The progeny of a cosmic titan: a massive multi-component proto-supercluster in formation at z = 2.45 in VUDS

@article{Cucciati2018ThePO,
  title={The progeny of a cosmic titan: a massive multi-component proto-supercluster in formation at z = 2.45 in VUDS},
  author={Olga Cucciati and Brian C. Lemaux and Gianni Zamorani and Olivier Le F{\`e}vre and L. A. M. Tasca and Nimish P. Hathi and K-G. Lee and Sandro Bardelli and Paolo Cassata and Bianca Garilli and Vincent Le Brun and Dario Maccagni and Laura Pentericci and R. Thomas and Eros Vanzella and Elena Zucca and Lori M. Lubin and Ricardo Amor{\'i}n and Letizia P. Cassar{\`a} and Andrea Cimatti and Margherita Talia and D. Vergani and Anton M. Koekemoer and J Pforr and Mara Salvato},
  journal={Astronomy \& Astrophysics},
  year={2018}
}
We unveil the complex shape of a proto-supercluster at z ∼ 2.45 in the COSMOS field exploiting the synergy of both spectroscopic and photometric redshifts. Thanks to the spectroscopic redshifts of the VIMOS Ultra-Deep Survey (VUDS), complemented by the zCOSMOS-Deep spectroscopic sample and high-quality photometric redshifts, we compute the three-dimensional (3D) overdensity field in a volume of ∼100 × 100 × 250 comoving Mpc3 in the central region of the COSMOS field, centred at z ∼ 2.45 along… 
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