Modeling multi-wavelength properties of high redshift galaxies

Pierluigi Monaco; Fabio Fontanot; Barbara Lo Faro; Gabriella De Lucia; Eros Vanzella; Rachel Somerville; Stefano Cristiani; Laura Silva; Paola Santini

doi:10.1063/1.3141597

Modeling multi-wavelength properties of high redshift galaxies

Pierluigi Monaco, Fabio Fontanot, Barbara Lo Faro, Gabriella De Lucia, Eros Vanzella, Rachel Somerville, Stefano Cristiani, Laura Silva, Paola Santini

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

1 Scopus citations

Abstract

By comparing galaxy formation models within the ACDM cosmology with available data on high redshift galaxies, we show that small galaxies , with stellar masses < 10¹¹ M, are formed too early, are too passive since z ̃ 3 and too old at z = 0. This is due to an overproduction of small galaxies at high redshift, visible also as an excess of Z_AB ̃ 27 V-dropouts. We discuss the consequences of this excess.

Original language	English (US)
Title of host publication	Probing Stellar Populations Out To The Distant Universe - Cefalu 2008 - Proceedings of the International Conference
Pages	48-51
Number of pages	4
DOIs	https://doi.org/10.1063/1.3141597
State	Published - 2009
Externally published	Yes
Event	International Conference on Probing Stellar Populations Out To The Distant Universe, Cefalu 2008 - Cefalu, Sicily, Italy Duration: Sep 7 2008 → Sep 19 2008

Publication series

Name	AIP Conference Proceedings
Volume	1111
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	International Conference on Probing Stellar Populations Out To The Distant Universe, Cefalu 2008
Country/Territory	Italy
City	Cefalu, Sicily
Period	9/7/08 → 9/19/08

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

Keywords

Galaxy evolution
Galaxy formation

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10.1063/1.3141597

Cite this

Monaco, P., Fontanot, F., Lo Faro, B., De Lucia, G., Vanzella, E., Somerville, R., Cristiani, S., Silva, L., & Santini, P. (2009). Modeling multi-wavelength properties of high redshift galaxies. In Probing Stellar Populations Out To The Distant Universe - Cefalu 2008 - Proceedings of the International Conference (pp. 48-51). (AIP Conference Proceedings; Vol. 1111). https://doi.org/10.1063/1.3141597

@inproceedings{0b30ab5f40134642a3eef317bcf4c8ef,

title = "Modeling multi-wavelength properties of high redshift galaxies",

abstract = "By comparing galaxy formation models within the ACDM cosmology with available data on high redshift galaxies, we show that small galaxies , with stellar masses < 1011 M, are formed too early, are too passive since z{\~ } 3 and too old at z = 0. This is due to an overproduction of small galaxies at high redshift, visible also as an excess of ZAB{\~ } 27 V-dropouts. We discuss the consequences of this excess.",

keywords = "Galaxy evolution, Galaxy formation",

author = "Pierluigi Monaco and Fabio Fontanot and {Lo Faro}, Barbara and {De Lucia}, Gabriella and Eros Vanzella and Rachel Somerville and Stefano Cristiani and Laura Silva and Paola Santini",

year = "2009",

doi = "10.1063/1.3141597",

language = "English (US)",

isbn = "9780735406483",

series = "AIP Conference Proceedings",

pages = "48--51",

booktitle = "Probing Stellar Populations Out To The Distant Universe - Cefalu 2008 - Proceedings of the International Conference",

note = "International Conference on Probing Stellar Populations Out To The Distant Universe, Cefalu 2008 ; Conference date: 07-09-2008 Through 19-09-2008",

}

Monaco, P, Fontanot, F, Lo Faro, B, De Lucia, G, Vanzella, E, Somerville, R, Cristiani, S, Silva, L & Santini, P 2009, Modeling multi-wavelength properties of high redshift galaxies. in Probing Stellar Populations Out To The Distant Universe - Cefalu 2008 - Proceedings of the International Conference. AIP Conference Proceedings, vol. 1111, pp. 48-51, International Conference on Probing Stellar Populations Out To The Distant Universe, Cefalu 2008, Cefalu, Sicily, Italy, 9/7/08. https://doi.org/10.1063/1.3141597

Modeling multi-wavelength properties of high redshift galaxies. / Monaco, Pierluigi; Fontanot, Fabio; Lo Faro, Barbara et al.
Probing Stellar Populations Out To The Distant Universe - Cefalu 2008 - Proceedings of the International Conference. 2009. p. 48-51 (AIP Conference Proceedings; Vol. 1111).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Modeling multi-wavelength properties of high redshift galaxies

AU - Monaco, Pierluigi

AU - Fontanot, Fabio

AU - Lo Faro, Barbara

AU - De Lucia, Gabriella

AU - Vanzella, Eros

AU - Somerville, Rachel

AU - Cristiani, Stefano

AU - Silva, Laura

AU - Santini, Paola

PY - 2009

Y1 - 2009

N2 - By comparing galaxy formation models within the ACDM cosmology with available data on high redshift galaxies, we show that small galaxies , with stellar masses < 1011 M, are formed too early, are too passive since z ̃ 3 and too old at z = 0. This is due to an overproduction of small galaxies at high redshift, visible also as an excess of ZAB ̃ 27 V-dropouts. We discuss the consequences of this excess.

AB - By comparing galaxy formation models within the ACDM cosmology with available data on high redshift galaxies, we show that small galaxies , with stellar masses < 1011 M, are formed too early, are too passive since z ̃ 3 and too old at z = 0. This is due to an overproduction of small galaxies at high redshift, visible also as an excess of ZAB ̃ 27 V-dropouts. We discuss the consequences of this excess.

KW - Galaxy evolution

KW - Galaxy formation

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UR - http://www.scopus.com/inward/citedby.url?scp=67650564661&partnerID=8YFLogxK

U2 - 10.1063/1.3141597

DO - 10.1063/1.3141597

M3 - Conference contribution

AN - SCOPUS:67650564661

SN - 9780735406483

T3 - AIP Conference Proceedings

SP - 48

EP - 51

BT - Probing Stellar Populations Out To The Distant Universe - Cefalu 2008 - Proceedings of the International Conference

T2 - International Conference on Probing Stellar Populations Out To The Distant Universe, Cefalu 2008

Y2 - 7 September 2008 through 19 September 2008

ER -

Modeling multi-wavelength properties of high redshift galaxies

Abstract

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Keywords

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