The VIMOS VLT Deep Survey: A census of active and passive galaxies to redshift 1.3
2006 ◽
Vol 2
(S235)
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pp. 400-400
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AbstractWe are studying how stellar masses assemble through cosmic time since the Universe had only 30% of its present age. We are conducting a census of galaxies which covers the end of the most active star-forming phase, using a mass-limited sample of approximately 5,000 objects selected from the VIMOS VLT Deep Survey (VVDS) in the redshift range 0.45 < z < 1.3. With a criterion based on the direct spectral measurement of the 4000Å Balmer break, Dn(4000), we have classified our sample in spectroscopically early and late-type galaxies. The trends existing between stellar mass, spectroscopic classification, and star formation activity are clearly shown in our analysis.
2020 ◽
Vol 499
(1)
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pp. 948-956
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2020 ◽
Vol 493
(4)
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pp. 5596-5605
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2010 ◽
Vol 19
(08n10)
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pp. 1371-1377
2016 ◽
Vol 11
(S321)
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pp. 273-273
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2020 ◽
Vol 501
(2)
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pp. 2231-2249
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2006 ◽
Vol 2
(14)
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pp. 248-248
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2013 ◽
Vol 9
(S304)
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pp. 343-344
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2006 ◽
Vol 2
(S235)
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pp. 368-372
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2019 ◽
Vol 489
(1)
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pp. 339-348
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