{ "id": "1903.03126", "version": "v1", "published": "2019-03-07T19:04:56.000Z", "updated": "2019-03-07T19:04:56.000Z", "title": "A GeV-TeV Measurement of the Extragalactic Background Light", "authors": [ "Abhishek Desai", "Kári Helgason", "Marco Ajello", "Vaidehi Paliya", "Alberto Domínguez", "Justin Finke", "Dieter H. Hartmann" ], "categories": [ "astro-ph.HE" ], "abstract": "The Extragalactic Background Light (EBL) can be probed via the absorption imprint it leaves in the spectra of gamma-ray sources ($\\gamma\\gamma \\rightarrow e^-e^+$). We recently developed a dedicated technique to reconstruct the EBL, and its evolution with redshift, from $\\gamma$ ray optical depth data using a large sample of blazars detected by the {\\it Fermi} Large Area Telescope. Here, we extend this dataset to the TeV regime using ground-based Cherenkov observations of 38 blazars and report the first homogeneous measurement of the EBL spectral intensity covering the ultraviolet to infrared wavelengths ($\\sim$0.1-100$\\mathrm{\\mu m}$). A minimal EBL throughout the wavelength range with respect to integrated galaxy light is found, allowing little additional unresolved emission from faint or truly diffuse populations setting an upper limit of $\\lesssim 4~{\\rm nW\\cdot m^{-2}sr^{-1}}$ at 1.4\\,${\\rm \\mu m}$. In particular, the cosmic optical background (COB) at $z=0$ is found to be $27.8_{-2.0}^{+2.1}~{\\rm nW\\cdot m^{-2}sr^{-1}}$. This work lays the foundation for accurate gamma-ray measurements of the EBL across its whole spectral range using a combination of GeV and TeV data.", "revisions": [ { "version": "v1", "updated": "2019-03-07T19:04:56.000Z" } ], "analyses": { "keywords": [ "extragalactic background light", "gev-tev measurement", "accurate gamma-ray measurements", "little additional unresolved emission", "ray optical depth data" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }