The UVES Paranal Observatory Project: A Library of High- Resolution Spectra of Stars across the Hertzsprung-Russell Diagram

By S. Bagnulo, E. Jehin, C. Ledoux, R. Cabanac, C. Melo, R. Gilmozzi. 2003

246 citations recorded by the source corpus.

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Citations in the corpus

NLTE abundances of Mn in a sample of metal-poor stars ⋆ (2008, methodology): “The UVES observations of Procyon (HD 61421) and HD 84937 were taken from the UVESPOP survey (Bagnulo et al. 2003).”
Alpha element abundances and gradients in the Milky Way bulge from FLAMES-GIRAFFE spectra of 650 K giants (2011, methodology): “The Arcturus spectrum with a resolution of 120 000 comes from the UVES database (Bagnulo et al. 2003).”
Oxygen abundances in nearby stars - Clues to the formation and evolution of the Galactic disk (2007, methodology): “We also used 44 FGK stars spectra from the online UVES-VLT library by Bagnulo et al. (2003)5, who took advantage of the availability of the UVES spectrograph on the VLT during part of twilight time to observe a significant number 4 http://hebe.as.utexas.edu/s4n, http://www.astro.uu.se/∼s4n 5…”
Oxygen, Sodium, Magnesium and Aluminium as tracers of the Galactic Bulge Formation (2006, methodology): “TheVLT + UVES spectrum of Arcturus (R=120 000) was taken from the UVES Paranal Observatory Project database (Bagnulo et al. 2003).”
The metal content of bulge field stars from FLAMES-GIRAFFE spectra - I. Stellar parameters and iron abundances (2008, unknown): “In order to ensure a smooth transition between the so calledm talrich and themetalpoorline list, we measured the metallicity of Arcturus, from a UVES spectrum (Bagnulo et al. 2003) with both, and switch from one to the other at [Fe/H]=-0.4, where we check that the two would give consistent results.”
A non-LTE study of neutral and singly-ionized iron line spectra in 1D models of the Sun and selected late-type stars ? (2011, methodology): “For HD 84937 and HD 122563, we used high-quality observed spectra from the ESO UVESPOP survey (Bagnulo et al. 2003).”
The VLT-FLAMES Survey of Massive Stars: Observations in the Galactic Clusters NGC 3293, NGC 4755 and NGC 6611 ⋆ (2005, background): “Work is underway by other groups (e.g. Bagnulo et al. 2003) to compile high-resolution observations of spectral standards and our survey will significantly add to such efforts.”
EVIDENCE FOR A MASSIVE NEUTRON STAR FROM A RADIAL-VELOCITY STUDY OF THE COMPANION TO THE BLACK-WIDOW PULSAR PSR B1957+20 (2010, methodology): “Radial Velocities We determined velocities by fitting the flux-calibrated blue spectra of both the pulsar companion and the contaminator with a template based on the high-resolution spectrum of the G2 IV starβ Hyi (HD 2151) from the UVESPOP library (Bagnulo et al. 2003).”
Exploring the Milky Way stellar disk - A detailed elemental abundance study of 714 F and G dwarf stars in the solar neighbourhood (2013, methodology): “Finally we obtained reduced spectra for 31 stars from the UVES Paranal Observatory Project8, Bagnulo et al. 2003 (UVES POP).”
STECMAP: STEllar Content from high-resolution galactic spectra via Maximum A Posteriori (2005, unknown): “The library UVES POP (Bagnulo et al. 2003) is an example.”
Gaia FGK benchmark stars: Metallicity (2013, methodology): “…Data Products collection of the ESO Science Archive Facility2 (reduced by the standard UVES pipeline version 3.2, Ballester et al. 2000), and the UVES Paranal Observatory Project UVES-POP library (Bagnulo et al. 2003, processed with data reduction tools specifically developed for that library).”
Non‐LTE line formation of Fe in late‐type stars – I. Standard stars with 1D and 〈3D〉 model atmospheres (2012, methodology): “The UVES observations of Procyon (HD 61421), HD 84937, HD 140283, and HD 122563 were taken from the UVES-POP survey (Bagnulo et al. 2003).”
Chemical similarities between Galactic bulge and local thick disk red giants: O, Na, Mg, Al, Si, Ca, and Ti (2010, methodology): “Furthermore, the UVES library of stellar spectra (Bagnulo et al. 2003) was searched for suitable disk and halo giants.”
THE SEGUE STELLAR PARAMETER PIPELINE. I. DESCRIPTION AND COMPARISON OF INDIVIDUAL METHODS (2007, methodology): “…standards derived from spectral libraries of comparable resolution and coverage (Allen & Strom 1995; Prugniel & Soubiran 2001; Hawley et al. 2002; Bagnulo et al. 2003; Le Borgne et al. 2003; Valdes et al. 2The Hammer has been made available for community use: the IDL code can be downloaded…”
Automatic determination of stellar atmospheric parameters and construction of stellar spectral templates of the Guoshoujing Telescope (LAMOST) (2011, background): “Some popular empirical libraries are: ELODIE (Prugniel & Soubiran 2001; Prugniel & Soubiran 2004;Prugniel et al. 2007b); UVES-POP (Bagnulo et al. 2003); STELIB (Le Borgne et al. 2003); CFLIB (The INDO-US library of Coud́efeed Stellar Spectra) (Valdes et al. 2004); MILES (Sánchez-Bĺazquez et al.…”