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<ri:Resource created="1997-12-09T21:27:16Z" 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>Far UV Stellar Photometry</title><shortName>J/ApJS/96/605</shortName><identifier>ivo://CDS.VizieR/J/ApJS/96/605</identifier><altIdentifier>doi:10.26093/cds/vizier.20960605</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Schmidt E.G.</name></creator><creator><name>Carruthers G.R.</name></creator><date role="Updated">2013-02-27T06:18:54Z</date><date role="Created">1997-12-09T21:27:16Z</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>ultraviolet-photometry</subject><subject>early-type-stars</subject><description>Far-ultraviolet photometry for 741 objects in a field in Sagittarius centered near M8 and 541 objects in a field centered near zeta Scorpii is presented. These data were extracted from electrographic images obtained with two cameras during a shuttle flight in 1991 April/May. The cameras provided band passes with lambda_eff = 1375 A and lambda_eff = 1781 A. Synthetic colors show that these bands are sensitive to effective temperature for hot stars. Our measurements were placed on a quantitative far-ultraviolet magnitude scale by convolving the spectra of stars observed by IUE with our cameras' spectral response functions. Fifty-eight percent of the ultraviolet objects were identified with visible stars using the SIMBAD database while another 40% of the objects are blends of early type stars too close together to separate with our resolution. Our photometry is compared with that from the TD-1, OAO 2, and ANS satellites and the S201 (Apollo 16) far-ultraviolet camera and found to agree at the level of a few tenths of a magnitude. Unlike previous studies, almost half of the identified visual counterparts to the ultraviolet objects are early B stars. 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42344 42345 42346 42356 42359 42361 42362 42368 42369 42370 42373 42374 42375 42376 42379 42381 42382 42383 42384 42385 42387 42393 42394 42395 42396 42408 42410 42416 42417 42418 42424 42426 42428 42430 42434 42441 42442 42443 42444 42449 42450 42453 42455 42458 42460 42461 42463 42468 42470 42471 42473 42475 42476 42477 42479 42481 42482 42483 42486 42488 42489 42491 42492 42560 42564 42568 42569 42573 42574 42575 42577 42578 42579 42587 42591 42593 42599 42609 42610 42611 42612 42622 42623 42752 42757 42760 42763 42764 42768 42770 42771 42777 42778 42779 42782 42791 42800 42801 42804 42808 42819 42820 42821 42823 42824 42825 42826 42828 42829 42830 42832 42834 42848 42850 47854 47855 47866 47867 47870 48042</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/96/605?format=ascii</footprint><waveband>UV</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/96/605/table4</name><description>*Ultraviolet objects in 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V or ptg. magnitude from SIMBAD</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_Mag</name><description>[P] 'P' when Mag is photographic</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table><table><name>J/ApJS/96/605/table5</name><description>*Ultraviolet objects in the zeta Sco field</description><column><name>n_Mag</name><description>[P] 'P' when Mag is photographic</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Sp</name><description>Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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