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ATLAS and SYNTHE under Linux
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We have successfully ported under GNU Linux ATLAS 9, the widely used stellar atmosphere modeling code, as well as both the SYNTHE suite of programs, its ``companion'' for spectral synthesis, and WIDTH, used to derive chemical abundances from equivalent widths of spectral lines. The porting has been realized by using the Intel Fortran Compiler. Our aim was to port the codes with the minimum possible amount of modifications: full compatibility with the VMS version has been maintained, along with all the codes functionalities. Dramatic improvement in calculation speed with respect to the VMS version has been achieved. The full suite of codes is intended to be freely available to anyone.
Forward citations
Cited by 8 Pith papers
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BEBOP VII. SOPHIE discovery of BEBOP-3b, a circumbinary giant planet on an eccentric orbit
BEBOP-3b is a 0.56-Jupiter-mass circumbinary giant planet on a 547-day, moderately eccentric orbit, the first radial-velocity discovery of a previously unknown circumbinary system.
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NGTS-EB-7, an eccentric, long-period, low-mass eclipsing binary
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The Hubble Missing Globular Clusters Survey IV. Ultra-faint compact satellites of the Milky Way. The case of Koposov 2
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HD 28471: a near-resonant compact multiplanet system with a possible cold giant planet
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gr8stars I: A homogeneous spectroscopic study of bright FGKM dwarfs and a public library of their high-resolution spectra
The gr8stars catalogue provides homogeneous spectroscopic and photometric stellar parameters for 1716 bright FGKM dwarfs, along with a public library of high-resolution spectra.
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oMEGACat V: Helium Enrichment in $\omega$ Centauri as a Function of Metallicity
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Introducing STARDIS: An Open and Modular Stellar Spectral Synthesis Code
STARDIS is an open-source, modular 1D LTE stellar spectral synthesis code for FGK stars that agrees with korg at the few percent level redward of about 4000 Å and diverges in the ultraviolet.
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gr8stars II : judgement day for spectroscopic parameter model systematics
Multi-method spectroscopic analysis of 585 FGK dwarfs shows parameter scatters larger than internal errors, inducing sub-5% fractional uncertainties on derived exoplanet radius and mass.
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