activity
20022026
most citedNew H-band Stellar Spectral Libraries for the SDSS-III/APOGEE survey

147 citations · 589 across the 10 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2026

The open cluster NGC 2509. Stellar rotation and main sequence turnoff extension from FLAMES spectroscopy

C. Boeche, J. Alonso-Santiago, A. Bragaglia +8

NGC 2509 is a distant (~2.5 kpc) and little-studied open cluster located in the third Galactic quadrant. It is a moderately old cluster, whose age has not yet been precisely determ…

astro-ph.GA2017★ 10 cited

The open cluster King~1 in the second quadrant

R. Carrera, L. Rodríguez Espinosa, L. Casamiquela +4

We analyse the poorly-studied open cluster King~1 in the second Galactic quadrant. From wide-field photometry we have studied the spatial distribution of this cluster. We determine…

astro-ph.SR2015★ 147 cited

New H-band Stellar Spectral Libraries for the SDSS-III/APOGEE survey

O. Zamora, D. A. Garcia-Hernandez, C. Allende Prieto +18

The Sloan Digital Sky Survey--III (SDSS--III) Apache Point Observatory Galactic Evolution Experiment (APOGEE) has obtained high resolution (R 22,500), high signal-to-noise r…

astro-ph.GA2012★ 15 cited

Analysis of the CN and CH molecular band strengths in stars of the open cluster NGC 6791

R. Carrera

Low resolution SDSS/SEGUE spectra have been used to study the behavior of the strengths of the CN and CH molecular bands in stars at different evolutionary stages of the open clust…

astro-ph.GA2010★ 81 cited

Low-resolution spectroscopy of main sequence stars belonging to 12 Galactic globular clusters. I. CH and CN band strength variations

E. Pancino, M. Rejkuba, M. Zoccali +1

Globular clusters show abundance variations for light elements that are not yet well understood. The preferred explanation involves a self-enrichment scenario, with two subsequent…

astro-ph.GA2009★ 32 cited

Radial extent of the SGB in NGC 1851

M. Zoccali, E. Pancino, M. Catelan +3

Recent HST-ACS observations revealed the presence of a double subgiant branch (SGB) in the core of the Galactic globular cluster NGC 1851. This peculiarity was tentatively explaine…