in The Magnetized Interstellar Medium

By B. Uyaniker, W. Reich, R. Wielebinski. 2004

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An absolutely calibrated survey of polarized emission from the northern sky at 1.4 GHz. Observations (2005, methodology): “The Effelsberg Medium Latitude Survey (EMLS) at 1.4 GHz (Uyaniker et al. 1998, 1999; Reich et al. 2004) has an angular resolution of 9.4′.”
Revisiting the radial distribution of pulsars in the Galaxy (2004, background): “Some improvements also may be achieved taking into account warp and flaring structure of the Galaxy (Yusifov 2003).”
Radio observational constraints on Galactic 3D-emission models (2007, background): “Spectral index maps show spatial variations of the spectral index and a spectral steepening at high frequencies is indicated (Reich et al. 2004).”
Revised equipartition and minimum energy formula for magnetic field strength estimates from radio synchrotron observations (2005, background): “Magnetic fields play an important role in supernova remnants (Fürst & Reich 2004), in the interstellar medium of galaxies (Beck et al. 1996; Beck 2004), in the intergalactic medium of clusters (Carilli & Taylor 2002), and in the jets and lobes of active galaxies (Rees 1985; Blandford 2001).”