Modeling the Extragalactic Background Light and the Cosmic Star Formation History (data)

  1. Finke, Justin D. 1
  2. Ajello, Marco 2
  3. Dominguez, Alberto 3
  4. Desai, Abhishek 4
  5. Hartmann, Dieter H. 2
  6. Paliya, Vaidehi S. 5
  7. Saldana-Lopez, Alberto 6
  1. 1 United States Naval Research Laboratory
    info

    United States Naval Research Laboratory

    Washington, Estados Unidos

    ROR https://ror.org/04d23a975

  2. 2 Clemson University
    info

    Clemson University

    Clemson, Estados Unidos

    ROR https://ror.org/037s24f05

  3. 3 Universidad Complutense de Madrid
    info

    Universidad Complutense de Madrid

    Madrid, España

    ROR 02p0gd045

  4. 4 University of Wisconsin–Madison
    info

    University of Wisconsin–Madison

    Madison, Estados Unidos

    ROR https://ror.org/01y2jtd41

  5. 5 Inter-University Centre for Astronomy and Astrophysics
    info

    Inter-University Centre for Astronomy and Astrophysics

    Pune, India

    ROR https://ror.org/04etcj997

  6. 6 Université de Genève
    info

    Université de Genève

    Ginebra, Suiza

    ROR https://ror.org/01swzsf04

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Editor: Zenodo

Año de publicación: 2022

Tipo: Dataset

CC BY 4.0

DOI: 10.5281/ZENODO.7023072 lock_openAcceso abierto editor

Resumen

Paper: Modeling the Extragalactic Background Light and the Cosmic Star Formation History Authors: Justin D. Finke, Marco Ajello, Alberto Dominguez, Abhishek Desai, Dieter H. Hartmann, Vaidehi S. Paliya, Alberto Saldana-Lopez Description: These are the luminosity densities, EBL energy density/intensities, and gamma-ray absorption optical depths for "Model A" from this publication. Contents: lumdens.tar.gz: The model luminosity density, with redshift given in the title of the file. Each file contains the wavelength in microns, and the luminosity density in Watts/Mpc^3. EBL_energydensity.tar.gz: The model EBL energy density, with redshift given in the name of the file. Each file contains the photon energy in eV, and the energy density in erg/cm^3. EBL_intensity.tar.gz: The model EBL intensity, with redshift given in the name of the file. Each file contains the wavelength in angstroms, and the intensity in nW/(m^2 srad). tau.tar.gz: The model gamma-gamma absorption optical depths, with redshift given in the name of the file. Each file contains the photon energy in TeV, and the absorption optical depth. Distribution Statement A. Approved for public release. Distribution is unlimited.<br>