The bright extragalactic ALMA redshift survey (BEARS) – II. Millimetre photometry of gravitational lens candidates
Journal article, 2023

We present 101- and 151-GHz ALMA continuum images for 85 fields selected from Herschel observations that have 500-μm flux densities >80 mJy and 250–500-μm colours consistent with z > 2, most of which are expected to be gravitationally lensed or hyperluminous infrared galaxies. Approximately half of the Herschel 500-μm sources were resolved into multiple ALMA sources, but 11 of the 15 brightest 500-μm Herschel sources correspond to individual ALMA sources. For the 37 fields containing either a single source with a spectroscopic redshift or two sources with the same spectroscopic redshift, we examined the colour temperatures and dust emissivity indices. The colour temperatures only vary weakly with redshift and are statistically consistent with no redshift-dependent temperature variations, which generally corresponds to results from other samples selected in far-infrared, submillimetre, or millimetre bands but not to results from samples selected in optical or near-infrared bands. The dust emissivity indices, with very few exceptions, are largely consistent with a value of 2. We also compared spectroscopic redshifts to photometric redshifts based on spectral energy distribution templates designed for infrared-bright high-redshift galaxies. While the templates systematically underestimate the redshifts by ∼15 per cent, the inclusion of ALMA data decreases the scatter in the predicted redshifts by a factor of ∼2, illustrating the potential usefulness of these millimetre data for estimating photometric redshifts.

submillimetre: galaxies

galaxies: ISM

galaxies: high-redshift

infrared: galaxies

Author

G. J. Bendo

University of Manchester

S. Urquhart

Open University

S. Serjeant

Open University

Tom J.L.C. Bakx

National Astronomical Observatory of Japan

Nagoya University

Masato Hagimoto

Nagoya University

P. Cox

Institut d 'Astrophysique de Paris

R. Neri

Institut de Radioastronomie Millimétrique (IRAM)

M. Lehnert

École Normale Supérieure de Lyon

H. Dannerbauer

University of La Laguna

Instituto de Astrofísica de Canarias

A. Amvrosiadis

Durham University

P. Andreani

European Southern Observatory (ESO)

A. J. Baker

Rutgers University

University of the Western Cape

A. Beelen

Laboratoire d'Astrophysique de Marseille

S. Berta

Institut de Radioastronomie Millimétrique (IRAM)

E. Borsato

University of Padua

V. Buat

Laboratoire d'Astrophysique de Marseille

K. M. Butler

Leiden University

A. Cooray

University of California at Irvine (UCI)

G. De Zotti

Istituto nazionale di astrofisica (INAF)

L. Dunne

Cardiff University

S. Dye

University of Nottingham

S. Eales

Cardiff University

A. F.M. Enia

Istituto nazionale di astrofisica (INAF)

University of Bologna

Lulu Fan

University of Science and Technology of China

R. Gavazzi

Laboratoire d'Astrophysique de Marseille

Institut d 'Astrophysique de Paris

J. González-Nuevo

Instituto Universitario de Ciencias y Tecnologías Espaciales de Asturias (ICTEA)

University of Oviedo

A. I. Harris

University of Maryland

C. N. Herrera

Institut de Radioastronomie Millimétrique (IRAM)

D. Hughes

National Institute of Astrophysics, Optics and Electronics

D. Ismail

Laboratoire d'Astrophysique de Marseille

B. M. Jones

University of Cologne

K. Kohno

University of Tokyo

Research Center for the Early Universe

M. Krips

Institut de Radioastronomie Millimétrique (IRAM)

Guilaine Lagache

Laboratoire d'Astrophysique de Marseille

L. Marchetti

Istituto nazionale di astrofisica (INAF)

University of Cape Town

M. Massardi

Istituto nazionale di astrofisica (INAF)

Scuola Internazionale Superiore di Studi Avanzati

H. Messias

Atacama Large Millimeter-submillimeter Array (ALMA)

European Southern Observatory Santiago

M. Negrello

Cardiff University

A.A. Omont

Institut d 'Astrophysique de Paris

I. Perez-Fournon

Instituto de Astrofísica de Canarias

University of La Laguna

D. A. Riechers

University of Cologne

D. Scott

University of British Columbia (UBC)

M. W.L. Smith

Cardiff University

F. Stanley

Institut de Radioastronomie Millimétrique (IRAM)

Y. Tamura

Nagoya University

P. Temi

NASA Ames Research Center

P. van der Werf

Leiden University

A. Verma

University of Oxford

C. Vlahakis

National Radio Astronomy Observatory

A. Weiss

Max Planck Society

Chentao Yang

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

A. J. Young

Rutgers University

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 522 2 2995-3017

Subject Categories

Astronomy, Astrophysics and Cosmology

Other Electrical Engineering, Electronic Engineering, Information Engineering

DOI

10.1093/mnras/stac3771

More information

Latest update

9/15/2023