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Article 2018-04

Autor: Muirhead, P.S. Dressing, C.D. Mann, A.W. Rojas-Ayala, B. Lépine, S. Paegert, M. De Lee, N. Oelkers, R.

We present a catalog of cool dwarf targets (V - > J 2.7, T eff ≳4000 K) and their stellar properties for the upcoming Transiting Exoplanet Survey Satellite (TESS), for the purpose of determining which cool dwarfs should be observed using two minute observations. TESS has the opportunity to search...

Enlace original: http://repositorio.unab.cl/xmlui/handle/ria/8556

Repositorio Universidad Andrés Bello
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Muirhead, P.S. ,  Dressing, C.D. ,  Mann, A.W. ,  Rojas-Ayala, B. ,  Lépine, S. ,  Paegert, M. ,  De Lee, N. ,  Oelkers, R. ,  [A Catalog of Cool Dwarf Targets for the Transiting Exoplanet Survey Satellite] ,  A Catalog of Cool Dwarf Targets for the Transiting Exoplanet Survey Satellite
Article 2018-09

Autor: Stassun, K.G. Oelkers, R.J. Pepper, J. Paegert, M. Lee, N.D. Torres, G. Latham, D.W. Charpinet, S. Dressing, C.D. Huber, D. Kane, S.R. Lépine, S. Mann, A. Muirhead, P.S. Rojas-Ayala, B. Silvotti, R. Fleming, S.W. Levine, A. Plavchan, P.

The Transiting Exoplanet Survey Satellite (TESS) will be conducting a nearly all-sky photometric survey over two years, with a core mission goal to discover small transiting exoplanets orbiting nearby bright stars. It will obtain 30 minute cadence observations of all objects in the TESS fields of...

Enlace original: http://repositorio.unab.cl/xmlui/handle/ria/11143

Repositorio Universidad Andrés Bello
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Stassun, K.G. ,  Oelkers, R.J. ,  Pepper, J. ,  Paegert, M. ,  Lee, N.D. ,  Torres, G. ,  Latham, D.W. ,  Charpinet, S. ,  Dressing, C.D. ,  Huber, D. ,  Kane, S.R. ,  Lépine, S. ,  Mann, A. ,  Muirhead, P.S. ,  Rojas-Ayala, B. ,  Silvotti, R. ,  Fleming, S.W. ,  Levine, A. ,  Plavchan, P. ,  [The TESS Input Catalog and Candidate Target List] ,  The TESS Input Catalog and Candidate Target List
Article 2018

Autor: Zhao, L. Fischer, D.A. Brewer, J. Giguere, M. Rojas-Ayala, B.

We use more than a decade of radial-velocity measurements for α Cen A, B, and Proxima Centauri from the High Accuracy Radial Velocity Planet Searcher, CTIO High Resolution Spectrograph, and the Ultraviolet and Visual Echelle Spectrograph to identify the M i sin and orbital periods of planets that...

Enlace original: http://repositorio.unab.cl/xmlui/handle/ria/6357

Repositorio Universidad Andrés Bello
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Zhao, L. ,  Fischer, D.A. ,  Brewer, J. ,  Giguere, M. ,  Rojas-Ayala, B. ,  [Planet Detectability in the Alpha Centauri System] ,  Planet Detectability in the Alpha Centauri System

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