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On the origin of near-infrared extragalactic background light anisotropy

Zemcov, Michael and Smidt, Joseph and Arai, Toshiaki and Bock, James and Cooray, Asantha and Gong, Yan and Kim, Min Gyu and Korngut, Phillip and Lam, Anson and Lee, Dae Hee and Matsumoto, Toshio and Matsuura, Shuji and Nam, Uk Won and Roudier, Gael and Tsumura, Kohji and Wada, Takehiko (2014) On the origin of near-infrared extragalactic background light anisotropy. Science, 346 (6210). pp. 732-735. ISSN 0036-8075. doi:10.1126/science.1258168. https://resolver.caltech.edu/CaltechAUTHORS:20141106-112913256

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Abstract

Extragalactic background light (EBL) anisotropy traces variations in the total production of photons over cosmic history and may contain faint, extended components missed in galaxy point-source surveys. Infrared EBL fluctuations have been attributed to primordial galaxies and black holes at the epoch of reionization (EOR) or, alternately, intrahalo light (IHL) from stars tidally stripped from their parent galaxies at low redshift. We report new EBL anisotropy measurements from a specialized sounding rocket experiment at 1.1 and 1.6 micrometers. The observed fluctuations exceed the amplitude from known galaxy populations, are inconsistent with EOR galaxies and black holes, and are largely explained by IHL emission. The measured fluctuations are associated with an EBL intensity that is comparable to the background from known galaxies measured through number counts and therefore a substantial contribution to the energy contained in photons in the cosmos.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1126/science.1258168DOIArticle
http://www.sciencemag.org/content/346/6210/732.abstractPublisherArticle
http://www.sciencemag.org/content/346/6210/732/suppl/DC1PublisherSupplemental Material
http://dx.doi.org/10.1126/science.aac9468 ErrataErratum
http://www.sciencemag.org/content/349/6244/aac9468ErrataErratum
ORCID:
AuthorORCID
Zemcov, Michael0000-0001-8253-1451
Bock, James0000-0002-5710-5212
Cooray, Asantha0000-0002-3892-0190
Matsumoto, Toshio0000-0001-6066-5221
Matsuura, Shuji0000-0002-5698-9634
Additional Information:© 2014 American Association for the Advancement of Science. 1 July 2014; accepted 3 October 2014. Our thanks to O. Doré, J. Filippini, and K. Ganga for useful conversations and comments throughout the course of this work and K. Helgason for kindly providing models of the statistics of the near-infrared CIB. The authors acknowledge the excellent support from the NASA sounding rockets program that was essential in developing, testing, qualifying, launching, and recovering our payloads. The CIBER auto- and cross-power spectra are available for public download at http://ciber.caltech.edu/zemcovetal. This work was supported by NASA APRA research grants NNX07AI54G, NNG05WC18G, NNX07AG43G, NNX07AJ24G, and NNX10AE12G. 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, and 21111004) 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). M.Z. and P.K. acknowledge support from NASA Postdoctoral Program fellowships, A.C. acknowledges support from an NSF CAREER award AST-0645427 and NSF AST-1313319, and K.T. acknowledges support from the JSPS Research Fellowship for Young Scientists. This publication makes use of data products from the Two Micron All Sky Survey (2MASS), 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. This work made use of images and/or data products provided by the National Optical Astronomy Observatory (NOAO) Deep Wide-Field Survey (NDWFS), which is supported by NOAO, operated by AURA, Inc., under a cooperative agreement with the National Science Foundation.
Funders:
Funding AgencyGrant Number
NASANNX07A154G
NASANNG05WC18G
NASANNX07AG43G
NASANNX07AJ24G
NASANNX10AE12G
JPL Research and Technology Development FundUNSPECIFIED
Japan Society for the Promotion of Science (JSPS)UNSPECIFIED
Ministry of Education, Culture, Sports, Science and Technology (MEXT)UNSPECIFIED
Korea Astronomy and Space Science Institute (KASI)UNSPECIFIED
NSFAST-0645427
NSFAST-1313319
Issue or Number:6210
DOI:10.1126/science.1258168
Record Number:CaltechAUTHORS:20141106-112913256
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20141106-112913256
Official Citation:On the origin of near-infrared extragalactic background light anisotropy Michael Zemcov, Joseph Smidt, Toshiaki Arai, James Bock, Asantha Cooray, Yan Gong, Min Gyu Kim, Phillip Korngut, Anson Lam, Dae Hee Lee, Toshio Matsumoto, Shuji Matsuura, Uk Won Nam, Gael Roudier, Kohji Tsumura, and Takehiko Wada Science 7 November 2014: 346 (6210), 732-735. [DOI:10.1126/science.1258168]
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:51370
Collection:CaltechAUTHORS
Deposited By:INVALID USER
Deposited On:06 Nov 2014 19:47
Last Modified:10 Nov 2021 19:09

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