Details

Autor(en) / Beteiligte

• Shah, Ekta A
• Lemaux, Brian
• Forrest, Benjamin
• Cucciati, Olga
• Hung, Denise
• Staab, Priti
• Hathi, Nimish
• Lubin, Lori
• Gal, Roy R
• Shen, Lu
• Zamorani, Giovanni
• Giddings, Finn
• Bardelli, Sandro
• Cassara, Letizia Pasqua
• Cassata, Paolo
• Contini, Thierry
• Golden-Marx, Emmet
• Guaita, Lucia
• Gururajan, Gayathri
• Koekemoer, Anton M
• McLeod, Derek
• Tasca, Lidia A M
• Tresse, Laurence
• Vergani, Daniela
• Zucca, Elena

Titel

Identification and characterization of six spectroscopically confirmed massive protostructures at 2.5 < z < 4.5

Ist Teil von

• Monthly notices of the Royal Astronomical Society, 2024-04, Vol.529 (2), p.873-882

Ort / Verlag

Oxford University Press

Erscheinungsjahr

2024

Link zum Volltext

Quelle

EZB Electronic Journals Library

Beschreibungen/Notizen

• ABSTRACT We present six spectroscopically confirmed massive protostructures, spanning a redshift range of 2.5 < z < 4.5 in the Extended Chandra Deep Field South (ECDFS) field discovered as part of the Charting Cluster Construction in VUDS and ORELSE (C3VO) survey. We identify and characterize these remarkable systems by applying an overdensity measurement technique on an extensive data compilation of public and proprietary spectroscopic and photometric observations in this highly studied extragalactic field. Each of these six protostructures, i.e. a large scale overdensity (volume >9000 cMpc3) of more than 2.5σδ above the field density levels at these redshifts, have a total mass Mtot ≥ 1014.8 M⊙ and one or more highly overdense (overdensity$\, \gt 5\sigma _{\delta }$) peaks. One of the most complex protostructures discovered is a massive (Mtot = 1015.1M⊙) system at z ∼ 3.47 that contains six peaks and 55 spectroscopic members. We also discover protostructures at z ∼ 3.30 and z ∼ 3.70 that appear to at least partially overlap on sky with the protostructure at z ∼ 3.47, suggesting a possible connection. We additionally report on the discovery of three massive protostructures at z = 2.67, 2.80, and 4.14 and discuss their properties. Finally, we discuss the relationship between star formation rate and environment in the richest of these protostructures, finding an enhancement of star formation activity in the densest regions. The diversity of the protostructures reported here provide an opportunity to study the complex effects of dense environments on galaxy evolution over a large redshift range in the early Universe.