activity
19982015
most citedNew H-band Stellar Spectral Libraries for the SDSS-III/APOGEE survey

147 citations · 167 across the 2 of their papers we have counts for

collaborators

10 papers

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.GA2011★ 20 cited

Sulphur abundances in halo giants from the [S I] line at 1082 nm and the S I triplet around 1045 nm

H. Jönsson, N. Ryde, P. E. Nissen +4

It is still debated whether or not the Galactic chemical evolution of sulphur in the halo followed the constant or flat trend with [Fe/H], ascribed to the result of explosive nucle…

astro-ph.SR2010

High-resolution HST/ACS images of detached shells around carbon stars

H. Olofsson, M. Maercker, K. Eriksson +2

Aims: The detached shells carry information on their formation process, as well as on the small-scale structure of the circumstellar medium around AGB stars due to the absence of s…

astro-ph.SR2009

The detached dust and gas shells around the carbon star U Ant

M. Maercker, H. Olofsson, K. Eriksson +2

Context: Geometrically thin, detached shells of gas have been found around a handful of carbon stars. --Aims: Previous observations of scattered stellar light in the circumstellar…

astro-ph2005

Oxygen abundances in metal-poor subgiants as determined from [O I], O I and OH lines

A. E. García Pérez, M. Asplund, F. Primas +2

The debate on the oxygen abundances of metal-poor stars has its origin in contradictory results obtained using different abundance indicators. To achieve a better understanding of…

astro-ph2002

ISO-SWS calibration and the accurate modelling of cool-star atmospheres - II. General results

L. Decin, B. Vandenbussche, C. Waelkens +5

The fine calibration of the ISO-SWS detectors (Infrared Space Observatory - Short Wavelength Spectrometer) has proven to be a delicate problem. We therefore present a detailed spec…