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researcher

V. Smith

120 papers hereh-index 00 citations0 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author7
  • middle author79
  • last author17

Across the 103 of 120 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR53
  • astro-ph.GA47
  • astro-ph11
  • astro-ph.EP7
  • astro-ph.IM2
same name
  • V. Smith — 37 papers, h 14
  • V. Smith — 33 papers, h 64
  • V. Smith — 8 papers, h 13
  • V. Smith — 8 papers, h 90
  • V. Smith — 8 papers, h 3
  • V. Smith — 5 papers, h 37

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20002023
most citedThe Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment

1k citations · 12k across the 120 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.SR2016★ 10 cited

Lithium Inventory of 2 M⊙​ Red Clump Stars in Open Clusters: A Test of the Helium Flash Mechanism

Joleen K. Carlberg, Katia Cunha, Verne V. Smith

The temperature distribution of field Li-rich red giants suggests the presence of a population of Li-rich red clump (RC) stars. One proposed explanation for this population is that…

astro-ph.SR2016★ 32 cited

Chemical Abundances in a Sample of Red Giants in the Open Cluster NGC 2420 from APOGEE

Diogo Souto, Katia Cunha, Verne Smith +20

NGC 2420 is a ∼2 Gyr-old well-populated open cluster that lies about 2 kpc beyond the solar circle, in the general direction of the Galactic anti-center. Most previous abundan…

astro-ph.GA2016★ 45 cited

Chemical abundance gradients from open clusters in the Milky Way disk: results from the APOGEE survey

Katia Cunha, Peter M. Frinchaboy, Diogo Souto +23

Metallicity gradients provide strong constraints for understanding the chemical evolution of the Galaxy. We report on radial abundance gradients of Fe, Ni, Ca, Si, and Mg obtained…

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