The Resolved Near-Infrared Extragalactic Background

Abstract

We present a current best estimate of the integrated near-infrared (NIR) extragalactic background light (EBL) attributable to resolved galaxies in J, H, and Ks. Our results in units of nW m-2 sr-1 are 11.7+5.6 -2.6 in J, 11.5+4.5 -1.5 in H and 10.0+2.8 -0.8 in Ks. We derive these new limits by combining our deep wide-field NIR photometry from five widely separated fields with other studies from the literature to create a galaxy counts sample that is highly complete and has good counting statistics out to JHKs ~ 27-28. As part of this effort we present new ultradeep Ks-band galaxy counts from 22 hours of observations with the Multi Object Infrared Camera and Spectrograph (MOIRCS) instrument on the Subaru Telescope. We use this MOIRCS Ks-band mosaic to estimate the total missing flux from sources beyond our detection limits. Our new limits to the NIR EBL are in basic agreement with, but 10 - 20% higher than previous estimates, bringing them into better agreement with estimates of the total NIR EBL (resolved + unresolved sources) obtained from TeV gamma-ray opacity measurements and recent direct measurements of the total NIR EBL. We examine field to field variations in our photometry to show that the integrated light from galaxies is isotropic to within uncertainties, consistent with the expected large-scale isotropy of the EBL. Our data also allow for a robust estimate of the NIR light from Galactic stars, which we find to be 14.7 +/- 2.4 in J, 10.1 +/- 1.9 in H and 7.6 +/- 1.8 in Ks in units of nW m-2 sr-1.

Accepted to ApJ

References in corpus (32)

• The UKIRT Infrared Deep Sky Survey (UKIDSS)
• The Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging
• The Chandra Deep Field-North Survey. XIII. 2 Ms Point-Source Catalogs
• The Cosmic Infrared Background: Measurements and Implications
• The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: I. Limits and Detections
• A low level of extragalactic background light as revealed by gamma-rays from blazars
• Deep Galaxy Counts, Extragalactic Background Light, and the Stellar Baryon Budget
• The Chandra Deep Field North Survey. V. 1 Ms Source Catalogs
• A Highly Complete Spectroscopic Survey of the GOODS-N Field
• New limits on the density of the extragalactic background light in the optical to the far-infrared from the spectra of all known TeV blazars
• IRTS observation of the near-infrared extragalactic background light
• The Contribution of the First Stars to the Cosmic Infrared Background
• Infrared Emission from the Radio Supernebula in NGC 5253: A Proto-Globular Cluster?
• The Cosmic Infrared Background at 1.25 microns and 2.2 microns using DIRBE and 2MASS: a contribution not due to galaxies ?
• A Tentative Detection of the Cosmic Infrared Background at 3.5 microns from COBE/DIRBE Observations
• Cosmic Infrared Background and Early Galaxy Evolution
• Subaru Deep Survey I. Near-Infrared Observations
• Population III and the Near-Infrared Background Excess
• Diffuse Extragalactic Background Light versus Deep Galaxy Counts in the Subaru Deep Field: Missing Light in the Universe?
• DIRBE Minus 2MASS: Confirming the Cosmic Infrared Background at 2.2 Microns
• Constraints on the Cosmic Near Infrared Background Excess from NICMOS Deep Field Observations
• Ultradeep Near-Infrared Observations of GOODS 850-5
• DIRBE Minus 2MASS: Confirming the CIRB in 40 New Regions at 2.2 and 3.5 Microns
• The OPTX Project I: The Flux and Redshift Catalogs for the CLANS, CLASXS, and CDF-N fields
• The Chandra Large Area Synoptic X-ray Survey (CLASXS) of the Lockman Hole-Northwest: The X-ray Catalog
• An Optical Catalog of the Chandra Large Area Synoptic X-ray Survey Sources
• MOIRCS Deep Survey. I: DRG Number Counts
• Is There an Imprint of Primordial Stars in the Tev Gamma-Ray Spectrum of Blazars?
• Subaru Super Deep Field with Adaptive Optics I. Observations and First Implications
• Star Formation History and Other Properties of the Northern HDF
• An Extremely Deep Wide-Field Near-Infrared Survey: Bright Galaxy Counts and Local Large Scale Structure
• The OPTX Project III: X-ray versus Optical Spectral Type for AGNs

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