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Research Notes of the AAS is a peer-reviewed journal published by American Astronomical Society, covering Stellar, planetary, and galactic studies, Astronomy and Astrophysical Research, Astrophysics and Star Formation Studies. Over its lifetime it has published 2,440 papers, which have received 7,690 citations.
| Publisher | American Astronomical Society |
|---|---|
| Reference style | Author–year (AAS) Author–year — (Smith, 2023) in the text Smith, A., Jones, B., & Lee, C. 2023, Research Notes of the AAS, 12, 45
Formats any DOI in Research Notes of the AAS style. No sign-up. |
| Publishes research in | Stellar, planetary, and galactic studies Astronomy and Astrophysical Research Astrophysics and Star Formation Studies Gamma-ray bursts and supernovae Astro and Planetary Science |
| ISSN | 2515-5172 |
| Citation impact (2-yr) | 0.94 |
| h-index | 35 |
| i10-index | 162 |
| Top institutions publishing here | Sorbonne Université |
| Journal website | iopscience.iop.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 Transiting Exoplanet Survey Satellite (TESS) is the first high-precision full-sky photometric survey in space. We extracted light curves from a magnitude limited set of stars and other stationary luminous objects from the TESS Full Frame Images using the MIT Quick Look Pipeline. Here, we describe the techniques used to create light curves.
Abstract We present light curves from a magnitude limited set of stars and other stationary luminous objects from the TESS Full Frame Images, as reduced by the MIT Quick Look Pipeline (QLP). Our light curves cover the full two-year TESS Primary Mission and include ∼14,770,000 and ∼9,600,000 individual light curve segments in the Southern and…
We announce barycorrpy (BCPy) , a Python implementation to calculate precise barycentric corrections well below the 1 cm/s level, following the algorithm of Wright and Eastman (2014). This level of precision is required in the search for 1 Earth mass planets in the Habitable Zones of Sun-like stars by the Radial Velocity (RV) method, where…
When LSST begins surveying the sky, it is expected to produce a stream of up to 10^7 transients per night. This time domain stream of data will need to be rapidly mined, with digestible alerts produced in a timely manner. Since early 2018, the Zwicky Transient Factory (ZTF) has been producing alerts at a rate…
