0000000000179389

AUTHOR

Garrett Ebelke

showing 2 related works from this author

The Baryon Oscillation Spectroscopic Survey of SDSS-III

2012

The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the combined efforts of all previous spectroscopic surveys of large-scale structure. BOSS uses 1.5 million luminous galaxies as faint as i = 19.9 over 10,000 deg(2) to measure BAO to redshifts z < 0.7. Observations of neutral hydrogen in the Ly alpha forest in more than 150,000 quasar spectra (g < 22) will constrain BAO over the redshift range 2.15 < z < 3.5. Early results from BOSS include the first detection of the large-scale three-dimensional clustering of the Ly alpha forest and a strong detection from the Data R…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveysAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Settore FIS/05 - Astronomia e AstrofisicaObservacions astronòmiques0103 physical sciencesPhysical Sciences and Mathematicsobservations [Cosmology]010303 astronomy & astrophysicsObservationsAstrophysics::Galaxy AstrophysicsPhysicsCosmologia010308 nuclear & particles physicsAngular diameter distanceAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsQuasarCosmology and Extragalactic AstrophysicsLyman-alpha forestRedshiftGalaxyCosmologyBaryonBossSpace and Planetary ScienceAstronomiaBaryon acoustic oscillationsAstronomical observationsAstrophysics - Cosmology and Nongalactic Astrophysics
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Chemical Cartography with APOGEE: Multi-element Abundance Ratios

2019

We map the trends of elemental abundance ratios across the Galactic disk, spanning R = 3-15 kpc and midplane distance |Z|= 0-2 kpc, for 15 elements in a sample of 20,485 stars measured by the SDSS/APOGEE survey (O, Na, Mg, Al, Si, P, S, K, Ca, V, Cr, Mn, Fe, Co, Ni). Adopting Mg rather than Fe as our reference element, and separating stars into two populations based on [Fe/Mg], we find that the median trends of [X/Mg] vs. [Mg/H] in each population are nearly independent of location in the Galaxy. The full multi-element cartography can be summarized by combining these nearly universal median sequences with our measured metallicity distribution functions and the relative proportions of the lo…

stars: abundances010504 meteorology & atmospheric sciencesMilky WayMetallicityPopulationFOS: Physical sciences01 natural sciencesGalaxy: diskStellar nucleosynthesisNucleosynthesis0103 physical scienceseducation010303 astronomy & astrophysicsnuclear reactions0105 earth and related environmental sciencesPhysicseducation.field_of_studyabundancesnucleosynthesisAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxySupernova13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy: abundancesSupernova nucleosynthesis[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]CartographyThe Astrophysical Journal
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