The Southern Galactic Plane Survey (SGPS) is an H I and 1.4 GHz continuum survey of the fourth quadrant of the Galaxy at arcminute resolution. We present here results on linearly polarized continuum emission from an initial 28 deg2 test region for the SGPS, consisting of 190 mosaicked pointings of the Australia Telescope Compact Array and covering the range 325.5d<l<332.5d, -0.5d<b<3.5d. Complicated extended structure is seen in linear polarization throughout the test region, almost all of which has no correlation with total intensity. We interpret the brightest regions of polarized emission as representing intrinsic structure in extended polarization, most likely originating in the Crux spiral arm at a distance of 3.5 kpc; fainter polarize...
We discuss observations of the linearly polarized component of the diffuse galactic radio background...
LAL 04-91International audienceWe present the first determination of the Galactic polarized emission...
We have analyzed the available polarization surveys of the Galactic emission to estimate to what ext...
The Southern Galactic Plane Survey (SGPS) is an H I and 1.4 GHz continuum survey of the fourth quadr...
We present 1420 MHz (lambda = 21 cm) observations of polarized emission from an area of 117 deg(2) i...
(Abridged) Polarization measurements of the Galactic plane at lambda6 cm probe the interstellar medi...
We present high-sensitivity and absolutely calibrated images of diffuse radio polarization at a reso...
Context. Observations of polarized emission are a significant source of information on the magnetic...
Received; accepted Context. Observations of polarized emission are a significant source of informati...
Context. Linear polarization of Galactic synchrotron emission provides valuable information on the G...
The Southern Galactic Plane Survey (SGPS) is an effort to map the southern Galaxy in the HI line and...
Polarimetric results from the Parkes 2.4-GHz survey of the southern Galactic plane are presented. Th...
We present WSRT observations at low frequencies (315-388 MHz) of the diffuse polarized emission in a...
Abstract. The polarized component of the diffuse radio synchrotron emission of our Galaxy shows stru...
Abstract: We present multi-frequency polarization observations of the diffuse radio synchrotron back...
We discuss observations of the linearly polarized component of the diffuse galactic radio background...
LAL 04-91International audienceWe present the first determination of the Galactic polarized emission...
We have analyzed the available polarization surveys of the Galactic emission to estimate to what ext...
The Southern Galactic Plane Survey (SGPS) is an H I and 1.4 GHz continuum survey of the fourth quadr...
We present 1420 MHz (lambda = 21 cm) observations of polarized emission from an area of 117 deg(2) i...
(Abridged) Polarization measurements of the Galactic plane at lambda6 cm probe the interstellar medi...
We present high-sensitivity and absolutely calibrated images of diffuse radio polarization at a reso...
Context. Observations of polarized emission are a significant source of information on the magnetic...
Received; accepted Context. Observations of polarized emission are a significant source of informati...
Context. Linear polarization of Galactic synchrotron emission provides valuable information on the G...
The Southern Galactic Plane Survey (SGPS) is an effort to map the southern Galaxy in the HI line and...
Polarimetric results from the Parkes 2.4-GHz survey of the southern Galactic plane are presented. Th...
We present WSRT observations at low frequencies (315-388 MHz) of the diffuse polarized emission in a...
Abstract. The polarized component of the diffuse radio synchrotron emission of our Galaxy shows stru...
Abstract: We present multi-frequency polarization observations of the diffuse radio synchrotron back...
We discuss observations of the linearly polarized component of the diffuse galactic radio background...
LAL 04-91International audienceWe present the first determination of the Galactic polarized emission...
We have analyzed the available polarization surveys of the Galactic emission to estimate to what ext...