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<ri:Resource created="1998-10-26T05:20:34Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>General Catalog of S Stars, second edition</title><shortName>III/168</shortName><identifier>ivo://CDS.VizieR/III/168</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Stephenson</name></creator><creator><name>C.B.</name></creator><date role="Updated">2013-02-26T11:57:39Z</date><date role="Created">1998-10-26T05:20:34Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>late-type-stars</subject><subject>s-stars</subject><description>This catalog is intended to list all Galactic S stars having known positions of at least roughly the precision of the Henry Draper catalog. An S star is a star in whose spectrum the bands of the ZrO molecule are detectable, ordinarily without needing sufficient spectral resolution to resolve the individual rotational lines of a band. In addition, stars exhibiting readily detectable LaO in the photographic infrared, where there is no significant ZrO, are known to form a subset of S stars (more extreme in abundances or low temperature), and this catalog includes stars classified only from the infrared. The majority of the stars were, however, discovered on the basis of the (0,0) band, with head near 6474Angstroem, of the red system of ZrO. Nomenclature Note: There are three catalogues of S stars by Stephenson, each being numbered from 1. Care should therefore be taken to make a clear distinction between a) The first Edition (1976, Publ. Warner &amp; Swasey Obs. 2, No. 2; Catalog &lt;III/60&gt;); these objects are designated "GCSS" b) This second edition published in 1984; these objects are designated "CSS" c) A complement to the Second Edition published in 1990 (=1990AJ....100..569S), designated by "CSS2" Ahthor's Introduction: The first edition of this catalog, published more than eight years ago, contained little more than half of the present number of stars, but nearly half of those were previously unpublished although lists of Henize's discoveries had been widely circulated. The principal additions since then come from three sources: (1) A low-dispersion infrared survey of the southern Milky Way by Westerlund, the S stars from which are hitherto unpublished; (2) a relatively high-dispersion red survey by MacConnell, also of the southern Milky Way, published in two lists here catalog-coded as MacCon79 and MacCon82; and (3) an unpublished and just-completed intermediate-dispersion red survey by Stephenson, covering the sky north of declination -25d and outside of galactic latitudes +/-10d. This last survey was intended to create for such red surveys a degree of completeness for the entire sky that was wholly lacking in the first edition. As remarked in the first edition, a logical reason for undertaking this catalog is the author's access to the Observatory's extensive collection of blue, red, and infrared objective prism plates, which covers the entire northern sky (though not in all wavelength regions) plus the southern Milky Way. As before, this collection was used not only for new discoveries, but also to resolve many cases of confusion in the literature. Previous objective prism surveys that were capable of identifying S stars have been summarized by Stephenson in the first edition of this catalog (Stephenson 1976), and also by Yorka and Wing (1979). The best combination of limiting magnitude (mostly 11.5 to 12, visual) and completeness has been achieved in the red spectral region, using the ZrO band with head at 6474 A. The entire northern sky north of declination -25d, plus the southern Milky Way, has been surveyed by Stephenson or N. Sanduleak (who did about 40% of the southern Milky Way), at 1,000 A/mm at H alpha (about 700 A/mm at the D lines). The rest of the southern sky has been done to 10th mag. by K. Henize, using 300 A/mm at the D lines. When the first edition of the S-star catalog was published, there had been no satisfactory red survey (that is, one that was capable of finding S stars consistently) of the sky north of declination -25d and outside of galactic latitudes +/-10d. The author has since remedied this lack, using the Burrell Schmidt telescope. The survey was begun at the old site in Ohio, using improved telescope optics (new corrector plus refigured mirror), but all but some 140 of the nearly 1300 required fields were taken at the Schmidt's new location on Kitt Peak. Also, additional surveys have turned up numbers of S stars in the southern Milky Way. B. Westerlund has used the infrared region at 2100 A/mm to search between galactic latitudes +/-5d and longitudes 235d to 7d, to a limiting infrared magnitude of 12.5. The comparable northern infrared surveys stop about 3 mags. brighter than this, but the author hopes to remedy this situation within a few years. Westerlund's new S stars are published for the first time in the present catalog. MacConnell's new S stars were found with 420 A/mm at H alpha; his plates have the highest spectral resolution of any of the red surveys, and so include the weakest S stars.</description><source>Publ. 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