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Medium-resolution Isaac Newton Telescope library of empirical spectra

dc.contributor.authorSánchez Blázquez, Patricia
dc.contributor.authorPeletier, R. F.
dc.contributor.authorJiménez Vicente, J.
dc.contributor.authorCardiel López, Nicolás
dc.contributor.authorCenarro, A. J.
dc.contributor.authorFalcón Barroso, J.
dc.contributor.authorGorgas García, Francisco Javier
dc.contributor.authorSelam, S.
dc.contributor.authorVazdekis, A.
dc.date.accessioned2023-06-20T10:50:56Z
dc.date.available2023-06-20T10:50:56Z
dc.date.issued2006-09-11
dc.descriptionThis article has been accepted for publication in Monthly notices of the Royal Astronomical Society. © 2006 The Authors. Journal compilation © 2006 RAS. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. We are indebted to the referee, Guy Worthey, for noting the presence of scattered light in the first version of the library. We would also like to thank Scott C. Trager for the careful reading of this manuscript and for his very useful comments and to Ricardo Schiavon for helping us find references to correct the spectra for atmospheric extinction. This paper is based on observations obtained at the Isaac Newton Telescope, operated by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. This work was supported by the Spanish research project AYA2003-01840. This work has made extensive use of the SIMBAD data base. We are grateful to the ASTRON-PC and CAT for generous allocation of telescope time. AV is a Ramón y Cajal Fellow of the Spanish Ministry of Education and Science. This work has been supported by the Spanish Ministry of Education and Science (grant AYA2004-03059).
dc.description.abstractA new stellar library developed for stellar population synthesis modelling is presented. The library consists of 985 stars spanning a large range in atmospheric parameters. The spectra were obtained at the 2.5-m Isaac Newton Telescope and cover the range λλ 3525–7500 Å at 2.3 Å (full width at half-maximum) spectral resolution. The spectral resolution, spectral-type coverage, flux-calibration accuracy and number of stars represent a substantial improvement over previous libraries used in population-synthesis models.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipSpanish Ministry of Education and Science
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/29321
dc.identifier.doi10.1111/j.1365-2966.2006.10699.x
dc.identifier.issn0035-8711
dc.identifier.officialurlhttp://dx.doi.org/10.1111/j.1365-2966.2006.10699.x
dc.identifier.relatedurlhttp://mnras.oxfordjournals.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/51332
dc.issue.number2
dc.journal.titleMonthly notices of the Royal Astronomical Society
dc.language.isoeng
dc.page.final718
dc.page.initial703
dc.publisherWiley
dc.relation.projectIDAYA2003-01840
dc.relation.projectIDAYA2004-03059
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordOld stellar populations
dc.subject.keywordEarly-type galaxies
dc.subject.keywordAbsorption-line spectra
dc.subject.keywordInfrared caii triplet
dc.subject.keywordMetal-rich stars
dc.subject.keywordGlobular-clusters
dc.subject.keywordK-stars
dc.subject.keywordSpectrophotometric atlas
dc.subject.keywordInterstellar extinction
dc.subject.keywordAbundance analysis
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.subject.ucmFísica atmosférica
dc.subject.unesco2501 Ciencias de la Atmósfera
dc.titleMedium-resolution Isaac Newton Telescope library of empirical spectra
dc.typejournal article
dc.volume.number371
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