Asteroseismology from dome a, antarctica

Simple item page
dc.contributor.authorFu, J. N.en
dc.contributor.authorZong, W. K.en
dc.contributor.authorYang, Y.en
dc.contributor.authorMoore, A.en
dc.contributor.authorAshley, M. C.B.en
dc.contributor.authorCui, X. Q.en
dc.contributor.authorFeng, L. L.en
dc.contributor.authorGong, X. F.en
dc.contributor.authorLawrence, J. S.en
dc.contributor.authorLuong-Van, D.en
dc.contributor.authorLiu, Q.en
dc.contributor.authorPennypacker, C. R.en
dc.contributor.authorShang, Z. H.en
dc.contributor.authorStorey, J. W.V.en
dc.contributor.authorWang, L. Z.en
dc.contributor.authorWang, L. F.en
dc.contributor.authorYang, H. G.en
dc.contributor.authorYuan, X. Y.en
dc.contributor.authorYork, D. G.en
dc.contributor.authorZhou, X.en
dc.contributor.authorZhu, Z. H.en
dc.date.accessioned2025-12-31T21:42:13Z
dc.date.available2025-12-31T21:42:13Z
dc.date.issued2014en
dc.description.abstractGattini and CSTAR have been installed at Dome A, Antarctica, which provide time-series photometric data for a large number of pulsating variable stars. We present the study for several variable stars with the data collected with the two facilities in 2009 to demonstrate the scientific potential of observations from Dome A for asteroseismology.en
dc.description.statusPeer-revieweden
dc.format.extent2en
dc.identifier.isbn9781107045170en
dc.identifier.issn1743-9213en
dc.identifier.otherORCID:/0000-0002-2894-6936/work/161348809en
dc.identifier.scopus84894572115en
dc.identifier.urihttps://hdl.handle.net/1885/733798345
dc.language.isoenen
dc.relation.ispartofPrecision Asteroseismologyen
dc.relation.ispartofseriesProceedings of the International Astronomical Unionen
dc.relation.isversionofS301en
dc.titleAsteroseismology from dome a, antarcticaen
dc.typeConference paperen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage410en
local.bibliographicCitation.startpage409en
local.contributor.affiliationFu, J. N.; Beijing Normal Universityen
local.contributor.affiliationZong, W. K.; Beijing Normal Universityen
local.contributor.affiliationYang, Y.; Beijing Normal Universityen
local.contributor.affiliationMoore, A.; California Institute of Technologyen
local.contributor.affiliationAshley, M. C.B.; University of New South Walesen
local.contributor.affiliationCui, X. Q.; CAS - National Astronomical Observatoriesen
local.contributor.affiliationFeng, L. L.; CAS - Purple Mountain Observatoryen
local.contributor.affiliationGong, X. F.; CAS - National Astronomical Observatoriesen
local.contributor.affiliationLawrence, J. S.; University of New South Walesen
local.contributor.affiliationLuong-Van, D.; University of New South Walesen
local.contributor.affiliationLiu, Q.; Chinese Academy of Sciencesen
local.contributor.affiliationPennypacker, C. R.; Lawrence Berkeley National Laboratoryen
local.contributor.affiliationShang, Z. H.; Tianjin Normal Universityen
local.contributor.affiliationStorey, J. W.V.; University of New South Walesen
local.contributor.affiliationWang, L. Z.; Chinese Academy of Sciencesen
local.contributor.affiliationWang, L. F.; Texas A&M Universityen
local.contributor.affiliationYang, H. G.; Polar Research Institute of Chinaen
local.contributor.affiliationYuan, X. Y.; CAS - Purple Mountain Observatoryen
local.contributor.affiliationYork, D. G.; The University of Chicagoen
local.contributor.affiliationZhou, X.; Chinese Academy of Sciencesen
local.contributor.affiliationZhu, Z. H.; Beijing Normal Universityen
local.identifier.ariespublicationa383154xPUB6713en
local.identifier.doi10.1017/S1743921313014798en
local.identifier.essn1743-9221en
local.identifier.pure91eec4f5-889a-49e7-93e8-8e0b03097b89en
local.identifier.urlhttps://www.scopus.com/pages/publications/84894572115en
local.type.statusPublisheden

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