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John M. Brewer

Researcher at San Francisco State University

Publications -  126
Citations -  5888

John M. Brewer is an academic researcher from San Francisco State University. The author has contributed to research in topics: Planet & Stars. The author has an hindex of 42, co-authored 120 publications receiving 5143 citations. Previous affiliations of John M. Brewer include Columbia University & Yale University.

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Spectral Properties Of Cool Stars : Extended Abundance Analysis Of 1,617 Planet-Search Stars

TL;DR: In this article, a catalog of uniformly determined stellar properties and abundances for 1,617 F, G, and K stars using an automated spectral synthesis modeling procedure was presented, and all stars were observed using a single image.
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Spectral Properties of Cool Stars: Extended Abundance Analysis of 1617 Planet Search Stars

TL;DR: In this paper, a catalog of uniformly determined stellar properties and abundances for 1626 F, G, and K stars using an automated spectral synthesis modeling procedure was presented using the HIRES spectrograph at Keck Observatory.
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On machine-learned classification of variable stars with sparse and noisy time-series data

TL;DR: In this article, a methodology for variable-star classification using machine learning techniques has been proposed, which can quickly and automatically produce calibrated classification probabilities for newly observed variables based on small numbers of time-series measurements.
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Planet Hunters IX. KIC 8462852-where's the flux?

TL;DR: In this paper, the authors made use of data from the first public release of the WASP data (Butters et al. 2010) as provided by the NASA Exoplanet Archive, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration under the ERC grant number 279973.
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On Machine-Learned Classification of Variable Stars with Sparse and Noisy Time-Series Data

TL;DR: A methodology for variable-star classification, drawing from modern machine-learning techniques, which is effective for identifying samples of specific science classes and presents the first astronomical use of hierarchical classification methods to incorporate a known class taxonomy in the classifier.