Publication
Detailed analysis of Balmer lines in cool dwarf stars
An analysis of Hα and Hβ spectra in a sample of 30 cool dwarf and subgiant stars is presented using MARCS model atmospheres based on the most recent...
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PublicationDetailed Chemical Abundances for a Benchmark Sample of M Dwarfs from the APOGEE SurveyIndividual chemical abundances for 14 elements (C, O, Na, Mg, Al, Si, K, Ca, Ti, V, Cr, Mn, Fe, and Ni) are derived for a sample of M dwarfs using high...
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PublicationDetailed chemical composition of the globular cluster Sextans A GC-1 on the outskirts of the Local GroupContext. The chemical composition of globular clusters (GCs) across the Local Group provides information on chemical abundance trends. Studying GCs in isolated...
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PublicationDetailed chemical evolution models of the Tucana dSph galaxyWe use semi-analytical methods to obtain detailed chemical evolution models (CEMs) for the dwarf spheroidal (dSph) galaxy Tucana. Published star formation rates...
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PublicationDetailed cool star flare morphology with CHEOPS and TESS (Corrigendum)
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PublicationDetailed cool star flare morphology with CHEOPS and TESS***Context. White-light stellar flares are proxies for some of the most energetic types of flares, but their triggering mechanism is still poorly understood. As...
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PublicationDetailed Diagnostics of an X-Ray Flare in the Single Giant HR 9024We analyze a 96 ks Chandra HETGS observation of the single G-type giant HR 9024. The high flux allows us to examine spectral line and continuum diagnostics at...
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PublicationDetailed Photometric Study of the Merging Group of Galaxies HCG 95Results from Hα + continuum and Johnson UBVI imaging for HCG 95 are presented in order to study the star formation history of the galaxies in the group. Based...
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PublicationDetailed spectrophotometric analysis of the superluminous and fast evolving SN 2019neqSN 2019neq was a very fast evolving superluminous supernova. At a redshift z = 0.1059, its peak absolute magnitude was -21.5 ± 0.2 mag in g band. In this work...