activity
20172019
most citedA GeV-TeV Measurement of the Extragalactic Background Light

54 citations · 133 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.CO20193 cited

Populations behind the source-subtracted cosmic infrared background anisotropies

A. Kashlinsky, R. G. Arendt, M. Ashby +27

While the upcoming telescopes will reveal correspondingly fainter, more distant galaxies, a question will persist: what more is there that these telescopes cannot see? One answer i…

astro-ph.HE201954 cited

A GeV-TeV Measurement of the Extragalactic Background Light

Abhishek Desai, Kári Helgason, Marco Ajello +4

The Extragalactic Background Light (EBL) can be probed via the absorption imprint it leaves in the spectra of gamma-ray sources (). We recently developed a de…

astro-ph.CO2019

A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light -ray attenuation

Alberto Domínguez, Radoslaw Wojtak, Justin Finke +7

The Hubble constant and matter density of the Universe are measured using the latest -ray attenuation results from Fermi-LAT and Cherenkov telescopes. This metho…

astro-ph.CO201820 cited

Probing the cross-power of unresolved cosmic infrared and X-ray backgrounds with upcoming space missions

A. Kashlinsky, R. G. Arendt, N. Cappelluti +4

The source-subtracted cosmic infrared background (CIB) fluctuations uncovered in deep Spitzer data cannot be explained by known galaxy populations and appear strongly coherent with…

astro-ph.GA2018

The SPLASH and Chandra COSMOS Legacy Survey: the Cross Power Between Near-Infrared and X-Ray Background Fluctuations

Yanxia Li, Nico Cappelluti, Richard G. Arendt +3

We study the source-subtracted near-infrared and X-ray background fluctuations of the COSMOS field using data from the Spitzer SPLASH program (1272 hours) and Chandra COSMOS…

astro-ph.CO2018

X-ray background and its correlation with the 21 cm signal

Q. Ma, B. Ciardi, M. B. Eide +1

We use high resolution hydrodynamical simulations to study the contribution to the X-ray background from high- energetic sources, such as X-ray binaries, accreting nuclear black…