![]() ![]() We used the VLT/FORS2 multi-object spectrograph to target ~80 high-redshift galaxy candidates, and obtain robust spectroscopic redshifts for more than half the targets. ![]() The structure was initially discovered as an overdensity of both near-infrared selected z > 1.6 and mid-infrared selected z > 1.2 galaxy candidates. We present the spectroscopic confirmation of a structure of galaxies surrounding the radio galaxy MRC 0156-252 at z = 2.02. Astronomical objects: linking to databasesĪudrey Galametz 1, Daniel Stern 2, Laura Pentericci 1, Carlos De Breuck 3, Joël Vernet 3, Dominika Wylezalek 3, Rene Fassbender 1 ,5, Nina Hatch 4, Jaron Kurk 5, Roderik Overzier 6 ,7, Alessandro Rettura 8 and Nick Seymour 9ġ INAF – Osservatorio di Roma, via Frascati 33, 00040 Monteporzio, ItalyĮ-mail: Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USAģ European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching, GermanyĤ University of Nottingham, School of Physics and Astronomy, Nottingham NG7 2RD, UKĥ Max-Planck-Institut für extraterrestrische Physik (MPE), Postfach 1312, Giessenbachstr., 85741 Garching, GermanyĦ Observatório Nacional, Rua José Cristino 77, CEP 20921-400 São Cristóvão, Rio de Janeiro, RJ, Brazilħ Department of Astronomy, The University of Texas at Austin, 2515 Speedway, Stop C1400, Austin, TX 78712, USAĨ Department of Astrophysics, California Institute of Technology, MS 249-17, Pasadena, CA 91125, USAĩ CSIRO Astronomy & Space Science, PO Box 76, NSW 1710 Epping, Australia.Including author names using non-Roman alphabets.Suggested resources for more tips on language editing in the sciences ![]() Punctuation and style concerns regarding equations, figures, tables, and footnotes ![]()
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