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20022009
most citedA grid of MARCS model atmospheres for late-type stars I. Methods and general properties

2.6k citations

Showing 2006Show all

17 papers · 1 filter

gr-qc200633 cited

Plebanski Theory and Covariant Canonical Formulation

Sergei Alexandrov, Eric Buffenoir, Philippe Roche

We establish an equivalence between the Hamiltonian formulation of the Plebanski action for general relativity and the covariant canonical formulation of the Hilbert-Palatini actio…

hep-ph2006196 cited

NMSPEC: A Fortran code for the sparticle and Higgs masses in the NMSSM with GUT scale boundary conditions

Ulrich Ellwanger, Cyril Hugonie

NMSPEC is a Fortran code that computes the sparticle and Higgs masses, as well as Higgs decay widths and couplings in the NMSSM, with soft SUSY breaking terms specified at MGUT. Ex…

hep-ph200613 cited

A FORTRAN code for in SM and MSSM

Th. Diakonidis, G. J. Gounaris, J. Layssac

Through the present paper, the code gamgamZZ is presented, which may be used to calculate all possible observables related to the process , in either the Standard Model (…

hep-ph200683 cited

The upper bound on the lightest Higgs mass in the NMSSM revisited

Ulrich Ellwanger, Cyril Hugonie

We update the upper bound on the lightest CP even Higgs mass in the NMSSM, which is given as a function of tan(beta) and lambda. We include the available one and two loop correctio…

gr-qc2006708 cited

Conditions for the cosmological viability of f(R) dark energy models

Luca Amendola, Radouane Gannouji, David Polarski +1

We derive the conditions under which dark energy models whose Lagrangian densities f are written in terms of the Ricci scalar R are cosmologically viable. We show that the cosmolog…

astro-ph200636 cited

Near-Infrared Spectroscopy of Carbon-Enhanced Metal-Poor Stars. I. A SOAR/OSIRIS Pilot Study

Timothy C. Beers, Thirupathi Sivarani, Brian Marstellar +3

We report on an abundance analysis for a pilot study of seven Carbon-Enhanced Metal-Poor (CEMP) stars, based on medium-resolution optical and near-infrared spectroscopy. The optica…