Hostname: page-component-77c89778f8-m8s7h Total loading time: 0 Render date: 2024-07-17T10:31:02.154Z Has data issue: false hasContentIssue false
  • English
  • Français

Properties of high z galaxies in the ELTs era

Published online by Cambridge University Press:  17 August 2016

L. Greggio ,
M. Gullieuszik ,
R. Falomo ,
D. Fantinel  and
M. Uslenghi
L. Greggio
Affiliation:
INAF, Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy
M. Gullieuszik
Affiliation:
INAF, Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy
R. Falomo
Affiliation:
INAF, Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy
D. Fantinel
Affiliation:
INAF, Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy
M. Uslenghi
Affiliation:
INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica, Via Bassini 15, 20133 Milano, Italy
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The extraordinary sensitivity and spatial resolution of the future extremely large telescopes will allow us to extensively characterize the photometrical and structural properties of high redshift galaxies in spite of their very small size. With such future facilities it will be possible to derive both accurate photometry and detailed morphology of very distant galaxies that are mandatory to tackle fundamental problems on the processes of galaxy formation and evolution.

Keywords

instrumentation: adaptive opticsgalaxies: fundamental parametersgalaxies: high-redshift
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S319: Galaxies at High Redshift and Their Evolution Over Cosmic Time , August 2015 , pp. 21
Copyright
Copyright © International Astronomical Union 2016