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Cited by 1,130 publications
(1,041 citation statements)
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“…The white dwarf spectrum is calculated using TLUSTY and SYNSPEC (Hubeny & Lanz 1995) and input parameters of T wd = 13,280 K and log g = 8.06 (Farihi et al 2012a). To fit the SED of the dust disk, we use the opaque disk model described in Jura (2003) with three free parameters, the inner disk radius R in , outer disk radius R out , and disk inclination i.…”
Section: Sed Fitsmentioning
confidence: 99%
“…The white dwarf spectrum is calculated using TLUSTY and SYNSPEC (Hubeny & Lanz 1995) and input parameters of T wd = 13,280 K and log g = 8.06 (Farihi et al 2012a). To fit the SED of the dust disk, we use the opaque disk model described in Jura (2003) with three free parameters, the inner disk radius R in , outer disk radius R out , and disk inclination i.…”
Section: Sed Fitsmentioning
confidence: 99%
“…For the spectral fits, we used a grid of white dwarf models generated with the latest version of TLUSTY204N and SYNSPEC49T (Hubeny & Lanz 1995). The grid covers T eff = 9000-69 900 K in steps of 100 K, log g = 8.35 dex, and a metallicity of 0.1 times the solar metallicity, which reproduces well the metal absorption lines.…”
Section: 2010 and 2011 Observationsmentioning
confidence: 99%
“…The synthetic model spectra of the WD stellar atmosphere are generated using the FORTRAN suite of codes TLUSTY, SYNSPEC, and ROTIN (Hubeny 1988;Hubeny & Lanz 1995). The basic input parameters are the stellar effective surface temperature, surface gravity, and chemical composition.…”
Section: Synthetic Spectral Modeling and Analysismentioning
confidence: 99%