Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. The Global Magneto-ionic Medium Survey: A Faraday Depth Survey of the Northern Sky Covering 1280-1750 MHz
 

The Global Magneto-ionic Medium Survey: A Faraday Depth Survey of the Northern Sky Covering 1280-1750 MHz

Journal
THE ASTRONOMICAL JOURNAL  
Date Issued
2021
Author(s)
Wolleben, M.
•
Landecker, T. L.
•
Douglas, K. A.
•
Gray, A. D.
•
Ordog, A.
•
Dickey, J. M.
•
Hill, A. S.
•
CARRETTI, ETTORE  
•
Brown, J. C.
•
Gaensler, B. M.
•
Han, J. L.
•
Haverkorn, M.
•
Kothes, R.
•
Leahy, J. P.
•
McClure-Griffiths, N.
•
McConnell, D.
•
Reich, W.
•
Taylor, A. R.
•
Thomson, A. J. M.
•
West, J. L.
DOI
10.3847/1538-3881/abf7c1
Abstract
The Galactic interstellar medium hosts a significant magnetic field, which can be probed through the synchrotron emission produced from its interaction with relativistic electrons. Linearly polarized synchrotron emission is generated throughout the Galaxy and, at longer wavelengths, modified along nearly every path by Faraday rotation in the intervening magneto-ionic medium. Full characterization of the polarized emission requires wideband observations with many frequency channels. We have surveyed polarized radio emission from the Northern sky over the range 1280-1750 MHz, with channel width 236.8 kHz, using the John A. Galt Telescope (diameter 25.6 m) at the Dominion Radio Astrophysical Observatory, as part of the Global Magneto-Ionic Medium Survey. The survey covered 72% of the sky, decl. -30° to +87° at all R.A. The intensity scale was absolutely calibrated, based on the flux density and spectral index of Cygnus A. Polarization angle was calibrated using the extended polarized emission of the Fan Region. Data are presented as brightness temperatures with angular resolution 40'. Sensitivity in Stokes Q and U is 45 mK rms in a 1.18 MHz band. We have applied rotation measure synthesis to the data to obtain a Faraday depth cube of resolution 150 rad m-2 and sensitivity 3 mK rms of polarized intensity. Features in Faraday depth up to a width of 110 rad m-2 are represented. The maximum detectable Faraday depth is ±2 × 104 rad m-2. The survey data are available at the Canadian Astronomy Data Centre.
Volume
162
Issue
1
Start page
35
Uri
http://hdl.handle.net/20.500.12386/32266
Url
https://iopscience.iop.org/article/10.3847/1538-3881/abf7c1
https://arxiv.org/abs/2106.00945
Issn Identifier
0004-6256
Ads BibCode
2021AJ....162...35W
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

Wolleben_2021_AJ_162_35.pdf

Description
PDF editoriale
Size

5.52 MB

Format

Adobe PDF

Checksum (MD5)

31ac92fb3a6a5455863fb459b7d3b364

Loading...
Thumbnail Image
Name

2106.00945.pdf

Description
postprint
Size

6.87 MB

Format

Adobe PDF

Checksum (MD5)

f3b981eccab058a839a1bf9e9f6a5ffe

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback