J/ApJS/123/283ivo://CDS.VizieR/J/ApJS/123/283doi:10.26093/cds/vizier.21230283CDSMontes D.Ramsey L.W.Welty A.D.2000-06-09T12:03:08Z2000-06-09T12:02:10ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frspectroscopylate-type-starsWe present a library of Penn State Fiber Optic Echelle (FOE) observations of a sample of field stars with spectral types F to M and luminosity classes V to I. The spectral coverage is from 3800 to 10000{AA} with a nominal resolving power of 12,000. These spectra include many of the spectral lines most widely used as optical and near-infrared indicators of chromospheric activity such as the Balmer lines (H{alpha} to H{delta}), Ca II H & K, the Mg I b triplet, Na I D_1_, D_2_, He I D_3_, and Ca II IRT lines. There are also a large number of photospheric lines, which can also be affected by chromospheric activity, and temperature-sensitive photospheric features such as TiO bands. The spectra have been compiled with the goal of providing a set of standards observed at medium resolution. We have extensively used such data for the study of active chromosphere stars by applying a spectral subtraction technique. However, the data set presented here can also be utilized in a wide variety of ways ranging from radial velocity templates to study of variable stars and stellar population synthesis. This library can also be used for spectral classification purposes and determination of atmospheric parameters (T_eff_, logg, [Fe/H]). A digital version of all the fully reduced spectra is available via ftp and the World Wide Web (WWW) in FITS format.1999ApJS..123..283Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/123/283CatalogResearchIsServedByTAP VizieR generic servicerelated-toDigital version with all the fully reduced spectra:http://www.ucm.es/info/Astrof/fgkmsl/FOEfgkmsl.html : Digital versionJ/A+AS/123/473 : Late-type star spectra (Montes+ 1997)J/A+AS/128/485 : Library of UES spectra late-type stars (Montes+ 1998)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/123/283https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/123/283http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/123/283https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/123/283https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/123/283http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/123/283GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/ApJS/123/283/table3StarsType[FGKM] Type of starcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.intHD? HD (Cat. <III/135>) numberintnullablem_HDMultiplicity index on HDcharHR? HR (Cat. <V/50>) numberintnullablem_HRMultiplicity index on HRcharGJ? Gliese (Cat. <V/70>) numberfloatnullablem_GJMultiplicity index on GJcharNameOther namecharSimbadask the SIMBAD data-base about this objectcharSpTypeSpectral type and luminosity class (1)charMK[MK* ] Note about the spectral class (2)char[Fe/H]? Metallicitylog(Sun)floatnullableProt? Rotational perioddfloatnullablel_vsini[<= ] Limit flag on vsinicharvsini? Rotational velocitykm/sfloatnullableS? Ca II H & K spectrophotometric index (3)floatnullableRunObserving runs (4)charRefStar present in other papers: I: star in Paper I, Cat. <J/A+AS/123/473> II: star in Paper II, Cat. <J/A+AS/128/485>char