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dc.contributor.authorYi, S.K.
dc.contributor.authorYoon, S.-J.
dc.contributor.authorLee, Y.-W.
dc.contributor.authorRee, C.H.
dc.contributor.authorSohn, Y.-J.
dc.contributor.authorRey, S.-C.
dc.contributor.authorRhee, J.
dc.contributor.authorByun, Y.-I.
dc.contributor.authorKim, S.-W.
dc.contributor.authorKaviraj, S.
dc.contributor.authorDeharveng, J.-M.
dc.contributor.authorBoselli, A.
dc.contributor.authorDonas, J.
dc.contributor.authorMalina, R.
dc.contributor.authorMilliard, B.
dc.contributor.authorRich, R.M.
dc.contributor.authorSalim, S.
dc.contributor.authorFriedman, P.G.
dc.contributor.authorMartin, D.C.
dc.contributor.authorMorrissey, P.
dc.contributor.authorSmall, T.
dc.contributor.authorBarlow, T.
dc.contributor.authorForster, K.
dc.contributor.authorWyder, T.K.
dc.contributor.authorLee, J.-W.
dc.contributor.authorBianchi, L.
dc.contributor.authorHeckman, T.M.
dc.contributor.authorSzalay, A.S.
dc.contributor.authorJee, M.J.
dc.contributor.authorJelinsky, P.
dc.contributor.authorSiegmund, O.
dc.contributor.authorWelsh, B.
dc.contributor.authorMadore, B.F.
dc.contributor.authorNeff, S.
dc.contributor.authorSchiminovich, D.
dc.identifier.citationYi , S K , Yoon , S-J , Lee , Y-W , Ree , C H , Sohn , Y-J , Rey , S-C , Rhee , J , Byun , Y-I , Kim , S-W , Kaviraj , S , Deharveng , J-M , Boselli , A , Donas , J , Malina , R , Milliard , B , Rich , R M , Salim , S , Friedman , P G , Martin , D C , Morrissey , P , Small , T , Barlow , T , Forster , K , Wyder , T K , Lee , J-W , Bianchi , L , Heckman , T M , Szalay , A S , Jee , M J , Jelinsky , P , Siegmund , O , Welsh , B , Madore , B F , Neff , S & Schiminovich , D 2005 , ' Galaxy evolution explorer ultraviolet color-magnitude relations and evidence of recent star formation in early-type galaxies ' , Astrophysical Journal Letters , vol. 619 , no. 1 , L111 .
dc.identifier.otherPURE: 2065504
dc.identifier.otherPURE UUID: cd99aacf-7530-4758-bc14-775e1b328f14
dc.identifier.otherScopus: 20044373056
dc.identifier.otherORCID: /0000-0002-5601-575X/work/77850139
dc.description.abstractWe have used the Galaxy Evolution Explorer UV photometric data to construct a first near-UV (NUV) color-magnitude relation (CMR) for the galaxies preclassified as early-type by Sloan Digital Sky Survey studies. The NUV CMR is a powerful tool for tracking the recent star formation history in early-type galaxies, owing to its high sensitivity to the presence of young stellar populations. Our NUV CMR for UV-weak galaxies shows a well-defined slope and thus will be useful for interpreting the rest-frame NUV data of distant galaxies and studying their star formation history. Compared to optical CMRs, the NUV CMR shows a substantially larger scatter, which we interpret as evidence of recent star formation activities. Roughly 15% of the recent epoch (z <0.13) bright [M(r) <-22] early-type galaxies show a sign of recent ≤1 Gyr) star formation at the 1%-2% level (lower limit) in mass compared to the total stellar mass. This implies that low-level residual star formation was common during the last few billion years even in bright early-type galaxies.en
dc.relation.ispartofAstrophysical Journal Letters
dc.titleGalaxy evolution explorer ultraviolet color-magnitude relations and evidence of recent star formation in early-type galaxiesen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre of Data Innovation Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review

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