Aims. We study polarized short-wavelength emission from the inner Galaxy, which is nearly invisible at long wavelengths because of depolarization. We attempt to obtain information on the diffuse continuum emission at short wavelengths to help us to separate Galactic thermal and non-thermal components. Methods. We conducted a total intensity and polarization survey of the Galactic plane at λ6 cm using the Urumqi 25 m telescope for the Galactic longitude range of 10° ≤ l ≤ 60° and the Galactic latitude range of |b| ≤ 5°. Missing absolute zero levels of Stokes U and Q maps were restored by extrapolating the WMAP five-year K-band polarization data. For total intensities, we recovered missing large-scale components by referring to the ...
Observations of the submillimetre emission from Galactic dust, in both total intensity I and polariz...
Context. Low-frequency radio continuum observations are best suited to search for radio halos of inc...
Aims. Interstellar polarization of starlight at high galactic latitudes gives information on the dir...
Aims.Polarization measurements of the Galactic plane at λ6 cm probe the interstellar medium (ISM) to...
(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...
We present 1420 MHz (lambda = 21 cm) observations of polarized emission from an area of 117 deg(2) i...
This paper presents an overview of the polarized sky as seen by Planck HFI at 353 GHz, whi...
Context. Observations of polarized emission are a significant source of information on the magnetic...
et al.This paper presents an overview of the polarized sky as seen by Planck HFI at 353 GHz, which i...
Received; accepted Context. Observations of polarized emission are a significant source of informati...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The da...
Aims. We study the polarisation properties, magnetic field strength, and synchrotron emission scale-...
Observations of the submillimetre emission from Galactic dust, in both total intensity I and polariz...
Context. Low-frequency radio continuum observations are best suited to search for radio halos of inc...
Aims. Interstellar polarization of starlight at high galactic latitudes gives information on the dir...
Aims.Polarization measurements of the Galactic plane at λ6 cm probe the interstellar medium (ISM) to...
(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...
We present 1420 MHz (lambda = 21 cm) observations of polarized emission from an area of 117 deg(2) i...
This paper presents an overview of the polarized sky as seen by Planck HFI at 353 GHz, whi...
Context. Observations of polarized emission are a significant source of information on the magnetic...
et al.This paper presents an overview of the polarized sky as seen by Planck HFI at 353 GHz, which i...
Received; accepted Context. Observations of polarized emission are a significant source of informati...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The da...
Aims. We study the polarisation properties, magnetic field strength, and synchrotron emission scale-...
Observations of the submillimetre emission from Galactic dust, in both total intensity I and polariz...
Context. Low-frequency radio continuum observations are best suited to search for radio halos of inc...
Aims. Interstellar polarization of starlight at high galactic latitudes gives information on the dir...