Abstract The “Planetary Data System” (PDS) was developed and supported by the Solar System Exploration Division of the National Aeronautics and Space Administration (NASA) and has now successfully operated for a few years. Its primary objectives are to preserve data obtained from previous, current and future space missions; to help individual scientists in the analysis…
Highlights of Astronomy Template
Write in a clean editor, then format for Highlights of Astronomy in one click — DocuGuru applies the official Cambridge University Press template with numbered references and exports a submission-ready PDF plus the editable LaTeX source. Free to start.
About the Highlights of Astronomy format
Highlights of Astronomy is a peer-reviewed journal published by Cambridge University Press, covering Stellar, planetary, and galactic studies, Astro and Planetary Science, Astronomy and Astrophysical Research.
| 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, Highlights of Astronomy 12 (2023) 45–58.
Formats any DOI in the closest standard style — Highlights of Astronomy has no published style definition, so this is an approximation. No sign-up. |
| Publishes research in | Stellar, planetary, and galactic studies Astro and Planetary Science Astronomy and Astrophysical Research History and Developments in Astronomy Astrophysics and Star Formation Studies |
| ISSN | 1539-2996 |
| h-index | 26 |
| i10-index | 80 |
| Total citations | 4,810 |
| Top institutions publishing here | Observatoire de Paris |
| Journal website | www.iau.org |
| You get | A submission-ready PDF and the editable LaTeX source — ready to submit. |
Papers published in Highlights of Astronomy per year
Citation impact of Highlights of Astronomy by publication year
Citations each year’s papers have accumulated so far — the most recent years are still building up.
Most-cited papers in Highlights of Astronomy
Abstract We have measured the dynamical mass of the highly luminous star cluster W3 in the young merger remnant galaxy NGC 7252. The value is M dyn = (8 ± 2) × 10 7 M ⊙ , and represents the highest dynamically-confirmed mass for an extra-galactic star cluster so far. The dynamical mass is in…
Due to weather-related travel delays Dr. McCarthy was unable to present his scheduled paper. In his absence, however, Dr. K. Yokoyama, Chairman of the International Earth Rotation Service (IERS), reported on the status of the revision of the IERS Standards carried out by McCarthy who provided the following precis. These standards are meant to be…
Abstract Historical records are available for nine supernova explosions seen in our Galaxy over the last two millennia. The observations of these ‘historical’ supernovae are very useful for the modern astrophysical interpretation of the remnants of these supernovae. The ages of the remnants of these historical supernovae are definitively known, which greatly aids understanding of…
Abstract In the future, the ephemerides produced at JPL will be based upon the reference frame of the radio source catalogues. Recent planetary observations have been made directly with respect to the radio frame, and these observations have shown a satisfying degree of absolute accuracy and internal consistency; they provide an automatic frame-tie.