An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: an unbiased study of SMG environments measured with narrow-band imaging
Artikel i vetenskaplig tidskrift, 2024
Submillimetre galaxies (SMGs) are some of the most extreme star-forming systems in the Universe, whose place in the framework of galaxy evolution is as yet uncertain. It has been hypothesized that SMGs are progenitors of local early-type galaxies, requiring that SMGs generally reside in galaxy cluster progenitors at high redshift. We test this hypothesis and explore SMG environments using a narrow-band VLT/HAWK-I+GRAAL study of H α and [O III] emitters around an unbiased sample of three ALMA-identified and spectroscopically confirmed SMGs at z ∼ 2.3 and ∼ 3.3, where these SMGs were selected solely on spectroscopic redshift. Comparing with blank-field observations at similar epochs, we find that one of the three SMGs lies in an overdensity of emission-line sources on the ∼ 4 Mpc scale of the HAWK-I field of view, with overdensity parameter δg = 2.6+1.4-1.2. A second SMG is significantly overdense only on ≲ 1.6 Mpc scales and the final SMG is consistent with residing in a blank field environment. The total masses of the two overdensities are estimated to be log(Mh/M☉) = 12.1–14.4, leading to present-day masses of log(Mh, z=0/M☉) = 12.9–15.9. These results imply that SMGs occupy a range of environments, from overdense protoclusters or protogroups to the blank field, suggesting that while some SMGs are strong candidates for the progenitors of massive elliptical galaxies in clusters, this may not be their only possible evolutionary pathway.
galaxies: photometry
submillimetre: galaxies
galaxies: evolution
galaxies: star formation
Författare
Thomas M. Cornish
University of Oxford
Department of Physics, Lancaster University
J. L. Wardlow
Department of Physics, Lancaster University
Heather Wade
Department of Physics, Lancaster University
David Sobral
Department of Physics, Lancaster University
BNP Paribas
W. N. Brandt
Eberly College of Science
Pennsylvania State University
P. Cox
Institut d 'Astrophysique de Paris
H. Dannerbauer
Universidad de la Laguna
Instituto de Astrofísica de Canarias
R. Decarli
Istituto nazionale di astrofisica (INAF)
B. Gullberg
Danmarks Tekniske Universitet (DTU)
The Cosmic Dawn Centre (DAWN)
Kirsten Knudsen
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
John Stott
Department of Physics, Lancaster University
Mark Swinbank
Durham University
F. Walter
Max-Planck-Gesellschaft
P. van der Werf
Universiteit Leiden
Monthly Notices of the Royal Astronomical Society
00358711 (ISSN) 13652966 (eISSN)
Vol. 533 2 2399-2419Ämneskategorier
Astronomi, astrofysik och kosmologi
DOI
10.1093/mnras/stae1868