Models for Interstellar Extinction in the Galaxy

By E. Amôres, J. Lépine. 2005

160 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/8b9dc283ac010d8adf6551cbebfbf6bede12b257

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In Astronomy and Astrophysics

Citations in the corpus

Asteroseismology and Gaia: Testing Scaling Relations Using 2200 Kepler Stars with TGAS Parallaxes (2017, result): “We also show extinctions from Rodrigues et al. (2014), which were derived in a similar manner to the gridmodeling estimates presented here, and values from the model by Amôres & Lépine (2005), as applied by the BeSPP pipeline.”
One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c (2015, methodology): “We set the interstellar extinction to zero magnitude per kpc in the simulation, which we corrected a posteriori using the galactic extinction model of Amôres & Lépine (2005).”
LIFTING THE DUSTY VEIL WITH NEAR- AND MID-INFRARED PHOTOMETRY. I. DESCRIPTION AND APPLICATIONS OF THE RAYLEIGH–JEANS COLOR EXCESS METHOD (2011, methodology): “…studies using a wide variety of tracers have also derived significant V - band overestimates using the SFD maps: see Cambrésy et al. (2005), Choloniewski & Valentijn (2003), RochaPinto et al. (2004), Dutra et al. (2003a,b), Yasuda et al. (2007), and Amôres & Lépine (2005, 2007) for examples.”
LSST: From Science Drivers to Reference Design and Anticipated Data Products (2008, methodology): “For Galactic reddening, a value of E(B−V ) is assigned to each star using the three-dimensional Galactic model of Amores & Lepine (2005).”
Revised Stellar Properties of Kepler Targets for the Q1-17 (DR25) Transit Detection Run (2016, methodology): “For each model, we calculated a distance and extinction using observed apparent magnitudes, galactic coordinates of a given target, absolute magnitudes given by the model and the 3D extinction map by Amôres & Lépine (2005).”
Standing on the Shoulders of Dwarfs: the Kepler Asteroseismic LEGACY Sample. II. Radii, Masses, and Ages (2016, methodology): “2MASS photometry using the spectroscopic metallicity of each star and a reddening value given by the distance dependent map of Amôres & Lépine (2005).”
PASTIS: Bayesian extrasolar planet validation. I. General framework, models, and performance (2014, methodology): “In PASTIS, E(B − V) can be either fitted with the rest of the parameters or modelled using the threedimensional extinction model of Amôres & Lépine (2005).”
THE IMPACT OF STELLAR MULTIPLICITY ON PLANETARY SYSTEMS. I. THE RUINOUS INFLUENCE OF CLOSE BINARY COMPANIONS (2016, methodology): “Distance posteriors were calculated using absolute K-band magnitudes from the isochrone grid and the reddening map by Amôres & Lépine (2005), assuming the KOI is a single star with the given stellar parameters.”