Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey - II. Extending the mass-metallicity relation to the range z ≈ 0.89–1.24

Free Access

Table 1:

Distribution of star-forming galaxies and narrow-line AGNs among VVDS emission-line galaxies using the ``blue'' diagnostic diagrams based on the relation between [O III] (blue, 0.5 < z < 0.9) or [Ne III] (blue-Ne, 0.5 < z < 1.24) and [O II] emission lines. We show the distribution for the whole sample and for wide and deep fields. In the wide classification we include those galaxies belonging to the deep fields having $I_{\rm AB} \leq 22.5$ .
	0.5 <z< 0.9		0.5 <z< 0.9		z> 0.9
Sample/Diagnostic	blue	%	blue-Ne	%	blue-Ne	%
Wide
Emission-line (total)	924	100	338	100	62	100
Star-forming	768	83	157	45	34	55
Candidates	138	15	142	42	27	43
Seyfert 2	18	2	39	12	1	2
LINER	0	0	0	0	0	0
Deep
Emission-line (total)	568	100	197	100	36	100
Star-forming	412	73	110	56	18	50
Candidates	139	24	79	40	17	47
Seyfert 2	17	3	8	4	1	3
LINER	0	0	0	0	0	0
Total
Emission-line (total)	1213	100	418	100	72	100
Star-forming	945	78	216	52	40	55
Candidates	236	20	163	39	30	42
Seyfert 2	32	3	39	9	2	3
LINER	0	0	0	0	0	0

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.