115 citations · 398 across the 9 of their papers we have counts for
9 papers
Cosmic Infrared Background Fluctuations and Zodiacal Light
Richard G. Arendt, A. Kashlinsky, S. H. Moseley +1
We have performed a specific observational test to measure the effect that the zodiacal light can have on measurements of the spatial fluctuations of the near-IR background. Previo…
Reconstructing emission from pre-reionization sources with cosmic infrared background fluctuation measurements by the JWST
A. Kashlinsky, J. C. Mather, K. Helgason +3
We present new methodology to use cosmic infrared background (CIB) fluctuations to probe sources at 10<z<30 from a JWST/NIRCam configuration that will isolate known galaxies to 28…
Cross-correlating cosmic IR and X-ray background fluctuations: evidence of significant black hole populations among the CIB sources
N. Cappelluti, A. Kashlinsky, R. G. Arendt +7
In order to understand the nature of the sources producing the recently uncovered cosmic infrared background (CIB) fluctuations, we study cross-correlations between the fluctuation…
New measurements of the cosmic infrared background fluctuations in deep Spitzer/IRAC survey data and their cosmological implications
A. Kashlinsky, R. G. Arendt, M. L. N. Ashby +3
We extend previous measurements of cosmic infrared background (CIB) fluctuations to ~ 1 deg using new data from the Spitzer Extended Deep Survey. Two fields, with depths of ~12 hr/…
Cosmic Infrared Background Fluctuations in Deep Spitzer IRAC Images: Data Processing and Analysis
R. G. Arendt, A. Kashlinsky, S. H. Moseley +1
This paper provides a detailed description of the data reduction and analysis procedures that have been employed in our previous studies of spatial fluctuation of the cosmic infrar…
On the nature of the sources of the cosmic infrared background
A. Kashlinsky, R. G. Arendt, J. Mather +1
We discuss interpretation of the cosmic infrared background (CIB) anisotropies detected by us recently in the Spitzer IRAC based measurements. The fluctuations are approximately is…