Characterizing the intracluster light over the redshift range 0.2 < z < 0.8 in the DES-ACT overlap

Author:

Golden-Marx Jesse B1ORCID,Zhang Y2,Ogando R L C3ORCID,Allam S4,Tucker D L4,Miller C J56ORCID,Hilton M78,Mutlu-Pakdil B9ORCID,Abbott T M C10,Aguena M11ORCID,Alves O6,Andrade-Oliveira F6,Annis J4,Bacon D12,Bertin E1314ORCID,Bocquet S15,Brooks D16,Burke D L1718,Carnero Rosell A191120ORCID,Carrasco Kind M2122ORCID,Castander F J2324,Conselice C2526,Costanzi M272829,da Costa L N11,Pereira M E S30,De Vicente J31ORCID,Desai S32,Doel P16,Everett S33,Ferrero I34ORCID,Flaugher B4,Frieman J49,García-Bellido J35ORCID,Gerdes D W56,Gruen D15ORCID,Gruendl R A2122,Gutierrez G4,Hinton S R36ORCID,Hollowood D L37ORCID,Honscheid K3839,James D J40,Kuehn K4142,Kuropatkin N4,Lahav O16,Marshall J L2,Melchior P43ORCID,Mena-Fernández J31,Miquel R4445,Mohr J J4615,Palmese A47ORCID,Paz-Chinchón F2148,Pieres A113ORCID,Plazas Malagón A A43ORCID,Prat J499ORCID,Raveri M50,Rodriguez-Monroy M31,Romer A K51,Sanchez E31,Scarpine V4,Sevilla-Noarbe I31,Sifón C52ORCID,Smith M53ORCID,Suchyta E54ORCID,Swanson M E C21,Tarle G6,Vincenzi M1253,Weaverdyck N655ORCID,Yanny B4,

Affiliation:

1. Department of Astronomy, Shanghai Jiao Tong University , Shanghai 200240, China

2. George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University , College Station, TX 77843, USA

3. Observatório Nacional , Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil

4. Fermi National Accelerator Laboratory , PO Box 500, Batavia, IL 60510, USA

5. Department of Astronomy, University of Michigan , Ann Arbor, MI 48109, USA

6. Department of Physics, University of Michigan , Ann Arbor, MI 48109, USA

7. Astrophysics Research Centre, University of KwaZulu-Natal , Durban 3696, South Africa

8. Wits Centre for Astrophysics, School of Physics, University of Witwatersrand , Private Bag 3, Johannesburg 2050, South Africa

9. Kavli Institute for Cosmological Physics, University of Chicago , Chicago, IL 60637, USA

10. Cerro Tololo Inter-American Observatory, NSF’s National Optical-Infrared Astronomy Research Laboratory , Casilla 603, La Serena, Chile

11. Laboratório Interinstitucional de e-Astronomia – LIneA , Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil

12. Institute of Cosmology and Gravitation, University of Portsmouth , Portsmouth PO1 3FX, UK

13. CNRS, UMR 7095, Institut d’Astrophysique de Paris , F-75014 Paris, France

14. Institut d’Astrophysique de Paris, Sorbonne Universités , UPMC Univ Paris 06, UMR 7095, F-75014 Paris, France

15. Faculty of Physics, Ludwig-Maximilians-Universität, University Observatory , Scheinerstr 1, D-81679 Munich, Germany

16. Department of Physics & Astronomy, University College London , Gower Street, London WC1E 6BT, UK

17. Kavli Institute for Particle Astrophysics & Cosmology , PO Box 2450, Stanford University, Stanford, CA 94305, USA

18. SLAC National Accelerator Laboratory , Menlo Park, CA 94025, USA

19. Instituto de Astrofisica de Canarias , E-38205 La Laguna, Tenerife, Spain

20. Departmento Astrofísica, Universidad de La Laguna , E-38206 La Laguna, Tenerife, Spain

21. Center for Astrophysical Surveys, National Center for Supercomputing Applications , 1205 West Clark St., Urbana, IL 61801, USA

22. Department of Astronomy, University of Illinois at Urbana-Champaign , 1002 W. Green Street, Urbana, IL 61801, USA

23. Institut d’Estudis Espacials de Catalunya (IEEC) , E-08034 Barcelona, Spain

24. Institute of Space Sciences (ICE, CSIC) , Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain

25. Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester , Oxford Road, Manchester M13 9PL, UK

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

27. Astronomy Unit, Department of Physics, University of Trieste , via Tiepolo 11, I-34131 Trieste, Italy

28. INAF – Osservatorio Astronomico di Trieste , via G. B. Tiepolo 11, I-34143 Trieste, Italy

29. Institute for Fundamental Physics of the Universe , Via Beirut 2, I-34014 Trieste, Italy

30. Hamburger Sternwarte, Universität Hamburg , Gojenbergsweg 112, D-21029 Hamburg, Germany

31. Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT) , E-28040 Madrid, Spain

32. Department of Physics, IIT Hyderabad , Kandi, Telangana 502285, India

33. Jet Propulsion Laboratory, California Institute of Technology , 4800 Oak Grove Dr., Pasadena, CA 91109, USA

34. Institute of Theoretical Astrophysics, University of Oslo , PO Box 1029 Blindern, NO-0315 Oslo, Norway

35. Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid , E-28049 Madrid, Spain

36. School of Mathematics and Physics, University of Queensland , Brisbane, QLD 4072, Australia

37. Santa Cruz Institute for Particle Physics , Santa Cruz, CA 95064, USA

38. Center for Cosmology and Astro-Particle Physics, The Ohio State University , Columbus, OH 43210, USA

39. Department of Physics, The Ohio State University , Columbus, OH 43210, USA

40. Center for Astrophysics | Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USA

41. Australian Astronomical Optics, Macquarie University , North Ryde, NSW 2113, Australia

42. Lowell Observatory , 1400 Mars Hill Rd, Flagstaff, AZ 86001, USA

43. Department of Astrophysical Sciences, Princeton University , Peyton Hall, Princeton, NJ 08544, USA

44. Institució Catalana de Recerca i Estudis Avançats , E-08010 Barcelona, Spain

45. Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology , Campus UAB, Bellaterra, E-08193 Barcelona, Spain

46. Max Planck Institute for Extraterrestrial Physics , Giessenbachstrasse, D-85748 Garching, Germany

47. Department of Astronomy, University of California , Berkeley, 501 Campbell Hall, Berkeley, CA 94720, USA

48. Institute of Astronomy, University of Cambridge , Madingley Road, Cambridge CB3 0HA, UK

49. Department of Astronomy and Astrophysics, University of Chicago , Chicago, IL 60637, USA

50. Department of Physics and Astronomy, University of Pennsylvania , Philadelphia, PA 19104, USA

51. Department of Physics and Astronomy, Pevensey Building, University of Sussex , Brighton BN1 9QH, UK

52. Instituto de Física, Pontificia Universidad Católica de Valparaíso , Casilla 4059, Valparaíso, Chile

53. School of Physics and Astronomy, University of Southampton , Southampton SO17 1BJ, UK

54. Computer Science and Mathematics Division , Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA

55. Lawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA

Abstract

ABSTRACT We characterize the properties and evolution of bright central galaxies (BCGs) and the surrounding intracluster light (ICL) in galaxy clusters identified in the Dark Energy Survey and Atacama Cosmology Telescope Survey (DES-ACT) overlapping regions, covering the redshift range 0.20 < z < 0.80. Over this redshift range, we measure no change in the ICL’s stellar content (between 50 and 300 kpc) in clusters with log10(M200m,SZ/M⊙) >14.4. We also measure the stellar mass–halo mass (SMHM) relation for the BCG+ICL system and find that the slope, β, which characterizes the dependence of M200m,SZ on the BCG+ICL stellar mass, increases with radius. The outskirts are more strongly correlated with the halo than the core, which supports that the BCG+ICL system follows a two-phase growth, where recent growth (z < 2) occurs beyond the BCG’s core. Additionally, we compare our observed SMHM relation results to the IllustrisTNG300-1 cosmological hydrodynamic simulations and find moderate qualitative agreement in the amount of diffuse light. However, the SMHM relation’s slope is steeper in TNG300-1 and the intrinsic scatter is lower, likely from the absence of projection effects in TNG300-1. Additionally, we find that the ICL exhibits a colour gradient such that the outskirts are bluer than the core. Moreover, for the lower halo mass clusters (log10(M200m,SZ/M⊙) < 14.59), we detect a modest change in the colour gradient’s slope with lookback time, which combined with the absence of stellar mass growth may suggest that lower mass clusters have been involved in growth via tidal stripping more recently than their higher mass counterparts.

Funder

National Science Foundation of China

U.S. Department of Energy

National Science Foundation

Science and Technology Facilities Council

Higher Education Funding Council for England

MICINN

European Research Council

CNPq

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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