WebbLoading cross-sections ¶. We need to point TauREx3 to our cross-sections. This is handled by the caching classes. Once a cross-section is loaded it does not need to be loaded … Webbphoenix BT-Settl: Castelli & Kurucz (2003) + phoenix BT-Settl: New VLMS models with T– τ relation from phoenix BT-Settl: v1.2S: NBC: Calibrated phoenix BT-Settl: Castelli & …

SIMBAD references

WebbTop panel: a PHOENIX synthetic spectrum with parameters T eff = 3900 K, log g = 4.5, [Fe/H] = 0.0. Middle panel: the measured HARPS spectrum. The six bands used for rectification of the spectrum and subtraction of the photospheric flux (H, K, h1 , h2 , k1 , and k2 ) are marked as shaded areas. WebbThe PHOENIX stellar model (or PHOENIX or PHOENIX code ) is a computer model of the photosphere of a star. It was developed in the early 1990s with considerable improvement since. Through simulation, it gives a model spectrum of … note for loss of sister

Discovery of a warm, dusty giant planet around HIP 65426

WebbBT-Settl is a model that can simulate stellar atmospheres of small stars and brown dwarfs . It produces synthetic spectra. It uses the PHOENIX atmospheric code . ( … WebbBT-Settl Model Atmospheres and Spectra: The Role of Dust Allard et al 2003, IAUS 211, 325. K-H2 quasi-molecular absorption detected in the T-dwarf \varepsilon Indi Ba Allard … WebbContext:Age and mass determinations for isolated stellar objects remain model-dependent. While stellar interior and atmospheric theoretical models are rapidly evolving, we need a powerful tool to test them. Open cluste… note for loss of pet