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EVIDENCE FOR REDUCED SPECIFIC STAR FORMATION RATES IN THE CENTERS OF MASSIVE GALAXIES AT z = 4

dc.creatorJung, Intae
dc.creatorFinkelstein, Steven L.
dc.creatorSong, Mimi
dc.creatorDickinson, Mark
dc.creatorDekel, Avishai
dc.creatorFerguson, Henry C.
dc.creatorFontana, Adriano
dc.creatorKoekemoer, Anton M.
dc.creatorLu, Yu
dc.creatorMobasher, Bahram
dc.creatorPapovich, Casey
dc.creatorRyan, Russell E.
dc.creatorSalmon, Brett
dc.creatorStraughn, Amber N.
dc.date.accessioned2019-10-09T21:02:01Z
dc.date.available2019-10-09T21:02:01Z
dc.date.issued2017
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttps://hdl.handle.net/1969.1/182217
dc.format.extent1en
dc.publisherThe Astrophysical Journal
dc.relation.ispartof1foldr Import 2019-10-08 Batch 8en
dc.relation.uri10.3847/1538-4357/834/1/81en
dc.titleEVIDENCE FOR REDUCED SPECIFIC STAR FORMATION RATES IN THE CENTERS OF MASSIVE GALAXIES AT z = 4en


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