detections at z = 0.0043 and z = 0.0055 of HIPASS galaxies J2242-30 and J2309-30. Our new measurements generally agree with archival data in spectral shape and flux density, with small differences being due to differing beam patterns. We also detect signal in the stacked H i data of 1 094 individually undetected galaxies in the GAMA G23 field in the redshift range 0.05 ? z ? 0.075. Finally, we use the low standing wave ripple and wide bandwidth of the PAF to set a 3s upper limit to any positronium recombination line emission from the Galactic Centre of < 0.09 K, corresponding to a recombination rate of < 3.0 × 10 45 s -1 . | |
dc.publisher | Cambridge University Press | |
dc.title | Spectral-Line Observations Using a Phased Array Feed on the Parkes Telescope | |
dc.type | Journal Article | |
dcterms.source.issn | 1323-3580 | |
dcterms.source.title | Publications of the Astronomical Society of Australia | |
curtin.department | Curtin Institute of Radio Astronomy (Engineering) | |
curtin.accessStatus | Fulltext not available |
Files in this item
Files | Size | Format | View |
---|---|---|---|
There are no files associated with this item. |