906 citations
- O. Fèvre13 · h 98
- A. Mazure3 profiles12 · h 48
- H. Gouin11 · h 20
- B. Garilli2 profiles10 · h 77
- C. Adami2 profiles10 · h 56
- L. Guzzo2 profiles10 · h 73
- R. Pelló2 profiles10 · h 62
- D. Maccagni3 profiles9 · h 65
- L. Tresse2 profiles9 · h 79
- O. Ilbert2 profiles9 · h 102
- A. Cappi2 profiles8 · h 69
- B. Meneux2 profiles8 · h 45
- Laboratoire d’Astrophysique de MarseilleFR54 papers
- Centre National de la Recherche ScientifiqueFR39 papers
- Institut d'Astrophysique de ParisFR23 papers
- Observatoire de ParisFR19 papers
- Université Paris CitéFR15 papers
- Aix-Marseille UniversitéFR14 papers
- Janssen (France)FR14 papers
- Sorbonne UniversitéFR14 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR13 papers
- Institut Universitaire des Systèmes Thermiques IndustrielsFR13 papers
- CEA Paris-SaclayFR10 papers
- Laboratoire de Mécanique, Modélisation & Procédés PropresFR10 papers
Showing 2010 · astro-ph.COShow all
3 papers · 2 filters
astro-ph.CO2010★ 75 cited
The VIMOS VLT Deep Survey: the contribution of minor mergers to the growth of L_B >= L*_B galaxies since z ~ 1 from spectroscopically identified pairs
C. López-Sanjuan, O. Le Fèvre, L. de Ravel +14
In this work we measure the merger fraction, f_m, of L_B >= L*_B galaxies in the VVDS-Deep spectroscopic Survey. We define kinematical close pairs as those galaxies with a separati…
astro-ph.CO2010★ 26 cited
The DAFT/FADA survey. I.Photometric redshifts along lines of sight to clusters in the z=[0.4,0.9] interval
L. Guennou, C. Adami, M. P. Ulmer +20
As a contribution to the understanding of the dark energy concept, the Dark energy American French Team (DAFT, in French FADA) has started a large project to characterize statistic…
astro-ph.CO2010★ 34 cited
Spectro-photometric close pairs in GOODS-S: major and minor companions of intermediate-mass galaxies
C. López-Sanjuan, M. Balcells, P. G. Pérez-González +3
(Abriged) Our goal here is to provide merger frequencies that encompass both major and minor mergers, derived from close pair statistics. We use B-band luminosity- and mass-limited…