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V. Silva Aguirre

9 papers here

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

author position
  • first author2
  • middle author5
  • last author1

Across the 8 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR5
  • astro-ph.GA3
  • astro-ph.EP1
ORCID 0000-0002-6137-903X
same name
  • V. Silva Aguirre — 13 papers, h 15

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
20092021
most citedThe Thirteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey MApping Nearby Galaxies at Apache Point Observatory

509 citations · 996 across the 9 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2017★ 165 cited

Confirming chemical clocks: asteroseismic age dissection of the Milky Way disk(s)

V. Silva Aguirre, M. Bojsen-Hansen, D. Slumstrup +22

Investigations of the origin and evolution of the Milky Way disk have long relied on chemical and kinematic identification of its components to reconstruct our Galactic past. Diffi…

astro-ph.GA2016★ 509 cited

The Thirteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey MApping Nearby Galaxies at Apache Point Observatory

SDSS Collaboration, Franco D. Albareti, Carlos Allende Prieto +335

The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) began observations in July 2014. It pursues three core programs: APOGEE-2, MaNGA, and eBOSS. In addition, eBOSS cont…

astro-ph.GA2015★ 153 cited

Measuring the vertical age structure of the Galactic disc using asteroseismology and SAGA

L. Casagrande, V. Silva Aguirre, K. J. Schlesinger +10

The existence of a vertical age gradient in the Milky Way disc has been indirectly known for long. Here, we measure it directly for the first time with seismic ages, using red gian…

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