S-PLUS DR1 galaxy clusters and groups catalogue using PzWav

Author:

Werner S V12ORCID,Cypriano E S2,Gonzalez A H3ORCID,Mendes de Oliveira C2,Araya-Araya P2ORCID,Doubrawa L2,Lopes de Oliveira R245,Lopes P A A6ORCID,Vitorelli A Z27,Brambila D6,Costa-Duarte M2,Telles E5,Kanaan A8,Ribeiro T9,Schoenell W10,Gonçalves T S6,Menéndez-Delmestre K6,Bom C R1112,Nakazono L2ORCID

Affiliation:

1. School of Physics and Astronomy, University of Nottingham , Nottingham, NG7 2RD, UK

2. Departamento de Astronomia, Instituto de Astronomia, Geofísica e Ciências Atmosféricas da USP, Cidade Universitária , 05508-900 São Paulo, SP, Brazil

3. Department of Astronomy, University of Florida , 211, Bryant Space Center, Gainesville, FL 32611, USA

4. Departamento de Física, Universidade Federal de Sergipe , Av. Marechal Rondon, S/N, 49100-000 São Cristóvão, SE, Brazil

5. Observatório Nacional , Rua General José Cristino, 77, São Cristóvão, 20921-400 Rio de Janeiro, RJ, Brazil

6. Observatório do Valongo, Universidade Federal do Rio de Janeiro , Ladeira Pedro Antônio 43, Rio de Janeiro, RJ 20080-090, Brazil

7. AIM, CEA, CNRS, Université Paris-Saclay, Université de Paris , F-91191 Gif-sur-Yvette, France

8. Departamento de Física, Universidade Federal de Santa Catarina , Florianópolis, SC, 88040-900, Brazil

9. NOAO , 950 North Cherry Ave. Tucson, AZ 85719, United States

10. GMTO Corporation , N. Halstead Street 465, Suite 250, Pasadena, CA 91107, United States

11. Centro Brasileiro de Pesquisas Físicas , Rua Dr. Xavier Sigaud 150, CEP 22290-180 Rio de Janeiro, RJ, Brazil

12. Centro Federal de Educação Tecnológica Celso Suckow da Fonseca , Rodovia Mário Covas, lote J2, quadra J, CEP 23810-000 Itaguaí, RJ, Brazil

Abstract

ABSTRACT We present a catalogue of 4499 groups and clusters of galaxies from the first data release of the multi-filter (5 broad, 7 narrow) Southern Photometric Local Universe Survey (S-PLUS). These groups and clusters are distributed over 273 deg2 in the Stripe 82 region. They are found using the PzWav algorithm, which identifies peaks in galaxy density maps that have been smoothed by a cluster scale difference-of-Gaussians kernel to isolate clusters and groups. Using a simulation-based mock catalogue, we estimate the purity and completeness of cluster detections: at S/N > 3.3, we define a catalogue that is 80 per cent pure and complete in the redshift range 0.1 < z < 0.4, for clusters with M200 > 1014 M⊙. We also assessed the accuracy of the catalogue in terms of central positions and redshifts, finding scatter of σR = 12 kpc and σz = 8.8 × 10−3, respectively. Moreover, less than 1 per cent of the sample suffers from fragmentation or overmerging. The S-PLUS cluster catalogue recovers ∼80 per cent of all known X-ray and Sunyaev-Zel’dovich selected clusters in this field. This fraction is very close to the estimated completeness, thus validating the mock data analysis and paving an efficient way to find new groups and clusters of galaxies using data from the ongoing S-PLUS project. When complete, S-PLUS will have surveyed 9300 deg2 of the sky, representing the widest uninterrupted areas with narrow-through-broad multi-band photometry for cluster follow-up studies.

Funder

CNPq

Fundação de Amparo à Pesquisa do Estado de São Paulo

Federal University of Santa Catarina

São Paulo Research Foundation

Coordination for the Improvement of Higher Education Personnel

FAPERJ

FINEP

ESC

FAPESP

Serrapilheira Institute

Chinese Academy of Sciences

National Aeronautics and Space Administration

U.S. Department of Energy

National Energy Research Scientific Computing Center

National Science Foundation

Division of Astronomical Sciences

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. A case study of an early galaxy cluster with the Athena X-IFU;Astronomy & Astrophysics;2024-01-31

2. Galaxy cluster optical mass proxies from probabilistic memberships;Monthly Notices of the Royal Astronomical Society;2023-10-05

3. CALSAGOS: Clustering algorithms applied to galaxies in overdense systems;Monthly Notices of the Royal Astronomical Society;2022-12-22

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