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Publications of the Astronomical Society of Australia is a peer-reviewed journal published by Cambridge University Press, covering Stellar, planetary, and galactic studies, Astronomy and Astrophysical Research, Galaxies: Formation, Evolution, Phenomena.
| Publisher | Cambridge University Press |
|---|---|
| Reference style | Numbered Numbered — [1], [2] in the text [1] A. Smith, B. Jones, and C. Lee, A representative article title, Publications of the Astronomical Society of Australia 12 (2023) 45–58.
Formats any DOI in the closest standard style — Publications of the Astronomical Society of Australia has no published style definition, so this is an approximation. No sign-up. |
| Publishes research in | Stellar, planetary, and galactic studies Astronomy and Astrophysical Research Galaxies: Formation, Evolution, Phenomena Astrophysics and Star Formation Studies Radio Astronomy Observations and Technology |
| ISSN | 1323-3580 |
| Citation impact (2-yr) | 2.63 |
| h-index | 100 |
| i10-index | 937 |
| Total citations | 53,939 |
| Top institutions publishing here | Commonwealth Scientific and Industrial Research Organisation |
| Journal website | journals.cambridge.org |
| You get | A submission-ready PDF and the editable LaTeX source — ready to submit. |
Citations each year’s papers have accumulated so far — the most recent years are still building up.
Abstract The Murchison Widefield Array (MWA) is one of three Square Kilometre Array Precursor telescopes and is located at the Murchison Radio-astronomy Observatory in the Murchison Shire of the mid-west of Western Australia, a location chosen for its extremely low levels of radio frequency interference. The MWA operates at low radio frequencies, 80–300 MHz, with…
Abstract A new set of software applications and libraries for use in the archival and analysis of pulsar astronomical data is introduced. Known collectively as the psrchive scheme, the code was developed in parallel with a new data storage format called psrfits , which is based on the Flexible Image Transport System (FITS). Both of…
Abstract The Binary Population and Spectral Synthesis suite of binary stellar evolution models and synthetic stellar populations provides a framework for the physically motivated analysis of both the integrated light from distant stellar populations and the detailed properties of those nearby. We present a new version 2.1 data release of these models, detailing the methodology…
Abstract This paper presents SPLASH , a publicly available interactive visualisation tool for Smoothed Particle Hydrodynamics (SPH) simulations. Visualisation of SPH data is more complicated than for grid-based codes because the data are defined on a set of irregular points and therefore requires a mapping procedure to a two dimensional pixel array. This means that,…
Abstract Given the growing use of Sérsic's (1963, 1968) R 1/ n model for describing the stellar distributions in galaxies, and the lack of any single reference that provides the various associated mathematical expressions, we have endeavoured to compile such a resource here. We present the standard intensity profile, and its various guises such as…
