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Probing Intra-Halo Light with Galaxy Stacking in CIBER Images

Cheng, Yun-Ting and Arai, Toshiaki and Bangale, Priyadarshini and Bock, James J. and Chang, Tzu-Ching and Cooray, Asantha and Feder, Richard M. and Korngut, Phillip M. and Lee, Dae Hee and Liu, Lunjun and Matsumoto, Toshio and Matsuura, Shuji and Nguyen, Chi H. and Sano, Kei and Tsumura, Kohji and Zemcov, Michael (2021) Probing Intra-Halo Light with Galaxy Stacking in CIBER Images. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20210511-124440585

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Abstract

We study the stellar halos of 0.2 ≲ z ≲ 0.5 galaxies with stellar masses spanning M∗∼10^(10.5) to 10¹²M⊙ (approximately L∗ galaxies at this redshift) using imaging data from the Cosmic Infrared Background Experiment (CIBER). A previous CIBER fluctuation analysis suggested that intra-halo light (IHL) contributes a significant portion of the near-infrared extragalactic background light (EBL), the integrated emission from all sources throughout cosmic history. In this work, we carry out a stacking analysis with a sample of ∼30,000 Sloan Digital Sky Survey (SDSS) photometric galaxies from CIBER images in two near-infrared bands (1.1 and 1.8 μm) to directly probe the IHL associated with these galaxies. We stack galaxies in five sub-samples split by brightness, and detect an extended galaxy profile, beyond the instrument point spread function (PSF), derived by stacking stars. We jointly fit a model for the inherent galaxy light profile, plus large-scale one- and two-halo clustering to measure the extended galaxy IHL. We detect non-linear one-halo clustering in the 1.8 μm band, at a level consistent with numerical simulations. Our results on the galaxy profile suggest that ∼50% of the total galaxy light budget in our galaxy sample resides in the outskirts of the galaxies at r>10 kpc. We describe this extended emission as IHL and and are able to study how this fraction evolves with cosmic time. These results are new in the near-infrared wavelength at the L∗ mass scale, and suggest that IHL has a significant contribution to the integrated galactic light, and to the amplitude of large-scale background fluctuations.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/2103.03882arXivDiscussion Paper
ORCID:
AuthorORCID
Cheng, Yun-Ting0000-0002-5437-0504
Bock, James J.0000-0002-5710-5212
Chang, Tzu-Ching0000-0001-5929-4187
Cooray, Asantha0000-0002-3892-0190
Feder, Richard M.0000-0002-9330-8738
Matsumoto, Toshio0000-0001-6066-5221
Matsuura, Shuji0000-0002-5698-9634
Zemcov, Michael0000-0001-8253-1451
Additional Information:Attribution 4.0 International (CC BY 4.0). We thank the dedicated efforts of the sounding rocket Staff at NASA Wallops Flight Facility and White Sands Missile Range. This work was supported by NASA APRA research grants NNX07AI54G, NNG05WC18G, NNX07AG43G, NNX07AJ24G, NNX10AE12G, and 80NSSC20K0595. Initial support was provided by an award to J.B. from the Jet Propulsion Laboratory's Director's Research and Development Fund. Japanese participation in CIBER was supported by KAKENHI (20.34, 18204018, 19540250, 21340047, 21111004, 24111717, 26800112, and 15H05744) from Japan Society for the Promotion of Science (JSPS) and the Ministry of Education, Culture, Sports, Science and Technology (MEXT). Korean participation in CIBER was supported by the Pioneer Project from Korea Astronomy and Space Science Institute (KASI). Y.-T. C. acknowledges support by the Ministry of Education, Taiwan through the Taiwan-Caltech Scholarship. C. H. N. acknowledges support by NASA Headquarters under the NASA Earth and Space Science Fellowship Program - Grant 80NSSCK0706. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. The Pan-STARRS1 Surveys (PS1) and the PS1 public science archive have been made possible through contributions by the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max- Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, the Queen's University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation Grant No. AST-1238877, the University of Maryland, Eotvos Lorand University (ELTE), the Los Alamos National Laboratory, and the Gordon and Betty Moore Foundation. Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org. SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard- Smithsonian Center for Astrophysics, Instituto de Astrofisica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU) / University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut fur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatario Nacional / MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www. cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www. cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This work has made use of CosmoHub. CosmoHub has been developed by the Port d'Informacio Cientifca (PIC), maintained through a collaboration of the Institut de Fisica d'Altes Energies (IFAE) and the Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas (CIEMAT) and the Institute of Space Sciences (CSIC & IEEC), and was partially funded by the "Plan Estatal de Investigacion Cientifca y Tecnica y de Innovacion" program of the Spanish government. Software: astropy (Astropy Collaboration et al. 2013), emcee (Foreman-Mackey et al. 2013), corner (Foreman-Mackey 2016)
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
NASANNX07AI54G
NASANNG05WC18G
NASANNX07AG43G
NASANNX07AJ24G
NASANNX10AE12G
NASA80NSSC20K0595
JPL Research and Technology Development FundUNSPECIFIED
Japan Society for the Promotion of Science (JSPS)18204018
Japan Society for the Promotion of Science (JSPS)19540250
Japan Society for the Promotion of Science (JSPS)21340047
Japan Society for the Promotion of Science (JSPS)21111004
Japan Society for the Promotion of Science (JSPS)24111717
Japan Society for the Promotion of Science (JSPS)26800112
Japan Society for the Promotion of Science (JSPS)15H05744
Ministry of Education, Culture, Sports, Science and Technology (MEXT)UNSPECIFIED
Korea Astronomy and Space Science Institute (KASI)UNSPECIFIED
Ministry of Education (Taipei)UNSPECIFIED
NASA Earth and Space Science Fellowship80NSSCK0706
NASANNX08AR22G
NSFAST-1238877
University of MarylandUNSPECIFIED
Eotvos Lorand University (ELTE)UNSPECIFIED
Los Alamos National LaboratoryUNSPECIFIED
Gordon and Betty Moore FoundationUNSPECIFIED
Alfred P. Sloan FoundationUNSPECIFIED
Department of Energy (DOE)UNSPECIFIED
Participating InstitutionsUNSPECIFIED
Gaia Multilateral AgreementUNSPECIFIED
Subject Keywords:cosmology: observations; diffuse radiation; large-scale structure of universe
Record Number:CaltechAUTHORS:20210511-124440585
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210511-124440585
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:109082
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:11 May 2021 20:32
Last Modified:11 May 2021 20:32

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