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Maria Teresa Ruiz

Researcher at University of Chile

Publications -  138
Citations -  6648

Maria Teresa Ruiz is an academic researcher from University of Chile. The author has contributed to research in topics: Stars & White dwarf. The author has an hindex of 37, co-authored 137 publications receiving 6239 citations. Previous affiliations of Maria Teresa Ruiz include Novartis & Association of Universities for Research in Astronomy.

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Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager

Bruce Macintosh, +94 more
- 02 Oct 2015 - 
TL;DR: Using the Gemini Planet Imager, a Jupiter-like planet is discovered orbiting the ~20-million-year-old star 51 Eridani at a projected separation of 13 astronomical units and has a methane signature and is probably the smallest exoplanet that has been directly imaged.
Journal ArticleDOI

Vvv dr1: the first data release of the milky way bulge and southern plane from the near-infrared eso public survey vista variables in the via lactea

R. K. Saito, +121 more
TL;DR: The ESO VISTA public survey VISTA variables in the V�a L�ctea (VVV) started in 2010 and is expected to run for about five years.
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A comprehensive spectroscopic analysis of db white dwarfs

TL;DR: In this paper, a detailed analysis of 108 helium-line (DB) white dwarfs based on model atmosphere fits to high signal-to-noise optical spectroscopy is presented.
Journal ArticleDOI

Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager

Bruce Macintosh, +94 more
TL;DR: In this paper, the Gemini Planet Imager was used to detect a planet orbiting the star 51 Eridani at a projected separation of 13 astronomical units, with a spectrum with strong methane and water vapor absorption.
Journal ArticleDOI

A spectroscopic survey and analysis of bright, hydrogen-rich white dwarfs*

TL;DR: In this article, the authors conducted a survey of over 1300 bright (V ≤ 17.5), hydrogen-rich white dwarfs based largely on the last published version of the McCook & Sion catalog.