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Sergi Blanco-Cuaresma

Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA

68 papers hereh-index 3819.6k citations174 works total

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

author position
  • sole author3
  • first author9
  • middle author32
  • last author9

Across the 53 of 68 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR29
  • astro-ph.GA15
  • astro-ph.EP9
  • astro-ph.IM9
  • cs.CL3
  • cs.HC1
affiliations
  • Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
  • Faculty of Psychology, UniDistance Suisse, Schinerstrasse 18, Brig, 3900, Switzerland
Homepage
same name
  • Sergi Blanco-Cuaresma — 3 papers, 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
20152026
most citedModern stellar spectroscopy caveats

325 citations · 1.1k across the 37 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2017

NGC 6705 a young α-enhanced Open Cluster from OCCASO data

L. Casamiquela, R. Carrera, L. Balaguer-Núñez +12

The stellar [α/Fe] abundance is sometimes used as a proxy for stellar age, following standard chemical evolution models for the Galaxy, as seen by different observational results…

astro-ph.GA2017★ 84 cited

Atypical Mg-poor Milky Way field stars with globular cluster second-generation like chemical patterns

J. G. Fernández-Trincado, O. Zamora, D. A. Garcia-Hernandez +48

We report the peculiar chemical abundance patterns of eleven atypical Milky Way (MW) field red giant stars observed by the Apache Point Observatory Galactic Evolution Experiment (A…

astro-ph.GA2017★ 46 cited

OCCASO II. Physical parameters and Fe abundances of Red Clump stars in 18 Open Clusters

L. Casamiquela, R. Carrera, S. Blanco-Cuaresma +13

Open Clusters have long been used to study the chemo-dynamical evolution of the Galactic disk. This requires an homogeneously analysed sample covering a wide range of ages and dist…

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