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LOFAR Deep Fields: Probing faint Galactic polarised emission in ELAIS-N1

Šnidarić, Iva; Jelić, Vibor; Mevius, Maaijke; Brentjens, Michiel; Erceg, Ana; Shimwell, Timothy W.; Piras, Sara; Horellou, Cathy; Sabater, Jose; Best, Philip N.; Bracco, Andrea; Ceraj, Lana; Haverkorn, Marijke; O’Sullivan, Shane P.; Turić, Luka; Vacca, Valentina (2023) LOFAR Deep Fields: Probing faint Galactic polarised emission in ELAIS-N1. Astronomy & Astrophysics, 674 . ISSN 0004-6361

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Abstract

We present the first deep polarimetric study of Galactic synchrotron emission at low radio frequencies. Our study is based on 21 observations of the European Large Area Infrared Space Observatory Survey-North 1 (ELAIS-N1) field using the Low-Frequency Array (LOFAR) at frequencies from 114.9 to 177.4 MHz. These data are a part of the LOFAR Two-metre Sky Survey Deep Fields Data Release 1. We used very low-resolution (4.3') Stokes QU data cubes of this release. We applied rotation measure (RM) synthesis to decompose the distribution of polarised structures in Faraday depth, and cross-correlation RM synthesis to align different observations in Faraday depth. We stacked images of about 150 h of the ELAIS-N1 observations to produce the deepest Faraday cube at low radio frequencies to date, tailored to studies of Galactic synchrotron emission and the intervening magneto-ionic interstellar medium. This Faraday cube covers ~36 deg2 of the sky and has a noise of 27 µJy PSF-1 RMSF-1 in polarised intensity. This is an improvement in noise by a factor of approximately the square root of the number of stacked data cubes (~√20), as expected, compared to the one in a single data cube based on five-to-eight-hour observations. We detect a faint component of diffuse polarised emission in the stacked cube, which was not detected previously. Additionally, we verify the reliability of the ionospheric Faraday rotation corrections estimated from the satellite-based total electron content measurements to be of ~0.05 gad m-2. We also demonstrate that diffuse polarised emission itself can be used to account for the relative ionospheric Faraday rotation corrections with respect to a reference observation.

Item Type: Article
Uncontrolled Keywords: ISM: general; ISM: structure; ISM: magnetic fields; radio continuum: ISM; techniques: interferometric; techniques: polarimetric
Subjects: NATURAL SCIENCES > Physics > Astronomy and Astrophysics
Divisions: Division of Experimental Physics
Projects:
Project titleProject leaderProject codeProject type
Razumijevanje zračenja na niskim radio frekvencijama: ususret novoj generaciji radio teleskopa-LowFreqCROVibor Jelić; Vernesa Smolčić; Željka Marija Bošnjak; Bruno ŠlausIP-2018-01-2889HRZZ
Depositing User: Vibor Jelić
Date Deposited: 07 Feb 2024 09:59
URI: http://fulir.irb.hr/id/eprint/8528
DOI: 10.1051/0004-6361/202245124

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