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The evolution of activity in galaxies from z=0.45 to the present time

Published online by Cambridge University Press:  25 July 2014

Grażyna Stasińska
Affiliation:
LUTH, Observatoire de Paris, CNRS, Université Paris Diderot, Place Jules Janssen, F-92190 Meudon email: [email protected]
M. V. Costa-Duarte
Affiliation:
LUTH, Observatoire de Paris, CNRS, Université Paris Diderot, Place Jules Janssen, F-92190 Meudon email: [email protected] Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, São Paulo, Brazil email: [email protected]
N. Vale Asari
Affiliation:
Departamento de Física - CFM - Universidade Federal de Santa Catarina, Florianópolis, SC, Brazil email: [email protected]
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Abstract

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We use spectra from the SDSS to study the signatures of nuclear activity over cosmic time, dividing the samples in redshift and mass bins, and using various diagnostic diagrams. A redshift evolution clearly emerges from the analysis of our diagrams.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

Abazajian, K. N., et al., 2009, ApJS, 182, 543CrossRefGoogle Scholar
Baldwin, J. A., Phillips, M. M., & Terlevich, R., 1981, PASP, 93, 5CrossRefGoogle Scholar
Cid Fernandes, R., Stasińska, G., Mateus, A., & Vale Asari, N., 2011, MNRAS, 413, 1687Google Scholar
Cowie, L. L., Songaila, A., Hu, E. M., & Cohen, J. G., 1996, AJ, 112, 839CrossRefGoogle Scholar
Dopita, M. A., et al., 2013, ApJS, 208, 10Google Scholar
Kauffmann, G., et al., 2003, MNRAS, 346, 1055Google Scholar
Kewley, L. J., Dopita, M. A., Sutherland, R. S., Heisler, C. A., & Trevena, J., 2001, ApJ, 556, 121CrossRefGoogle Scholar
Stasińska, G., et al., 2008, MNRAS, 391, L29Google Scholar