Revealing Substructure in the Galactic Halo: The SEKBO RR Lyrae Survey

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dc.contributor.authorKeller, Stefan
dc.contributor.authorMurphy, Simon
dc.contributor.authorPrior, Sayuri
dc.contributor.authorDa Costa, Gary
dc.contributor.authorSchmidt, Brian
dc.date.accessioned2015-12-07T22:50:45Z
dc.date.issued2008
dc.date.updated2015-12-07T12:21:08Z
dc.description.abstractWe present a search for RR Lyrae variable stars from archival observations of the Southern Edgeworth-Kuiper Belt Object survey. The survey covers 1675 deg2 along the ecliptic to a mean depth of V = 19.5, i.e., a heliocentric distance of ∼50 kpc for RR L
dc.description.sponsorshipThis paper utilizes public domain data obtained by the MACHO Project, jointly funded by the US Department of Energy through the University of California, Lawrence Livermore National Laboratory, under contract W-7405-Eng-48, by the National Science Foundation through the Center for Particle Astrophysics of the University of California under cooperative agreement AST 88-09616, and by the Mount Stromlo and Siding Spring Observatory, part of the Australian National University.
dc.format14 pages
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/27152
dc.provenancehttp://www.sherpa.ac.uk/romeo/issn/0004-637X/ Author can archive publisher's version/PDF. Publisher's version/PDF may be used on any website or authors' institutional repository (Sherpa/Romeo as of 10/10/2018)
dc.publisherIOP Publishing
dc.rights© 2008. The American Astronomical Society.
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Galaxy: halo; Galaxy: structure; Stars: variables: other
dc.titleRevealing Substructure in the Galactic Halo: The SEKBO RR Lyrae Survey
dc.typeJournal article
dcterms.accessRightsOpen Access
local.bibliographicCitation.issueMay
local.bibliographicCitation.lastpage864
local.bibliographicCitation.startpage851
local.contributor.affiliationKeller, Stefan, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationMurphy, Simon, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationPrior, Sayuri, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationDa Costa, Gary, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationSchmidt, Brian, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.authoruidKeller, Stefan, u9702857
local.contributor.authoruidMurphy, Simon, u4203307
local.contributor.authoruidPrior, Sayuri, u2519876
local.contributor.authoruidDa Costa, Gary, u9501331
local.contributor.authoruidSchmidt, Brian, u9500253
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4362859xPUB49
local.identifier.citationvolume678
local.identifier.doi10.1086/526516
local.identifier.essn1538-4357
local.identifier.scopusID2-s2.0-43949125822
local.identifier.thomsonID000255438800026
local.type.statusPublished Version

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