Author pages are created from data sourced from our academic publisher partnerships and public sources.
- Publications
- Influence
Trumpeting M dwarfs with CONCH-SHELL: a catalogue of nearby cool host-stars for habitable exoplanets and life
We present an all-sky catalog of 2970 nearby (d . 50 pc), bright (J < 9) M- or late Ktype dwarf stars, 86% of which have been confirmed by spectroscopy. This catalog will be useful for searches for… Expand
Magnetic Activity Cycles in the Exoplanet Host Star epsilon Eridani
- T. Metcalfe, A. Buccino, +7 authors S. Basu
- Physics
- 18 December 2012
The active K2 dwarf epsilon Eri has been extensively characterized, both as a young solar analog and more recently as an exoplanet host star. As one of the nearest and brightest stars in the sky, it… Expand
The Muscles Treasury Survey. I. Motivation and Overview
- K. France, R. Loyd, +18 authors Kolby L. Weisenburger
- Physics
- 29 February 2016
Ground- and space-based planet searches employing radial velocity techniques and transit photometry have detected thousands of planet-hosting stars in the Milky Way. With so many planets discovered,… Expand
The rotation-lithium depletion correlation in the β Pictoris association and the LDB age determination
- S. Messina, A. Lanzafame, +9 authors R. Petrucci
- Physics
- 22 July 2016
Context. Evidence exists in the 125-Myr Pleiades cluster, and more recently in the 5-Myr NGC 2264 cluster, to show that rotation plays a key role in lithium (Li) depletion processes among low-mass… Expand
Mg II h + k emission lines as stellar activity indicators of main sequence F-K stars
- A. Buccino, P. Mauas
- Physics
- 7 April 2008
Context. The largest dataset of stellar activity measurements available at present is the one obtained at the Mount Wilson Observatory, where high-precision Ca II H+K uxes have been measured from… Expand
Semi-empirical Modeling of the Photosphere, Chromosphere, Transition Region, and Corona of the M-dwarf Host Star GJ 832
- J. Fontenla, J. Linsky, +5 authors L. Walkowicz
- Physics
- 2 August 2016
Stellar radiation from X-rays to the visible provides the energy that controls the photochemistry and mass loss from exoplanet atmospheres. The important extreme ultraviolet (EUV) region… Expand
The MUSCLES Treasury Survey. IV. : Scaling relations for ultraviolet, Ca II K, and energetic particle fluxes from M dwarfs
- A. Youngblood, K. France, +18 authors M. Vieytes
- Physics
- 11 May 2017
Characterizing the UV spectral energy distribution (SED) of an exoplanet host star is critically important for assessing its planet's potential habitability, particularly for M dwarfs as they are… Expand
Temperature condensation trend in the debris-disk binary system ζ2 Reticuli
- C. Saffe, M. Flores, M. Arancibia, A. Buccino, E. Jofr'e
- Physics
- 3 February 2016
Fil: Saffe, Carlos. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico Conicet - San Juan. Instituto de Ciencias Astronomicas, de la Tierra y del Espacio.… Expand
A possible long-term activity cycle for ι Horologii: First results from SPI-HKα project
- M. Flores, A. Buccino, C. Saffe, P. Mauas
- Physics
- 12 October 2016
Fil: Flores, Matias G.. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico Conicet - San Juan. Instituto de Ciencias Astronomicas, de la Tierra y del Espacio.… Expand
UV habitable zones around M stars
- A. Buccino, G. Lemarchand, P. Mauas
- Physics
- 11 January 2007
Abstract During the last decade there was a change in paradigm, which led to consider that terrestrial-type planets within liquid-water habitable zones (LW-HZ) around M stars can also be suitable… Expand