All-sky angular power spectrum ā I. Estimating brightness temperature fluctuations using the 150-MHz TGSS survey
| dc.contributor.author | Ghosh, Abhik | |
| dc.contributor.author | Choudhuri, Samir | |
| dc.contributor.author | Roy, Nirupam | |
| dc.date.accessioned | 2021-02-10T10:14:36Z | |
| dc.date.available | 2021-02-10T10:14:36Z | |
| dc.date.issued | 2020 | |
| dc.description.abstract | Measurements of the Galactic synchrotron emission are important for the 21-cm studies of the epoch of reionization. The study of synchrotron emission is also useful for quantifying the fluctuations in the magnetic field and the cosmic-ray electron density of the turbulent interstellar medium (ISM) of our Galaxy. Here, we present the all-sky angular power spectrum (Cā) measurements of the diffuse synchrotron emission obtained using the TIFR GMRT Sky Survey (TGSS) at 150 MHz. | en_US |
| dc.identifier.citation | Ghosh, A. et al. (2020). All-sky angular power spectrum ā I. Estimating brightness temperature fluctuations using the 150-MHz TGSS survey. Monthly Notices of the Royal Astronomical Society, 494(2), 1936ā1945 | en_US |
| dc.identifier.issn | 1365-2966 | |
| dc.identifier.uri | https://doi.org/10.1093/mnras/staa762 | |
| dc.identifier.uri | http://hdl.handle.net/10566/5882 | |
| dc.language.iso | en | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.subject | Methods: data analysis | en_US |
| dc.subject | Methods: statistical | en_US |
| dc.subject | Techniques: interferometric | en_US |
| dc.subject | Dark ages | en_US |
| dc.subject | Radio continuum: general | en_US |
| dc.title | All-sky angular power spectrum ā I. Estimating brightness temperature fluctuations using the 150-MHz TGSS survey | en_US |
| dc.type | Book | en_US |