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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 742356.0, MPI für Astronomie / Publikationen_mpia
The Pristine survey - III. Spectroscopic confirmation of an efficient search for extremely metal-poor stars
Authors:Youakim, K.; Starkenburg, E.; Aguado, D. S.; Martin, N. F.; Fouesneau, M.; González Hernández, J. I.; Allende Prieto, C.; Bonifacio, P.; Gentile, M.; Kielty, C.; Côté, P.; Jablonka, P.; McConnachie, A.; Sánchez Janssen, R.; Tolstoy, E.; Venn, K.
Date of Publication (YYYY-MM-DD):2017
Title of Journal:Monthly Notices of the Royal Astronomical Society
Volume:472
Issue / Number:3
Start Page:2963
End Page:2974
Audience:Not Specified
Abstract / Description:The Pristine survey is a narrow-band, photometric survey focused around the wavelength region of the Ca II H & K absorption lines, designed to efficiently search for extremely metal-poor stars. In this work, we use the first results of a medium-resolution spectroscopic follow-up to refine the selection criteria for finding extremely metal-poor stars ($\textrm{[Fe/H]} \leq -3.0$) in the Pristine survey. We consider methods by which stars can be selected from available broad-band and infrared photometry plus the additional Pristine narrow-band photometry. The spectroscopic sample presented in this paper consists of 205 stars in the magnitude range $14 < V < 18$. Applying the photometric selection criteria cuts the sample down to 149 stars, and from these we report a success rate of 70% for finding stars with $\textrm{[Fe/H]} \leq -2.5$ and 22% for finding stars with $\textrm{[Fe/H]} \leq -3.0$. These statistics compare favourably with other surveys that search for extremely metal-poor stars, namely an improvement by a factor of $\sim 4-5$ for recovering stars with $\textrm{[Fe/H]} \leq -3.0$. In addition, Pristine covers a fainter magnitude range than its predecessors, and can thus probe deeper into the Galactic halo.
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0035-8711 %R 10.1093/mnras/stx2005
URL:http://adsabs.harvard.edu/abs/2017MNRAS.472.2963Y
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