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researcher

K. Cunha

179 papers hereh-index 6217.5k citations324 works total

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

author position
  • sole author1
  • first author11
  • middle author127
  • last author8

Across the 147 of 179 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA72
  • astro-ph.SR61
  • astro-ph31
  • astro-ph.IM8
  • astro-ph.EP7
same name
  • K. Cunha — 13 papers, h 4
  • K. Cunha — 7 papers, h 2
  • K. Cunha — 2 papers, h 6
  • K. Cunha — 1 paper, h 0
  • K. Cunha — 1 paper, h 2

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
20002026
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations · 18.7k across the 179 of their papers we have counts for

collaborators
Showing 2009Show all

3 papers · 1 filter

astro-ph.GA2009★ 61 cited

A Two Micron All-Sky Survey View of the Sagittarius Dwarf Galaxy: VI. s-Process and Titanium Abundance Variations Along the Sagittarius Stream

Mei-Yin Chou, Katia Cunha, Steven R. Majewski +4

We present high-resolution spectroscopic measurements of the abundances of titanium (Ti), yttrium (Y) and lanthanum (La) for M giant candidates of the Sagittarius (Sgr) dwarf spher…

astro-ph.SR2009★ 31 cited

Sulfur Abundances in the Orion Association B Stars

Simone Daflon, Katia Cunha, Ramiro de la Reza +2

Sulfur abundances are derived for a sample of ten B main-sequence star members of the Orion association. The analysis is based on LTE plane-parallel model atmospheres and non-LTE l…

astro-ph.SR2009★ 2 cited

Detailed analyses of three neutron-capture-rich carbon-enhanced metal-poor stars

N. T. Behara, P. Bonifacio, H. -G. Ludwig +3

Approximately 20% of very metal-poor stars ([Fe/H] < -2.0) are strongly enhanced in carbon ([C/Fe] > +1.0). Such stars are referred to as carbon-enhanced metal-poor (CEMP) stars. W…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.