A ROTATION MEASURE IMAGE OF THE SKY

By A. Taylor, J. Stil, C. Sunstrum. 2009

284 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/0598069564cfdb309667e9e458a1b5e8d22c39c0

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Citations in the corpus

Complex Faraday depth structure of active galactic nuclei as revealed by broad‐band radio polarimetry (2012, methodology): “RMNVSS: derived using the same frequency coverage as in Taylor et al. (2009).”
A NEW MODEL OF THE GALACTIC MAGNETIC FIELD (2012, methodology): “The publicly available extragalactic RM data has increased by more than an order of magnitude since JFWE09, thanks to the re-analysis of NVSS polarization data by Taylor et al. (2009).”
Cosmological Magnetic Fields: Their Generation, Evolution and Observation (2013, background): “Recent accumulation of a large data base of Rotation Measures from extragalactic sources (Taylor et al 2009; Stil et al 2011) has enabled a significant improvement of the knowledge of the global structure of the Galactic magnetic field (Jansson and Farrar 2012a,b; Oppermann et al 2012).”
DERIVING THE GLOBAL STRUCTURE OF THE GALACTIC MAGNETIC FIELD FROM FARADAY ROTATION MEASURES OF EXTRAGALACTIC SOURCES (2011, background): “The first one is the compilation of RMs recently obtained by Taylor et al. (2009) who reanalyzed NRAO VLA Sky Survey (NVSS) data.”
THE GALACTIC MAGNETIC FIELD (2012, background): “The vertical component of the JF12 coherent local field is 0.2 µG, which is compatible with observational estimates (Han & Qiao 1994; Taylor et al. 2009; Mao et al. 2010).”
Science with the Murchison Widefield Array (2012, methodology): “These extragalactic source RMs will provide a “grid” (Beck & Gaensler 2004; Taylor et al. 2009) that can be used to model large-scale magnetic fields in the Milky Way and, if deeper observations can provide a sufficiently dense grid, in nearby galaxies.”
The case for electron re-acceleration at galaxy cluster shocks (2017, background): “Given the low Galactic Faraday Rotation Measure of≈ −7 rad m−1, we did not correct the polarization angles for Faraday Rotation [36].”
Estimating extragalactic Faraday rotation (2014, methodology): “2 as a function of Galactic latitude for the data from the NVSS RM catalog (Taylor et al. 2009).”
The Karl G. Jansky Very Large Array Sky Survey (VLASS). Science Case and Survey Design (2019, methodology): “Context NVSS has provided the wider astronomy community with a reliable reference image of the radio sky at Gigahertz frequencies for the past 20 years.”
The 511 keV emission from positron annihilation in the Galaxy (2010, background): “For the local halo, Taylor et al. (2009) obtained (Bu)Z ∼ −0.14 µG above the midplane (Z > 0) and (Bu)Z ∼ +0.30 µG below the midplane (Z < 0), whereas Mao et al. (2010) obtained (Bu)Z ∼ 0.00 µG toward the north Galactic pole and (Bu)Z ∼ +0.31 µG toward the south Galactic pole.”
Magnetic Fields in Galaxies (2010, background): “Taylor et al. (2009) and Mao et al. (2010) found a north-directed field of 0.30 µG below the Galactic plane.”
Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust (2014, methodology): “Using the catalogues of Brown et al. (2003), Brown et al. (2007), Taylor et al. (2009), and Van Eck et al. (2011), in Fig.”