The Vienna-KPNO search for Doppler-imaging candidate stars - I. A catalog of stellar-activity indicators for 1058 late-type Hipparcos stars

By K. Strassmeier, A. Washuettl, T. Granzer, M. Scheck, M. Weber. 2000

169 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Computational Mechanics

View Paper: https://www.semanticscholar.org/paper/e65cedc17530873c5b1797593cd475e4204b3751

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Citations in the corpus

THE PALOMAR/KECK ADAPTIVE OPTICS SURVEY OF YOUNG SOLAR ANALOGS: EVIDENCE FOR A UNIVERSAL COMPANION MASS FUNCTION (2008, methodology): “Where data from high-dispersion optical spectra were previously available (Strassmeier et al. 2000; White et al. 2007), these were also reviewed for the strength of the lithium 6708 Å absorption line to put additional constraints on the ages.”
Stellar Kinematic Groups. II. A Reexamination of the Membership, Activity, and Age of the Ursa Major Group (2003, background): “…(4) RV and (RV) from SM93; (5) Barbier-Brossat & Figon 2000 catalog; (6) radial velocity from Tokovinin & Smekhov 2002; (7) radial velocity from Strassmeier et al. 2000; (8) radial velocity from Grenier et al. 1999; (9) radial velocity from Delfosse et al. 1999 and is systemic velocity of…”
A PHOTOMETRIC VARIABILITY SURVEY OF FIELD K AND M DWARF STARS WITH HATNet (2009, methodology): “Studies of this sort have been carried out in abundance for open clusters (e.g., Radick et al. 1987) as well as for some field stars (e.g., Strassmeier et al. 2000; Kiraga & St ↪ epień 2007).”
Five New Multicomponent Planetary Systems (2005, result): “Optical photometry by Strassmeier et al. (2000) revealed a period of 11.5 days with an amplitude of 0.035 mag.”
Nearby Debris Disk Systems with High Fractional Luminosity Reconsidered (2006, methodology): “In the case of HD 121812 our age estimate is based on the former method, taking the measured value from Strassmeier et al. (2000) and using the calibration of Lachaume et al. (1999).”
CHROMOSPHERIC ACTIVITY AND JITTER MEASUREMENTS FOR 2630 STARS ON THE CALIFORNIA PLANET SEARCH (2010, background): “Henry et al. (1996) derived SHK values for more than 800 nearby stars from the southern hemisphere; Strassmeier et al. (2000) monitored SHK as a tracer for rotation period to find candidates for Doppler imaging; Hall et al. (2007) have measured H and K fluxes since 1994 to search for stars with…”
A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun (2010, background): “For that reason we check our star sample for pre-main sequence stars and find 236 of them either in catalogues (Chauvin et al. 2010; Ducourant et al. 2005; Hernández et al. 2005; Wichmann et al. 2005; Valenti et al. 2003; Köhler et al. 2000; Neuhäuser et al. 2000; Teixeira et al. 2000; Bertout et”
Chromospheric Ca II Emission in Nearby F, G, K, and M Stars (2004, background): “Other surveys include the ViennaKPNO survey (Strassmeier et al. 2000), whose motivation was to find Doppler-imaging candidates by using Ca II H & K as a tracer of rotation period in 1058 late-type stars, and that of our Anglo-Australian Planet Search (Tinney et al. 2002), which reported S values…”
The Orbit and Pulsation Periods of the γ Doradus Variable HR 6844 (V2502 Ophiuchi) (2003, background): “Danziger & Faber (1972) found v sin i 10 km s 1, while more recent values are 13 (Abt & Morrell 1995), 8.0 (Fekel 1997), and 8.1 km s 1 (Strassmeier et al. 2000).”
Fast-rotating nearby solar-type stars - I. Spectral classification, v sin i, Li abundances and X-ray luminosities (2002, background): “References: 1) Favata et al. (1998); 2) Torres et al. (2000); 3) Barrado y Navascues & Stauffer (1996); 4) Randich et al. (1999); 5) Strassmeier et al. (2000); 6) Soderblom et al. (1998); 7) Pallavicini et al. (1987).”