Properties of high z galaxies in the ELTs era

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.

Coverage

Galaxies at High Redshift and Their Evolution Over Cosmic Time

All editors

Kaviraj, S.

Series

PROCEEDINGS OF THE INTERNATIONAL ASTRONOMICAL UNION

Volume

vol. 11, S319

Start page

21

Conferenece

Galaxies at High Redshift and Their Evolution Over Cosmic Time

Conferenece place

Honolulu, Hawaii, USA

Conferenece date

3-7 August, 2015

Uri

http://hdl.handle.net/20.500.12386/26373

Url

https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/properties-of-high-z-galaxies-in-the-elts-era/083A0B99EAC54A8CE3428A31313DBF1D

Issn Identifier

1743-9213

Ads BibCode

2016IAUS..319...21G

Rights

open.access

File(s)

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Description

Pdf editoriale

Size

118.73 KB

Format

Adobe PDF

Checksum (MD5)

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Name

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Description

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Size

171.76 KB

Format

Adobe PDF

Checksum (MD5)

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Properties of high z galaxies in the ELTs era

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