Astronomische Nachrichten Template
Write in a clean editor, then format for Astronomische Nachrichten in one click — DocuGuru applies the official Wiley template with author–year references and exports a submission-ready PDF plus the editable LaTeX source. Free to start.
About the Astronomische Nachrichten format
Astronomische Nachrichten is a peer-reviewed journal published by Wiley, covering History and Developments in Astronomy, Astro and Planetary Science, Stellar, planetary, and galactic studies.
| Publisher | Wiley |
|---|---|
| Reference style | Author–year (Chicago) Author–year — (Smith, 2023) in the text Smith, Ada, Ben Jones, and Cara Lee. 2023. "A Representative Article Title." Astronomische Nachrichten 12 (3): 45–58.
Formats any DOI in Astronomische Nachrichten style. No sign-up. |
| Publishes research in | History and Developments in Astronomy Astro and Planetary Science Stellar, planetary, and galactic studies Historical Astronomy and Related Studies Agriculture and Biological Studies |
| ISSN | 0004-6337 |
| Citation impact (2-yr) | 0.88 |
| h-index | 84 |
| i10-index | 1,400 |
| Total citations | 62,856 |
| Article processing charge | $3,140 |
| Top institutions publishing here | Leibniz Institute for Astrophysics Potsdam |
| Journal website | onlinelibrary.wiley.com |
| You get | A submission-ready PDF and the editable LaTeX source — ready to submit. |
Papers published in Astronomische Nachrichten per year
Citation impact of Astronomische Nachrichten by publication year
Citations each year’s papers have accumulated so far — the most recent years are still building up.
Most-cited papers in Astronomische Nachrichten
Abstract We summarize the Sloan Digital Sky Survey data acquisition and processing steps, and describe runQA , a pipeline designed for automated data quality assessment. In particular, we show how the position of the stellar locus in color‐color diagrams can be used to estimate the accuracy of photometric zeropoint calibration to better than 0.01 mag…
Abstract The commonly used classical equipartition or minimum‐energy estimate of total magnetic fields strengths from radio synchrotron intensities is of limited practical use because it is based on the hardly known ratio K of the total energies of cosmic ray protons and electrons and also has inherent problems. We present a revised formula, using the…
J e suis trhsreconnaissant de la prompte communication que vous nous avez faite de la lettre dc Mr. Gauss par votre circulaire du 5 Janvier.L a forme enceptionrrelle de I'urbite de cette comkte, qui Lit une espixe de transition B la forme des orbites planktaires, est un fait fort intQressant.Ce n'est qu'hier que j'ai eu…
Abstract Nichtspiegelsymmetrische turbulente Bewegungen in einem elektrisch leitenden fluiden Medium rufen im Mittel eine elektromotorische Kraft (EMK) α magnified image parallel zum mittleren Magnetfeld magnified image hervor. Dieser Effekt – im folgenden α‐Effekt genannt – kann zum selbsterregten Aufbau von Magnetfeldern aus schwachen Anfangsfeldern führen. Da eine Turbulenz in rotierenden Systemen auf Grund der Wirkung…