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Journal of Astronomical Instrumentation is a peer-reviewed journal published by World Scientific, covering Radio Astronomy Observations and Technology, Stellar, planetary, and galactic studies, Adaptive optics and wavefront sensing.
| Publisher | World Scientific |
|---|---|
| Reference style | Superscript numbered (World Scientific) Superscript — small raised numerals in the text 1. Smith, A., Jones, B. & Lee, C. A representative article title. Journal of Astronomical Instrumentation 12, 45–58 (2023).
Formats any DOI in the closest standard style — Journal of Astronomical Instrumentation has no published style definition, so this is an approximation. No sign-up. |
| Publishes research in | Radio Astronomy Observations and Technology Stellar, planetary, and galactic studies Adaptive optics and wavefront sensing Astrophysics and Cosmic Phenomena Astronomy and Astrophysical Research |
| ISSN | 2251-1717 |
| Citation impact (2-yr) | 0.69 |
| h-index | 34 |
| i10-index | 93 |
| Total citations | 3,688 |
| Top institutions publishing here | Center for Astrophysics Harvard & Smithsonian |
| Journal website | www.worldscientific.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.
We introduce Probing Radio Intensity at high-Z from Marion (PRI Z M), a new experiment designed to measure the globally averaged sky brightness, including the expected redshifted 21[Formula: see text]cm neutral hydrogen absorption feature arising from the formation of the first stars. PRI Z M consists of two dual-polarization antennas operating at central frequencies of…
High-resolution Airborne Wide-band Camera (HAWC[Formula: see text]) is the facility far-infrared imager and polarimeter for SOFIA, NASA’s Stratospheric Observatory for Infrared Astronomy. It is designed to cover the portion of the infrared spectrum that is completely inaccessible to ground-based observatories and which is essential for studies of astronomical sources with temperatures between tens and hundreds…
The first station of the Long Wavelength Array (LWA1) was completed in April 2011 and is currently performing observations resulting from its first call for proposals in addition to a continuing program of commissioning and characterization observations. The instrument consists of 258 dual-polarization dipoles, which are digitized and combined into beams. Four independently-steerable dual-polarization beams…
The Collaboration for Astronomy Signal Processing and Electronics Research (CASPER) has been working for a decade to reduce the time and cost of designing, building and deploying new digital radio-astronomy instruments. Today, CASPER open-source technology powers over 45 scientific instruments worldwide, and is used by scientists and engineers at dozens of academic institutions. In this…
We present the performance of the upGREAT heterodyne array receivers on the SOFIA telescope after several years of operations. This instrument is a multi-pixel high resolution ([Formula: see text]) spectrometer for the Stratospheric Observatory for Far-Infrared Astronomy (SOFIA). The receivers use 7-pixel subarrays configured in a hexagonal layout around a central pixel. The low frequency…
