UBV(RI)C JHK observations of Hipparcos-selected nearby stars

By C. Koen, D. Kilkenny, F. V. Wyk, F. Marang. 2010

162 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/674948a74e9f926f54bc2b46c3181be98f7efb36

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Citations in the corpus

VERY WIDE BINARIES AND OTHER COMOVING STELLAR COMPANIONS: A BAYESIAN ANALYSIS OF THE HIPPARCOS CATALOGUE (2010, methodology): “V data for early M dwarfs from Koen et al. (2010), and, to be consistent with the upper MS, we determine a lower-envelope to their HR diagram.7 For all cases, we use the dependence of a given color on Teff to interpolate over missing values.8 Then, for each star, their B–”
The M-dwarfs in Multiples (MinMs) survey – I. Stellar multiplicity among low-mass stars within 15 pc (2015, unknown): “– a Gray et al. (2006); b Browning et al. (2010); c Torres et al. (2006); d Poveda et al. (2009); e Koen et al. (2010); f Houk & Cowley (1975) c© 2015 RAS, MNRAS 000, 1–34”
BAYESIAN ANALYSIS TO IDENTIFY NEW STAR CANDIDATES IN NEARBY YOUNG STELLAR KINEMATIC GROUPS (2012, methodology): “The I -band photometric data come from the DENIS and SDSS-DR8 catalogs and several other studies (Torres et al. 2006; Reid & Cruz 2002; Koen et al. 2010; Casagrande et al. 2008; Reid et al. 2003, 2004, Riedel (in prep)).”
The effective temperature scale of M dwarfs (2013, methodology): “It comes from the NOMAD catalogue (Zacharias et al. 2005), the Deep Near-Infrared Survey (DENIS, Epchtein 1997), the Two Micron All Sky Survey (2MASS, Skrutskie et al. 2006), Reid et al. (2004, 2007), Koen & Eyer (2002); Koen et al. (2010).”
METALLICITY AND TEMPERATURE INDICATORS IN M DWARF K-BAND SPECTRA: TESTING NEW AND UPDATED CALIBRATIONS WITH OBSERVATIONS OF 133 SOLAR NEIGHBORHOOD M DWARFS (2011, unknown): “…spectra ∗Reference of distance and V magnitude: (1) HIPPARCOS (van Leeuwen 2007), (2) YALE (van Altena et al. 2001), (3) PMSU (Reid et al. 1997), (4) Koen et al. (2010), (5) Leggett (1992), (6) Bessel (1990), (7) Gould & Chanamé (2004), (8) Gliese & Jahreiss (1991) – 116 – – 117 – – 118 – Table…”
CHARACTERIZING THE COOL KOIs. III. KOI 961: A SMALL STAR WITH LARGE PROPER MOTION AND THREE SMALL PLANETS (2012, methodology): “Digital photometric measurements of Barnard’s Star include UV BRI photometry by Koen et al. (2010) and 2MASS JHK photometry.”
INTRINSIC COLORS, TEMPERATURES, AND BOLOMETRIC CORRECTIONS OF PRE-MAIN-SEQUENCE STARS (2013, unknown): “…(22) Luhman & Steeghs (2004); (23) Lyo et al. (2004); (24) Lawson et al. (2001); (25) Lawson et al. (2002); (26) Stephenson (1986); (27) Reid et al. (1995); (28) Koen et al. (2010); (29) Rodriguez et al. (2011); (30) Schneider et al. (2012b); (31) Scholz et al. (2005); (32) Teixeira et al.…”