On Determining Extinction from Reddening

By M. McCall. 2004

154 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Global and Planetary Change

View Paper: https://www.semanticscholar.org/paper/c9e6a9d3a2f0c7527b4ee8fdd184f4c799821d4a

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Citations in the corpus

THE AGES OF 55 GLOBULAR CLUSTERS AS DETERMINED USING AN IMPROVED METHOD ALONG WITH COLOR–MAGNITUDE DIAGRAM CONSTRAINTS, AND THEIR IMPLICATIONS FOR BROADER ISSUES (2013, unknown): “Accordingly, we adopted (m−M)V = 13.35, which, for E(B−V ) = 0.032, is equivalent to (m−M)F606W = 13.34, since AF606W ≈ 2.80E(B−V ) (Sirianni et al. 2005) as compared with AV ≈ 3.07E(B − V ) (McCall 2004).”
A new implementation of the infrared flux method using the 2MASS catalogue (2009, methodology): “Consistently, the magnitudes for Vega were taken from McCall (2004), which gives the model magnitudes of Bessell et al. (1998) for the optical bands.”
DIRECT OXYGEN ABUNDANCES FOR LOW-LUMINOSITY LVL GALAXIES (2012, methodology): “The MMT spectra were de-reddened using the reddening law of Cardelli et al. (1989), parameterized by AV = 3.1 E(B − V ), where the extinction, A1(λ) was calculated using the York Extinction Solver (McCall 2004) 5.”
Synthetic stellar photometry – I. General considerations and new transformations for broad-band systems (2014, methodology): “While the implications of these facts are discussed in the literature (e.g., Fitzpatrick 1999; McCall 2004; Maı́z Apellániz 2013), their importance is often overlooked.”
CHEMICAL ABUNDANCES FOR 855 GIANTS IN THE GLOBULAR CLUSTER OMEGA CENTAURI (NGC 5139) (2010, unknown): “V)=2.70 (McCall 2004).”
The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool as We Thought (2005, unknown): “The resulting temperature fits for the early and mid-K stars are therefore less certain, probably 100 K. 6 The value RV is typically taken to be 3.6 for RSGs (Lee 1970), due to the increase of the effective wavelength of broadband filters with redder stars; see McCall (2004) for a recent discussion.”
An absolutely calibrated T eff scale from the infrared flux method. Dwarfs and subgiants (2010, methodology): “They based their work on the Castelli & Kurucz (1994) model and McCall (2004) magnitudes instead of the HST (Bohlin & Gilliland 2004; Bohlin 2007) and 2MASS (Cohen et al. 2003) values that we use.”