The Contribution of Galaxies to the $3.4\,\mathrm{\mu m}$ Cosmic Infrared Background as Measured Using WISE
@article{Lake2019TheCO, title={The Contribution of Galaxies to the \$3.4\,\mathrm\{\mu m\}\$ Cosmic Infrared Background as Measured Using WISE}, author={S. E. Lake and E. Wright and R. J. Assef and T. Jarrett and S. Petty and S. Stanford and C. Tsai}, journal={arXiv: Astrophysics of Galaxies}, year={2019} }
The study of the extragalactic background light (EBL) in the optical and near infrared has received a lot of attention in the last decade, especially near a wavelength of $\lambda\approx 3.4\operatorname{\mu m}$, with remaining tension among different techniques for estimating the background. In this paper we present a measurement of the contribution of galaxies to the EBL at $3.4\operatorname{\mu m}$ that is based on the measurement of the luminosity function (LF) in Lake et al. (2018) and the… CONTINUE READING
Figures and Tables from this paper
Paper Mentions
References
SHOWING 1-10 OF 36 REFERENCES
The 2.4 μm Galaxy Luminosity Function as Measured Using WISE. III. Measurement Results
- Physics
- 2018
- 4
- PDF
The 2.4 $\mu$m Galaxy Luminosity Function as Measured Using WISE. I. Measurement Techniques
- Physics
- 2017
- 6
- PDF
Tentative Detection of the Cosmic Infrared Background at 2.2 and 3.5 Microns Using Ground-based and Space-based Observations
- Physics
- 1999
- 152
- PDF
The Cosmic Infrared Background at 1.25 and 2.2 Microns Using DIRBE and 2MASS: A Contribution Not Due to Galaxies?
- Physics
- 2001
- 133
- PDF
Detection of the Cosmic Infrared Background at 2.2 and 3.5 Microns Using DIRBE Observations
- Physics
- 2000
- 104
- PDF
$K$-corrections: an Examination of their Contribution to the Uncertainty of Luminosity Measurements
- Physics
- 2016
- 3
- PDF