MEASUREMENTS OF DIFFUSE SKY EMISSION COMPONENTS IN HIGH GALACTIC LATITUDES AT 3.5 AND 4.9 μm USING DIRBE AND WISE DATA

Using all-sky maps obtained from the Cosmic Background Explorer/Diffuse Infrared Background Experiment (DIRBE) at 3.5 and 4.9 mu m, we present a reanalysis of diffuse sky emissions such as zodiacal light (ZL), diffuse Galactic light (DGL), integrated starlight (ISL), and isotropic residual emission...

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Bibliographic Details
Published in:The Astrophysical journal 2016-02, Vol.818 (1), p.72
Main Authors: Sano, K, Kawara, K, Matsuura, S, Kataza, H, Arai, T, Matsuoka, Y
Format: Article
Language:English
Subjects:
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
BACKGROUND RADIATION
COMPARATIVE EVALUATIONS
COSMIC DUST
COSMOLOGY
DISTRIBUTION
Dust
EMISSION
Emission analysis
Estimates
GALAXIES
Latitude
MASS
Near infrared radiation
Polyallylamine hydrochloride
POLYCYCLIC AROMATIC HYDROCARBONS
SILICATES
Sky
SPECTRA
STARS
ZODIACAL LIGHT
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Summary:Using all-sky maps obtained from the Cosmic Background Explorer/Diffuse Infrared Background Experiment (DIRBE) at 3.5 and 4.9 mu m, we present a reanalysis of diffuse sky emissions such as zodiacal light (ZL), diffuse Galactic light (DGL), integrated starlight (ISL), and isotropic residual emission including the extragalactic background light (EBL). Our new analysis, which includes an improved estimate of ISL using the Wide-field Infrared Survey Explorer data, enabled us to find the DGL signal in a direct linear correlation between diffuse near-infrared and 100 mu m emission at high Galactic latitudes (b> 35[degrees]). At 3.5 mu m, the high-latitude DGL result is comparable to the low-latitude value derived from the previous DIRBE analysis. In comparison with models of the DGL spectrum assuming a size distribution of dust grains composed of amorphous silicate, graphite, and polycyclic aromatic hydrocarbon (PAH), the measured DGL values at 3.5 and 4.9 mu m constrain the mass fraction of PAH particles in the total dust species to be more than ~2%. This was consistent with the results of Spitzer/IRAC toward the lower Galactic latitude regions. The derived residual emission of 8.9 + or - 3.4 nWm super(-2) sr super(-1) at 3.5 mu m is marginally consistent with the level of integrated galaxy light and the EBL constraints from the gamma -ray observations. The residual emission at 4.9 mu m is not significantly detected due to the large uncertainty in the ZL subtraction, the same as in previous studies. Combined with our reanalysis of the DIRBE data at 1.25 and 2.2 mu m, the residual emission in the near-infrared exhibits the Rayleigh-Jeans spectrum.
ISSN:0004-637X
1538-4357
DOI:10.3847/0004-637X/818/1/72