FLASH: Faint Lenses from Associated Selection with Herschel
Artikel i vetenskaplig tidskrift, 2024

We report the ALMA Band 7 observations of 86 Herschel sources that likely contain gravitationally lensed galaxies. These sources are selected with relatively faint 500 μm flux densities between 15 and 85 mJy in an effort to characterize the effect of lensing across the entire million-source Herschel catalogue. These lensed candidates were identified by their close proximity to bright galaxies in the near-infrared VISTA Kilo-Degree Infrared Galaxy survey. Our high-resolution observations (0.15 arcsec) confirm 47 per cent of the initial candidates as gravitational lenses, while lensing cannot be excluded across the remaining sample. We find average lensing masses (log M/M⃝ = 12.9 ± 0.5) in line with previous experiments, although direct observations might struggle to identify the most massive foreground lenses across the remaining 53 per cent of the sample, particularly for lenses with larger Einstein radii. Our observations confirm previous indications that more lenses exist at low flux densities than expected from strong galaxy–galaxy lensing models alone, where the excess is likely due to additional contributions of cluster lenses and weak lensing. If we apply our method across the total 660 square degree H-ATLAS field, it would allow us to robustly identify 3000 gravitational lenses across the 660 square degree Herschel ATLAS fields.

submillimetre: galaxies

general

galaxies: evolution

gravitational lensing: strong

galaxies: high-redshift

Författare

Tom Bakx

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Nagoya University

National Astronomical Observatory of Japan

Bethany S. Gray

University of Bath

J. González-Nuevo

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

Universidad de Oviedo

L. Bonavera

Universidad de Oviedo

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

A. Amvrosiadis

Durham University

S. Eales

Cardiff University

Masato Hagimoto

Nagoya University

S. Serjeant

Open University

Monthly Notices of the Royal Astronomical Society

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

Vol. 527 3 8865-8885

Ämneskategorier

Subatomär fysik

Astronomi, astrofysik och kosmologi

DOI

10.1093/mnras/stad3759

Mer information

Senast uppdaterat

2024-01-18