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Presentation . 2017
License: CC BY
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Presentation . 2017
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Other literature type . 2017
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The KMOS Cluster Survey – KCS: Timing the formation of passive galaxies in clusters with 1.4

descriptionPublicationkeyboard_double_arrow_right Presentation , Other literature type 03 Aug 2017Publisher:Zenodo
Authors: Beifiori, Alessandra;

doi: 10.5281/zenodo.2595107 , 10.5281/zenodo.2595106 , 10.5281/zenodo.838557 , 10.5281/zenodo.838558

The KMOS Cluster Survey – KCS: Timing the formation of passive galaxies in clusters with 1.4

Abstract

In this talk I will discuss recent progress studying the rest-frame optical properties of quiescent galaxies at 1.4 < z < 1.8 using KMOS. I will highlight recent results form the KMOS Custer Survey (KCS), whose aim is to provide a census of quiescent galaxy kinematics at 1.4 < z < 1.8 in know overdensities. The combination of kinematic measurements from KMOS and structural parameters measured from deep HST imaging allowed us to place constraints on the formation ages of passive galaxies at 1.4 < z <1.8 and on the evolution of galaxy properties and scaling relations at high redshift.

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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