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LAMOST Observations in the Kepler Field: Spectral Classification with the MKCLASS Code

dc.contributor.authorGray R. O.
dc.contributor.authorCorbally C. J.
dc.contributor.authorDe Cat P.
dc.contributor.authorFu J. N.
dc.contributor.authorRen A. B.
dc.contributor.authorShi J. R.
dc.contributor.authorLuo A. L.
dc.contributor.authorZhang H. T.
dc.contributor.authorWu Y.
dc.contributor.authorCao Z.
dc.contributor.authorLi G.
dc.contributor.authorZhang Y.
dc.contributor.authorHou Y.
dc.contributor.authorWang Y.
dc.date1/2016
dc.date.accessioned2016-04-13T10:08:53Z
dc.date.available2016-04-13T10:08:53Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3979
dc.descriptionhttp://esoads.eso.org/abs/2016AJ....151...13G
dc.languageeng
dc.rightsRestricted Access
dc.titleLAMOST Observations in the Kepler Field: Spectral Classification with the MKCLASS Code
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleThe Astronomical Journal
dc.source.volume151
dc.source.page13
Orfeo.peerreviewedYes
dc.identifier.doi10.3847/0004-6256/151/1/13
dc.identifier.urlhttp://esoads.eso.org/abs/2016AJ....151...13G
dc.source.editorIOP


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