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dc.contributor.authorMarsan, Z.
dc.contributor.authorMarchesini, D.
dc.contributor.authorBrammer, G.
dc.contributor.authorStefanon, M.
dc.contributor.authorMuzzin, A.
dc.contributor.authorFernández-Soto, A.
dc.contributor.authorGeier, S.
dc.contributor.authorHainline, K.
dc.contributor.authorIntema, Hubertus
dc.contributor.authorKarim, A.
dc.contributor.authorLabbé, I.
dc.contributor.authorToft, S.
dc.contributor.authorDokkum, P.
dc.date.accessioned2019-02-19T04:15:04Z
dc.date.available2019-02-19T04:15:04Z
dc.date.created2019-02-19T03:58:21Z
dc.date.issued2015
dc.identifier.citationMarsan, Z. and Marchesini, D. and Brammer, G. and Stefanon, M. and Muzzin, A. and Fernández-Soto, A. and Geier, S. et al. 2015. Spectroscopic confirmation of an ultramassive and compact galaxy at Z = 3.35: A detailed look at an early progenitor of local giant ellipticals. Astrophysical Journal. 801 (2).
dc.identifier.urihttp://hdl.handle.net/20.500.11937/73888
dc.identifier.doi10.1088/0004-637X/801/2/133
dc.description.abstract

© 2015. The American Astronomical Society. All rights reserved. We present the first spectroscopic confirmation of an ultramassive galaxy at redshift z > 3 using data from Keck- NIRSPEC, VLT-X-shooter, and GTC-Osiris. We detect strong [O III] and Lya emission, and weak [O II], C IV, and He II, placing C1-23152 at a spectroscopic redshift of zspec = 3.351. The modeling of the emission-line-corrected spectral energy distribution (SED) results in a best-fit stellar mass of M* = 3.1-0.7+0.6 × 1011 M?, a star formation rate of <7 M?yr-1, and negligible dust extinction. The stars appear to have formed in a short intense burst ~300-500 Myr prior to the observation epoch, setting the formation redshift of this galaxy at z ~ 4.1. From the analysis of the line ratios and widths and the observed flux at 24 µm, we confirm the presence of a luminous hidden active galactic nucleus (AGN), with bolometric luminosity of ~1046 erg s-1. Potential contamination of the observed SED from the AGN continuum is constrained, placing a lower limit on the stellar mass of 2 × 1011 M?. HST/WFC3 H160 and ACS I814 images are modeled, resulting in an effective radius of re ~ 1 kpc in the H160 band and a -Sti-errsic index n ~ 4.4. This object may be a prototype of the progenitors of local most massive elliptical galaxies in the first 2 Gyr of cosmic history, having formed most of its stars at z > 4 in a highly dissipative, intense, and short burst of star formation. C1-23152 is completing its transition to a post-starburst phase while hosting a powerful AGN, potentially responsible for the quenching of the star formation activity.

dc.publisherInstitute of Physics Publishing
dc.titleSpectroscopic confirmation of an ultramassive and compact galaxy at Z = 3.35: A detailed look at an early progenitor of local giant ellipticals
dc.typeJournal Article
dcterms.source.volume801
dcterms.source.number2
dcterms.source.issn0004-637X
dcterms.source.titleAstrophysical Journal
curtin.accessStatusFulltext not available


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