GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey III: South Galactic Pole data release

被引:7
|
作者
Franzen, T. M. O. [1 ,2 ]
Hurley-Walker, N. [1 ]
White, S. V. [1 ,3 ]
Hancock, P. J. [1 ]
Seymour, N. [1 ]
Kapinska, A. D. [4 ,5 ]
Staveley-Smith, L. [4 ,6 ]
Wayth, R. B. [1 ,6 ]
机构
[1] Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia
[2] ASTRON Netherlands Inst Radio Astron, POB 2, NL-7990 AA Dwingeloo, Netherlands
[3] Rhodes Univ, Dept Phys & Elect, POB 94, ZA-6140 Grahamstown, South Africa
[4] Univ Western Australia, Int Ctr Radio Astron Res, Crawley 6009, Australia
[5] Natl Radio Astron Observ, 1003 Lopezville Rd, Socorro, NM 87801 USA
[6] ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Stromlo, ACT, Australia
关键词
radio continuum: galaxies; surveys; catalogues; methods: data analysis; techniques: interferometric;
D O I
10.1017/pasa.2021.5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the South Galactic Pole (SGP) data release from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey. These data combine both years of GLEAM observations at 72-231 MHz conducted with the Murchison Widefield Array (MWA) and cover an area of 5 113deg(2) centred on the SGP at 20(h)40(m) < RA < 05(h)04(m) and -48 degrees < Dec < -2 degrees. At 216 MHz, the typical rms noise is approximate to 5 mJy beam(-1) and the angular resolution approximate to 2 arcmin. The source catalogue contains a total of 108 851 components above 5 sigma, of which 77% have measured spectral indices between 72 and 231 MHz. Improvements to the data reduction in this release include the use of the GLEAM Extragalactic catalogue as a sky model to calibrate the data, a more efficient and automated algorithm to deconvolve the snapshot images, and a more accurate primary beam model to correct the flux scale. This data release enables more sensitive large-scale studies of extragalactic source populations as well as spectral variability studies on a one-year timescale.
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页数:10
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