HOLISMOKES. VIII. High-redshift, strong-lens search in the Hyper Suprime-Cam Subaru Strategic Program
arXiv:2201.11135 · doi:10.1051/0004-6361/202243203
Abstract
We carry out a search for strong-lens systems containing high-redshift lens galaxies with the goal of extending strong-lensing-assisted galaxy evolutionary studies to earlier cosmic time. Two strong-lens classifiers are constructed from a deep residual network and trained with datasets of different lens-redshift and brightness distributions. We classify a sample of 5,356,628 pre-selected objects from the Wide-layer fields in the second public data release of the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) by applying the two classifiers to their HSC -filter cutouts. Cutting off at thresholds that correspond to a false positive rate of on our test set, the two classifiers identify 5,468 and 6,119 strong-lens candidates. Visually inspecting the cutouts of those candidates results in 735 grade-A or B strong-lens candidates in total, of which 277 candidates are discovered for the first time. This is the single largest set of galaxy-scale strong-lens candidates discovered with HSC data to date, and nearly half of it (331/735) contains lens galaxies with photometric redshifts above 0.6. Our discoveries will serve as a valuable target list for ongoing and scheduled spectroscopic surveys such as the Dark Energy Spectroscopic Instrument, the Subaru Prime Focus Spectrograph project, and the Maunakea Spectroscopic Explorer.
15 pages, 8 figures + appendices, published on the A&A
References in corpus (22)
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: to 3.8% precision from strong lensing in a flat CDM model
- The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
- The Halos of Satellite Galaxies: the Companion of the Massive Elliptical Lens SL2S J08544-0121
- The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies
- LinKS: Discovering galaxy-scale strong lenses in the Kilo-Degree Survey using Convolutional Neural Networks
- The Sloan Lens ACS Survey. XIII. Discovery of 40 New Galaxy-Scale Strong Lenses
- The Sloan Lens ACS Survey. XII. Extending Strong Lensing to Lower Masses
- The Low Mass End of the Fundamental Relation for Gravitationally Lensed Star Forming Galaxies at 1<z<6
- The BOSS Emission-Line Lens Survey. IV. : Smooth Lens Models for the BELLS GALLERY Sample
- How to Find Gravitationally Lensed Type Ia Supernovae
- HOLISMOKES. VI. New galaxy-scale strong lens candidates from the HSC-SSP imaging survey
- Red nuggets grow inside-out: evidence from gravitational lensing
- On building a cluster watch-list for identifying strongly lensed supernovae, gravitational waves and kilonovae
- The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition
- A new quadruple gravitational lens from the Hyper Suprime-Cam Survey: the puzzle of HSC~J115252+004733
- Discovery of a Strong Lensing Galaxy Embedded in a Cluster at z = 1.62
- A census of optically dark massive galaxies in the early Universe from magnification by lensing galaxy clusters
- Planck's Dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5
- Rest-frame UV Properties of Luminous Strong Gravitationally Lensed Ly Emitters from the BELLS GALLERY Survey
- Discovery of a Very Bright and Intrinsically Very Luminous, Strongly Lensed Lyα Emitting Galaxy at z = 2.82 in the BOSS Emission-Line Lens Survey
- Discovering Strongly-lensed QSOs From Unresolved Light Curves