Search Results - "Cunha, Katia"
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A Spectroscopic Analysis of the California-Kepler Survey Sample. I. Stellar Parameters, Planetary Radii, and a Slope in the Radius Gap
Published in The Astrophysical journal (10-04-2019)“…We present results from a quantitative spectroscopic analysis conducted on archival Keck/HIRES high-resolution spectra from the California-Kepler Survey (CKS)…”
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Mapping the Galactic Metallicity Gradient with Open Clusters: The State-of-the-Art and Future Challenges
Published in Universe (Basel) (01-02-2022)“…In this paper, we make use of data collected for open cluster members by high-resolution spectroscopic surveys and programmes (i.e., APOGEE, Gaia-ESO, GALAH,…”
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A Metallicity Study of F, G, K, and M Dwarfs in the Coma Berenices Open Cluster from the APOGEE Survey
Published in The Astrophysical journal (01-08-2021)“…Abstract We present a study of metallicities in a sample of main-sequence stars with spectral types M , K , G , and F ( T eff ∼3200–6500K and log g ∼ 4.3–5.0…”
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The Lazy Giants: APOGEE Abundances Reveal Low Star Formation Efficiencies in the Magellanic Clouds
Published in The Astrophysical journal (01-06-2020)“…We report the first APOGEE metallicities and -element abundances measured for 3600 red giant stars spanning a large radial range of both the Large (LMC) and…”
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A Comprehensive Study of Open Cluster Chemical Homogeneity Using APOGEE and Milky Way Mapper Abundances
Published in The Astrophysical journal (01-11-2024)“…Abstract Stars in an open cluster are assumed to have formed from a broadly homogeneous distribution of gas, implying that they should be chemically…”
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Abundances of Planetary Nebulae and Evolved Stars: Iron and Sulfur Depletion, and Carbon and Nitrogen Enrichment, in Low- and Intermediate-mass Stellar Populations in the Milky Way
Published in The Astrophysical journal (01-09-2024)“…Abstract We research the elemental abundances in Galactic planetary nebulae (PNe) compared with those of their stellar progenitors (red giant branch and…”
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Boron Abundances in Early B Dwarfs of the Galactic Open Cluster NGC 3293
Published in The Astrophysical journal (01-06-2024)“…Abstract New boron abundances or upper limits have been determined for eight early B stars in the young Galactic open cluster NGC 3293, using UV spectra…”
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LITHIUM-RICH GIANTS IN GLOBULAR CLUSTERS
Published in The Astrophysical journal (10-03-2016)“…ABSTRACT Although red giants deplete lithium on their surfaces, some giants are Li-rich. Intermediate-mass asymptotic giant branch (AGB) stars can generate Li…”
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Magnetic Fields in a Sample of Planet-hosting M Dwarf Stars from Kepler, K2, and TESS Observed by APOGEE
Published in The Astrophysical journal (01-11-2024)“…Abstract Stellar magnetic fields have a major impact on space weather around exoplanets orbiting low-mass stars. From an analysis of Zeeman-broadened Fe i…”
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10
Stellar Characterization and a Chromospheric Activity Analysis of a K2 Sample of Planet-hosting Stars
Published in The Astrophysical journal (01-07-2024)“…Abstract Effective temperatures, surface gravities, and iron abundances were derived for 109 stars observed by the K2 mission using equivalent width…”
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IDENTIFICATION OF NEODYMIUM IN THE APOGEE H-BAND SPECTRA
Published in The Astrophysical journal (10-12-2016)“…ABSTRACT We present the detection of 10 lines of singly ionized neodymium (Nd ii, Z = 60) in H-band spectra using observations from the SDSS-III Apache Point…”
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A Tale of Two Disks: Mapping the Milky Way with the Final Data Release of APOGEE
Published in The Astrophysical journal (01-09-2023)“…Abstract We present new maps of the Milky Way disk showing the distribution of metallicity ([Fe/H]), α -element abundances ([Mg/Fe]), and stellar age, using a…”
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Fluorine in the Solar Neighborhood: The Need for Several Cosmic Sources
Published in The Astrophysical journal (01-04-2020)“…The cosmic origin of fluorine is still not well constrained. Several nucleosynthetic channels at different phases of stellar evolution have been suggested, but…”
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Using Photometrically Derived Properties of Young Stars to Refine TESS’s Transiting Young Planet Survey Completeness
Published in The Astronomical journal (01-10-2023)“…Abstract The demographics of young exoplanets can shed light on their formation and evolution processes. Exoplanet properties are derived from the properties…”
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Stellar Characterization of M Dwarfs from the APOGEE Survey: A Calibrator Sample for M-dwarf Metallicities
Published in The Astrophysical journal (20-02-2020)“…We present spectroscopic determinations of the effective temperatures, surface gravities, and metallicities for 21 M dwarfs observed at high resolution (R ∼…”
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Stellar Characterization and Chemical Abundances of Exoplanet-hosting M Dwarfs from APOGEE Spectra: Future JWST Targets
Published in The Astrophysical journal (01-10-2024)“…Abstract Exoplanets hosting M dwarfs are the best targets to characterize Earth-like or super-Earth planetary atmospheres with the James Webb Space Telescope…”
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High-resolution Elemental Abundance Measurements of Cool JWST Planet Hosts Using AutoSpecFit: An Application to the Sub-Neptune K2-18b’s Host M Dwarf
Published in The Astrophysical journal (01-09-2024)“…Abstract We present an in-depth, high-resolution spectroscopic analysis of the M dwarf K2-18, which hosts a sub-Neptune exoplanet in its habitable zone. We…”
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Magnetic Fields in M-dwarf Members of the Pleiades Open Cluster Using APOGEE Spectra
Published in The Astrophysical journal (01-08-2024)“…Abstract Average magnetic field measurements are presented for 62 M-dwarf members of the Pleiades open cluster, derived from Zeeman-enhanced Fe i lines in the…”
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Galactic Metallicity Gradients Derived from a Sample of OB Stars
Published in The Astrophysical journal (20-12-2004)“…The distribution of stellar abundances along the Galactic disk is an important constraint for models of chemical evolution and Galaxy formation. In this study…”
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The Bulge Metallicity Distribution from the APOGEE Survey
Published in The Astrophysical journal (10-01-2018)“…The Apache Point Observatory Galactic Evolution Experiment (APOGEE) provides spectroscopic information of regions of the inner Milky Way, which are…”
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