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Publications of the Astronomical Society of Japan is a peer-reviewed journal published by Oxford University Press, covering Stellar, planetary, and galactic studies, Astrophysics and Star Formation Studies, Astrophysical Phenomena and Observations.
| Publisher | Oxford University Press |
|---|---|
| Reference style | Author–year (OUP) Author–year — (Smith, 2023) in the text Smith, A., Jones, B. and Lee, C. (2023) 'A representative article title', Publications of the Astronomical Society of Japan, 12(3), pp. 45–58.
Formats any DOI in the closest standard style — Publications of the Astronomical Society of Japan has no published style definition, so this is an approximation. No sign-up. |
| Publishes research in | Stellar, planetary, and galactic studies Astrophysics and Star Formation Studies Astrophysical Phenomena and Observations Astronomy and Astrophysical Research Galaxies: Formation, Evolution, Phenomena |
| ISSN | 0004-6264 |
| Citation impact (2-yr) | 2.83 |
| h-index | 135 |
| i10-index | 2,726 |
| Total citations | 128,652 |
| Article processing charge | $2,474 |
| Top institutions publishing here | The University of Tokyo |
| Journal website | academic.oup.com |
| 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.
The XIS is an X-ray Imaging Spectrometer system, consisting of state-of-the-art charge-coupled devices (CCDs) optimized for X-ray detection, camera bodies, and control electronics. Four sets of XIS sensors are placed at the focal planes of the grazing-incidence, nested thin-foil mirrors (XRT: X-Ray Telescope) onboard the Suzaku satellite. Three of the XIS sensors have front-illuminated CCDs,…
Abstract Hyper Suprime-Cam (HSC) is a wide-field imaging camera on the prime focus of the 8.2-m Subaru telescope on the summit of Mauna Kea in Hawaii. A team of scientists from Japan, Taiwan, and Princeton University is using HSC to carry out a 300-night multi-band imaging survey of the high-latitude sky. The survey includes three…
High-sensitivity wide-band X-ray spectroscopy is the key feature of the Suzaku X-ray observatory, launched on 2005 July 10. This paper summarizes the spacecraft, in-orbit performance, operations, and data processing that are related to observations. The scientific instruments, the high-throughput X-ray telescopes, X-ray CCD cameras, non-imaging hard X-ray detector are also described.
Abstract AKARI, the first Japanese satellite dedicated to infrared astronomy, was launched on 2006 February 21, and started observations in May of the same year. AKARI has a 68.5 cm cooled telescope, together with two focal-plane instruments, which survey the sky in six wavelength bands from mid–to far-infrared. The instruments also have a capability for…
Abstract The Monitor of All-sky X-ray Image (MAXI) mission is the first astronomical payload to be installed on the Japanese Experiment Module — Exposed Facility (JEM-EF or Kibo-EF) on the International Space Station. It has two types of X-ray slit cameras with wide FOVs and two kinds of X-ray detectors consisting of gas proportional counters…
