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most citedS-band Polarization All Sky Survey (S-PASS): survey description and maps

82 citations · 350 across the 10 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2022★ 9 cited

New continuum and polarization observations of the Cygnus Loop with FAST II. Images and analyses

X. H. Sun, X. Y. Gao, W. Reich +4

We present total-intensity and polarized-intensity images of the Cygnus Loop supernova remnant (SNR) observed by the Five-hundred-meter Aperture Spherical radio Telescope (FAST). T…

astro-ph.GA2022★ 8 cited

Turbulent magnetic field in the HII region Sh 2-27

N. C. Raycheva, M. Haverkorn, S. Ideguchi +7

Magnetic fields in the turbulent interstellar medium (ISM) are a key element in understanding Galactic dynamics, but there are many observational challenges. One useful probe for s…

astro-ph.GA2019★ 82 cited

S-band Polarization All Sky Survey (S-PASS): survey description and maps

E. Carretti, M. Haverkorn, L. Staveley-Smith +9

We present the S-Band Polarization All Sky Survey (S-PASS), a survey of polarized radio emission over the southern sky at Dec~ taken with the Parkes radio telescope at…

astro-ph.GA2018★ 10 cited

Revealing the Faraday Depth Structure of Radio Galaxy NGC 612 with Broad-Band Radio Polarimetric Observations

J. F. Kaczmarek, C. R. Purcell, B. M. Gaensler +3

We present full-polarisation, broadband observations of the radio galaxy NGC 612 (PKS B0131-637) from 1.3 to 3.1 GHz using the Australia Telescope Compact Array. The relatively lar…

astro-ph.GA2017★ 27 cited

The Fan Region at 1.5 GHz. I: Polarized synchrotron emission extending beyond the Perseus Arm

A. S. Hill, T. L. Landecker, E. Carretti +12

The Fan Region is one of the dominant features in the polarized radio sky, long thought to be a local (distance < 500 pc) synchrotron feature. We present 1.3-1.8 GHz polarized radi…

astro-ph.GA2015★ 60 cited

A radio-polarisation and rotation measure study of the Gum Nebula and its environment

C. R. Purcell, B. M. Gaensler, X. H. Sun +7

The Gum Nebula is 36 degree wide shell-like emission nebula at a distance of only 450 pc. It has been hypothesised to be an old supernova remnant, fossil HII region, wind-blown bub…