Large angular scale fluctuations of near-infrared extragalactic background light based on the IRTS observations
Open Access
- 10 July 2019
- journal article
- research article
- Published by Oxford University Press (OUP) in Publications of the Astronomical Society of Japan
- Vol. 71 (4)
- https://doi.org/10.1093/pasj/psz063
Abstract
We measure the spatial fluctuations of the Near-Infrared Extragalactic Background Light (NIREBL) from 2° to 20° in angular scale at the 1.6 and |$2.2\, \mu \mathrm{m}$| using data obtained with Near-Infrared Spectrometer (NIRS) on board the Infrared Telescope in Space (IRTS). The brightness of the NIREBL is estimated by subtracting foreground components such as zodiacal light, diffuse Galactic light, and integrated star light from the observed sky. The foreground components are estimated using well-established models and archive data. The NIREBL fluctuations for the 1.6 and |$2.2\, \mu \mathrm{m}$| connect well toward the sub-degree scale measurements from previous studies. Overall, the fluctuations show a wide bump with a center at around 1° and the power decreases toward larger angular scales with nearly a single power-law spectrum (i.e., |${F[\sqrt{l(l+1)C_l/2\pi }]} \sim \theta ^{-1}]$|, indicating that the large-scale power is dominated by the random spatial distribution of the sources. After examining several known sources, contributors such as normal galaxies, high-redshift objects, intra-halo light, and far-IR cosmic background, we conclude that the excess fluctuation at around the 1° scale cannot be explained by any of them.Keywords
Funding Information
- Ministry of Education (2011-0007760)
- NRF (2012R1A4A1028713)
- JSPS (17K18789, 18KK0089)
- National Research Foundation of Korea
- Ministry of Science and ICT (NRF-2018M1A3A3A02065645)
- University of Massachusetts
- California Institute of Technology
- NASA
- NSF
- ESA
This publication has 56 references indexed in Scilit:
- MEASUREMENTS OF THE MEAN DIFFUSE GALACTIC LIGHT SPECTRUM IN THE 0.95–1.65μm BAND FROM CIBERThe Astrophysical Journal, 2015
- Near-infrared background anisotropies from diffuse intrahalo light of galaxiesNature, 2012
- THE NEAR-INFRARED BACKGROUND INTENSITY AND ANISOTROPIES DURING THE EPOCH OF REIONIZATIONThe Astrophysical Journal, 2012
- THE SPECTRUM OF THE DIFFUSE GALACTIC LIGHT: THE MILKY WAY IN SCATTERED LIGHTThe Astrophysical Journal, 2011
- The Optical Extragalactic Background Light: Revisions and Further CommentsThe Astrophysical Journal, 2007
- Fast estimation of polarization power spectra using correlation functionsMonthly Notices of the Royal Astronomical Society, 2004
- Spectral Irradiance Calibration in the Infrared. XIV. The Absolute Calibration of 2MASSThe Astronomical Journal, 2003
- Representations of celestial coordinates in FITSAstronomy & Astrophysics, 2002
- The Cosmic Infrared Background at 1.25 and 2.2 Microns Using DIRBE and 2MASS: A Contribution Not Due to Galaxies?The Astrophysical Journal, 2001
- Estimating the power spectrum of the cosmic microwave backgroundPhysical Review D, 1998