SPT 0538-50: PHYSICAL CONDITIONS IN THE INTERSTELLAR MEDIUM OF A STRONGLY LENSED DUSTY STAR-FORMING GALAXY AT <i>z</i>=2.8

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dc.contributor.authorBothwell, M. S.
dc.contributor.authorAguirre, J. E.
dc.contributor.authorChapman, S. C.
dc.contributor.authorMarrone, D. P.
dc.contributor.authorVieira, J. D.
dc.contributor.authorAshby, M. L. N.
dc.contributor.authorAravena, M.
dc.contributor.authorBenson, B. A.
dc.contributor.authorBock, J. J.
dc.contributor.authorBradford, C. M.
dc.contributor.authorBrodwin, M.
dc.contributor.authorCarlstrom, J. E.
dc.contributor.authorCrawford, T. M.
dc.contributor.authorDe Breuck, C.
dc.contributor.authorDownes, T. P.
dc.contributor.authorFassnacht, C. D.
dc.contributor.authorGonzalez, A. H.
dc.contributor.authorGreve, T. R.
dc.contributor.authorGullberg, B.
dc.contributor.authorHezaveh, Y.
dc.contributor.authorHolder, G. P.
dc.contributor.authorHolzapfel, W. L.
dc.contributor.authorIbar, E.
dc.contributor.authorIvison, R.
dc.contributor.authorKamenetzky, J.
dc.contributor.authorKeisler, R.
dc.contributor.authorLupu, R. E.
dc.contributor.authorMa, J.
dc.contributor.authorMalkan, M.
dc.contributor.authorMcIntyre, V.
dc.contributor.authorMurphy, E. J.
dc.contributor.authorNguyen, H. T.
dc.contributor.authorReichardt, C. L.
dc.contributor.authorRosenman, M.
dc.contributor.authorSpilker, J. S.
dc.contributor.authorStalder, B.
dc.contributor.authorStark, A. A.
dc.contributor.authorStrandet, M.
dc.contributor.authorVernet, J.
dc.contributor.authorWeiss, A.
dc.contributor.authorWelikala, N.
dc.date.accessioned2025-01-24T00:07:34Z
dc.date.available2025-01-24T00:07:34Z
dc.date.issued2013
dc.description.abstractWe present observations of SPT-S J053816-5030.8, a gravitationally lensed dusty star-forming galaxy (DSFG) at z = 2.7817 that was first discovered at millimeter wavelengths by the South Pole Telescope. SPT 0538-50 is typical of the brightest sources found by wide-field millimeter-wavelength surveys, being lensed by an intervening galaxy at moderate redshift (in this instance, at z = 0.441). We present a wide array of multi-wavelength spectroscopic and photometric data on SPT 0538-50, including data from ALMA, Herschel PACS and SPIRE, Hubble, Spitzer, the Very Large Telescope, ATCA, APEX, and the Submillimeter Array. We use high-resolution imaging from the Hubble Space Telescope to de-blend SPT 0538-50, separating DSFG emission from that of the foreground lens. Combined with a source model derived from ALMA imaging (which suggests a magnification factor of 21+/-4), we derive the intrinsic properties of SPT 0538-50, including the stellar mass, far-IR luminosity, star formation rate, molecular gas mass, and-using molecular line fluxes-the excitation conditions within the interstellar medium. The derived physical properties argue that we arewitnessing compact, merger-driven star formation in SPT 0538-50 similar to local starburst galaxies and unlike that seen in some other DSFGs at this epoch.
dc.fuente.origenWOS
dc.identifier.doi10.1088/0004-637X/779/1/67
dc.identifier.eissn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttps://doi.org/10.1088/0004-637X/779/1/67
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/101923
dc.identifier.wosidWOS:000328160100067
dc.issue.numero1
dc.language.isoen
dc.revistaAstrophysical journal
dc.rightsacceso restringido
dc.subjectgalaxies: evolution
dc.subjectgalaxies: formation
dc.subjectgalaxies: high-redshift
dc.subjectgalaxies: individual
dc.subjectgravitational lensing: strong
dc.subjectsubmillimeter: galaxies
dc.titleSPT 0538-50: PHYSICAL CONDITIONS IN THE INTERSTELLAR MEDIUM OF A STRONGLY LENSED DUSTY STAR-FORMING GALAXY AT <i>z</i>=2.8
dc.typeartículo
dc.volumen779
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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