Kim Venn astronome et chercheur ou chercheuse
Venn, Kimberley Ann, 1965-
Venn, Kimberley Ann
VIAF ID: 105903280 (Personal)
Permalink: http://viaf.org/viaf/105903280
Preferred Forms
4xx's: Alternate Name Forms (6)
Works
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The chemical abundances of galactic, A-type supergiants. |
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The chemical composition of three lambda Bootis stars |
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The chemical composition of two supergiants in the dwarf irregular galaxy WLM |
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Chemical Mapping of the Milky Way with The Canada–France Imaging Survey: A Non-parametric Metallicity–Distance Decomposition of the Galaxy |
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The chemistry of the most metal-rich damped Lyman {alpha} systems at z ~ 2 - II. Context with the Local Group |
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Chemo-dynamics of outer halo dwarf stars, including Gaia -Sausage and Gaia -Sequoia candidates |
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Could the ultra-metal-poor stars Be chemically peculiar and not related to the first stars? |
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The DART imaging and CaT survey of the Fornax dwarf spheroidal galaxy |
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Detailed chemical abundances of four stars in the unusual globular cluster Palomar 1 |
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The distance to an X-ray shadowing molecular cloud in Ursa Major |
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Evidence of ancient Milky Way merger |
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The extremely low-metallicity tail of the Sculptor dwarf spheroidal galaxy |
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Galactic abundance gradient in boron |
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Gemini high-resolution optical spectrograph conceptual design |
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GRACES observations of young [{alpha}/Fe]-rich stars |
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The impact of modeling assumptions in galactic chemical evolution models |
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Integrated light chemical tagging analyses of seven M31 outer halo globular clusters from the Pan-Andromeda Archaeological Survey |
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The interesting problem of the NLTE nitrogen abundance in Vega |
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IR excesses around nearby Lambda Boo stars are caused by debris discs rather than ISM bow waves |
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IRC +10420 : a cool hypergiant near the top of the H-R diagram |
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IRMOS: The near-infrared multi-object spectrograph for the TMT |
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LS 4825: a blue supergiant on the far side of the Galaxy |
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LTE and NLTE abundances in A-supergiants. A test of their evolutionary status |
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Major substructure in the M31 outer halo: distances and metallicities along the giant stellar stream |
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Mass-loss rates and stellar wind momenta of a-supergiants in M 31: first results from the Keck HIRES spectrograph |
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Massive stars spectroscopy in the Magellanic Clouds |
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Near-InfraRed Planet Searcher to Join HARPS on the ESO 3.6-metre Telescope |
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New identifications for blue objects towards the Galactic Center: post-AGB stars, Be/disk stars and others |
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Non-LTE line formation for neutral oxygen. Model atom and first results on A-type stars |
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Nucleosynthesis and the inhomogeneous chemical evolution of the Carina dwarf galaxy |
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On spectral line formation and measurement in cepheids: implications to distance determination |
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A peculiar faint satellite in the remote outer halo of M31 |
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The peculiar globular cluster Palomar 1 and persistence in the SDSS-APOGEE data base |
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Pristine dwarf galaxy survey – I. A detailed photometric and spectroscopic study of the very metal-poor Draco II satellite |
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The Pristine Inner Galaxy Survey (PIGS) II: Uncovering the most metal-poor populations in the inner Milky Way |
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The Pristine survey – IX. CFHT ESPaDOnS spectroscopic analysis of 115 bright metal-poor candidate stars |
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The Pristine survey – VI. The first three years of medium-resolution follow-up spectroscopy of Pristine EMP star candidates |
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The Pristine survey – VII. A cleaner view of the Galactic outer halo using blue horizontal branch stars |
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The Pristine Survey – VIII. The metallicity distribution function of the Milky Way halo down to the extremely metal-poor regime |
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The Pristine survey – X. A large population of low-metallicity stars permeates the Galactic disc |
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The Pristine survey – XI. the FORS2 sample |
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The Pristine survey – XII. Gemini-GRACES chemo-dynamical study of newly discovered extremely metal-poor stars in the Galaxy |
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The Pristine survey – XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations |
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The Pristine survey – XVII. The C-19 stream is dynamically hot and more extended than previously thought |
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i process and CEMP-s+r stars |
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The R-Process Alliance: First Release from the Northern Search for r-process-enhanced Metal-poor Stars in the Galactic Halo |
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Ram pressure stripping of an isolated Local Group dwarf galaxy: evidence for an intragroup medium |
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Raven: a harbinger of multi-object adaptive optics-based instruments at the Subaru Telescope |
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Rotational Velocities for B0-B3 Stars in Seven Young Clusters: Further Study of the Relationship between Rotation Speed and Density in Star-Forming Regions |
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The scatter about the ‘Universal’ dwarf spheroidal mass profile: a kinematic study of the M31 satellites And V and And VI |
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Science with GYES: a multifibre high-resolution spectrograph for the prime focus of the Canada-France-Hawaii Telescope |
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A search for boron in damped Ly{alpha} systems |
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Solo dwarfs I: survey introduction and first results for the Sagittarius dwarf irregular galaxy |
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The spatial homogeneity of nebular and stellar oxygen abundances in the Local Group dwarf irregular galaxy NGC 6822 |
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StarNet: a deep learning analysis of infrared stellar spectra |
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Stellar chemical signatures and hierarchical galaxy formation |
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Stellar Kinematics of the Isolated Dwarf Irregular WLM |
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Stellar wind momentum and extragalactic distances: a study of M 31 / M 33 supergiants using the Keck telescope |
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Testing rotational mixing predictions with new boron abundances in main-sequence B-type stars |
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Through thick and thin: kinematic and chemical components in the solar neighbourhood |
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Tracing the formation of the Milky Way through ultra metal-poor stars |
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A-type stars in the Canada–France Imaging Survey – II. Tracing the height of the disc at large distances with Blue Stragglers |
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A-type Stellar Abundances: A Corollary to Herschel Observations of Debris Disks |
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An upper limit on the sulphur abundance in HE 1327-2326 |
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VLT/FLAMES spectroscopy of red giant branch stars in the Carina dwarf spheroidal galaxy |
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The VLT-FLAMES survey of massive stars: Observations in the Galactic clusters NGC 3293, NGC 4755 and NGC 6611 |
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VLT/UVES abundances in four nearby dwarf spheroidal galaxies. II. Implications for understanding galaxy evolution |
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The wind momentum-luminosity relationship of galactic A- and B-supergiants |
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