Intrinsic Colors of Stars in the Near-Infrared
By J. Ducati, C. M. Bevilacqua, S. Rembold, Daiana Ribeiro. 2001
177 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/f27037ab6bf6bf379603b01c843ce25f1ab07951
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Citations in the corpus
- Ten eclipsing binaries in the Small Magellanic Cloud: fundamental parameters and SMC distance (2002, background): “This compares favourably with values of −0.28 and −0.33 reported by Wegner (1994) and by Ducati et al. (2001), after conversion from (V − I)J to (V − I)C using the transformation given by Cousins (1980).”
- PROSPECTING IN LATE-TYPE DWARFS: A CALIBRATION OF INFRARED AND VISIBLE SPECTROSCOPIC METALLICITIES OF LATE K AND M DWARFS SPANNING 1.5 dex (2012, background): “The resulting sample contains 262 pairs with primaries with colors in the range 0.8 < Vp−Jp < 2.5 and/or published temperatures consistent with a late-F, G, or early-K dwarf (Fitzgerald 1970; Ducati et al. 2001).”
- The White Dwarf Initial–Final Mass Relation for Progenitor Stars from 0.85 to 7.5 M⊙ (2018, methodology): “Here we take the photometric color and distance of Sirius A from the HIPPARCOS analysis of van Leeuwen (2007; confirmed by the recent Gaia DR2) and the apparent magnitude from Ducati et al. (2001).”
- Multiplicity of Galactic Cepheids from long-baseline interferometry – III. Sub-percent limits on the relative brightness of a close companion of δ Cephei (2016, methodology): “From our estimated reported limits, we can exclude the presence of a companion having a spectral type earlier than a F0V star within 25 mas, A1V star between 25–50 mas, and B9V star between 50–100 mas from δ Cep (estimated using intrinsic colors from Cox (2000) and Ducati et al. (2001)).”