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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S319(11), p. 16-16, 2015

DOI: 10.1017/s1743921315009849

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Clustering of massive compact galaxies at 1 ≤ z ≤ 3 in CANDELS/3D-HST

Journal article published in 2015 by Lulu Fan ORCID, Xiaozhi Lin, Xu Kong, Guanwen Fang
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe present a measurement of the spatial clustering of massive compact galaxies at 1 ≤ z ≤ 3 in CANDELS/3D-HST. We obtain the correlation length and characteristic DM halo masses for compact quiescent galaxies (cQGs) at z ~ 1.5 and compact starforming galaxies (cSFGs) at z ~ 2.5. By comparison with extended starforming galaxies (eSFGs), our result indicates that eSFGs are less possible to be the progenitors of cQGs at lower redshift. Our results indicates that cQGs at z ~ 1.5 could be the progenitors of local luminous ETGs and the descendants of cSFGs and SMGs at z > 2.

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