Survey of Gravitationally lensed objects in HSC Imaging (SuGOHI). VIII. New galaxy-scale lenses from the HSC SSP

Author:

Wong Kenneth C1ORCID,Chan James H H2,Chao Dani C-Y345,Jaelani Anton T6ORCID,Kayo Issha7ORCID,Lee Chien-Hsiu8,More Anupreeta910ORCID,Oguri Masamune101112

Affiliation:

1. National Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

2. Institute of Physics, Laboratory of Astrophysics , Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland

3. Ruđer Bošković Institute , Bijenička cesta 54, 10000 Zagreb, Croatia

4. Max Planck Institute for Astrophysics , Karl-Schwarzschild-Straße 1, 85741 Garching, Germany

5. Physik-Department, Technische Universität München , James-Franck-Straße 1, 85748 Garching, Germany

6. Astronomy Research Group and Bosscha Observatory , FMIPA, Institut Teknologi Bandung, Jl. Ganesha 10, Bandung 40132, Indonesia

7. Department of Liberal Arts, Tokyo University of Technology , 5-23-22 Nishikamata, Ota, Tokyo 144-8650, Japan

8. NSF’s National Optical-Infrared Astronomy Research Laboratory , 950 N. Cherry Avenue, Tucson, AZ 85719, USA

9. The Inter-University Centre for Astronomy and Astrophysics (IUCAA) , Post Bag 4, Ganeshkhind, Pune 411007, India

10. Kavli IPMU (WPI), UTIAS, The University of Tokyo , 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan

11. Center for Frontier Science, Chiba University , 1-33 Yayoi-cho, Inage-ku, Chiba 263-8522, Japan

12. Research Center for the Early Universe, The University of Tokyo , 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

Abstract

Abstract We conduct a search for galaxy-scale strong gravitational lens systems in Data Release 4 of the Hyper Suprime-Cam Subaru Strategic Program (HSC SSP), consisting of data taken up to the S21A semester. We select 103191 luminous red galaxies from the Baryon Oscillation Spectroscopic Survey (BOSS) sample that have deep multiband imaging from the HSC SSP and use the YattaLens algorithm to identify lens candidates with blue arc-like features automatically. The candidates are visually inspected and graded based on their likelihood of being a lens. We find eight definite lenses, 28 probable lenses, and 138 possible lenses. The new lens candidates generally have lens redshifts in the range 0.3 ≲ zL ≲ 0.9, a key intermediate redshift range to study the evolution of galaxy structure. Follow-up spectroscopy will confirm these new lenses and measure source redshifts to enable detailed lens modeling.

Funder

National Astronomical Observatory of Japan

Kavli Institute for the Physics and Mathematics of the Universe

University of Tokyo

High Energy Accelerator Research Organization

Academia Sinica Institute for Astronomy and Astrophysics

Princeton University

Ministry of Education, Culture, Sports, Science and Technology

Japan Society for the Promotion of Science

Japan Science and Technology Agency

Toray Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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