| DOI | Resolve DOI: https://doi.org/10.1093/mnras/staa1658 |
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| Author | Search for: Ng, C.ORCID identifier: https://orcid.org/0000-0002-3616-5160; Search for: Pandhi, A.; Search for: Naidu, A.; Search for: Fonseca, E.; Search for: Kaspi, V. M.; Search for: Masui, K. W; Search for: Mckinven, R.; Search for: Renard, A.; Search for: Scholz, P.1; Search for: Stairs, I. H.; Search for: Tendulkar, S. P.; Search for: Vanderlinde, K. |
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| Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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| Format | Text, Article |
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| Subject | techniques: polarimetric; pulsars: general; ISM: magnetic fields |
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| Abstract | Using commissioning data from the first year of operation of the Canadian Hydrogen Intensity Mapping Experiment’s (CHIME) Pulsar backend system, we conduct a systematic analysis of the Faraday Rotation Measure (RM) of the Northern hemisphere pulsars detected by CHIME. We present 55 new RMs as well as obtain improved RM uncertainties for 25 further pulsars. CHIME’s low observing frequency and wide bandwidth between 400 and 800 MHz contribute to the precision of our measurements, whereas the high cadence observation provides extremely high signal-to-noise co-added data. Our results represent a significant increase of the pulsar RM census, particularly regarding the Northern hemisphere. These new RMs are for sources that are located in the Galactic plane out to 10 kpc, as well as off the plane to a scale height of ∼16 kpc. This improved knowledge of the Faraday sky will contribute to future Galactic large-scale magnetic structure and ionosphere modelling. |
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| Publication date | 2020-08-11 |
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| Publisher | Royal Astronomical Society |
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| In | |
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| Language | English |
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| Peer reviewed | Yes |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 85eceffd-5976-413a-b363-7bc04741f76d |
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| Record created | 2022-03-09 |
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| Record modified | 2022-03-09 |
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