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THE MID-INFRARED LUMINOSITY FUNCTION AT z < 0.3 FROM 5MUSES: UNDERSTANDING THE STAR FORMATION/ACTIVE GALACTIC NUCLEUS BALANCE FROM A SPECTROSCOPIC VIEW

dc.creatorWu, Yanling
dc.creatorShi, Yong
dc.creatorHelou, George
dc.creatorArmus, Lee
dc.creatorDale, Daniel A.
dc.creatorPapovich, Casey
dc.creatorRahman, Nurur
dc.creatorDasyra, Kalliopi
dc.creatorStierwalt, Sabrina
dc.date.accessioned2019-10-08T21:09:06Z
dc.date.available2019-10-08T21:09:06Z
dc.date.issued2011
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttps://hdl.handle.net/1969.1/179690
dc.format.extent1en
dc.publisherThe Astrophysical Journal
dc.relation.ispartof1foldr Import 2019-10-08 Batch 3en
dc.relation.uri10.1088/0004-637X/734/1/40en
dc.titleTHE MID-INFRARED LUMINOSITY FUNCTION AT z < 0.3 FROM 5MUSES: UNDERSTANDING THE STAR FORMATION/ACTIVE GALACTIC NUCLEUS BALANCE FROM A SPECTROSCOPIC VIEWen


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