Astronomy and Astrophysics, 486, pp. 177-189, http://dx.doi.org./10.1051/0004-6361:09394
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2008 (v1)Journal articleUploaded on: December 4, 2022
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2009 (v1)Journal article
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August 2020 (v1)Journal article
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2009 (v1)Journal article
Astronomy and Astrophysics, 507, pp. 405-415 (2009)
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November 2013 (v1)Journal article
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2009 (v1)Journal article
Astronomy and Astrophysics, 508, pp. 289-295 (2009)
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2008 (v1)Journal article
Physica Scripta Volume T, 133, p. 4032, http://dx.doi.org./10.1088/0031-8949//t133/014032
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June 2018 (v1)Journal article
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March 2017 (v1)Journal article
Context. Several recent studies have demonstrated that the Galactic bulge hosts two components with different mean metallicities, and possibly different spatial distribution and kinematics. As a consequence, both the metallicity distribution and the radial velocity of bulge stars vary across different lines of sight. Aims: We present here the...
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2011 (v1)Journal article
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2007 (v1)Journal article
Astrophysical Journal, 663, pp. 296-314, http://dx.doi.org./10.1086/517905
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December 2015 (v1)Journal article
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2007 (v1)Journal article
Astronomy and Astrophysics, 474, pp. 105-119, http://dx.doi.org./10.1051/0004-6361:7806
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February 2014 (v1)Journal article
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2013 (v1)Journal article
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2013 (v1)Journal article
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2010 (v1)Journal article
Astronomy and Astrophysics, 509, p. A20 (2010)
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August 2012 (v1)Journal article
We present a group-galaxy cross-correlation analysis using a group catalog produced from the 16,500 spectra from the optical zCOSMOS galaxy survey. Our aim is to perform a consistency test in the redshift range 0.2 \textless= z \textless= 0.8 between the clustering strength of the groups and mass estimates that are based on the richness of the...
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March 2013 (v1)Journal article
We identify 42 "candidate groups" lying between 1.8\textlessz\textless3.0 from a sample of 3502 galaxies with spectroscopic redshifts in the zCOSMOS-deep redshift survey within this same redshift interval. These systems contain three to five spectroscopic galaxies that lie within 500 kpc in projected distance (in physical space) and within 700...
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April 2011 (v1)Journal article
We use the overdensity field reconstructed in the volume of the COSMOS area to study the nonlinear biasing of the zCOSMOS galaxies. The galaxy overdensity field is reconstructed using the current sample of ~8500 accurate zCOSMOS redshifts at I(AB)<22.5 out to z~1 on scales R from 8 to 12 Mpc/h. By comparing the probability distribution function...
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January 2011 (v1)Journal article
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January 2013 (v1)Journal article
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