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Search for photons above 1019eV with the surface detector of the Pierre Auger Observatory

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F23%3A00577871" target="_blank" >RIV/68378271:_____/23:00577871 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/23:10475996 RIV/61989592:15310/23:73620316

  • Result on the web

    <a href="https://hdl.handle.net/11104/0346968" target="_blank" >https://hdl.handle.net/11104/0346968</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/1475-7516/2023/05/021" target="_blank" >10.1088/1475-7516/2023/05/021</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Search for photons above 1019eV with the surface detector of the Pierre Auger Observatory

  • Original language description

    We use the surface detector of the Pierre Auger Observatory to search for air showers initiated by photons with an energy above 1019 eV. Photons in the zenith angle range from 30 & DEG, to 60 & DEG, can be identified in the overwhelming background of showers initiated by charged cosmic rays through the broader time structure of the signals induced in the water Cherenkov detectors of the array and the steeper lateral distribution of shower particles reaching ground. Applying the search method to data collected between January 2004 and June 2020, upper limits at 95% CL are set to an E-2 diffuse flux of ultra-high energy photons above 1019 eV, 2x1019 eV and 4x1019 eV amounting to 2.11x10-3, 3.12x10-4 and 1.72x10-4 km-2 sr-1 yr-1, respectively. While the sensitivity of the present search around 2 x 1019 eV approaches expectations of cosmogenic photon fluxes in the case of a pure-proton composition, it is one order of magnitude above those from more realistic mixed-composition models.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2023

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Journal of Cosmology and Astroparticle Physics

  • ISSN

    1475-7516

  • e-ISSN

    1475-7516

  • Volume of the periodical

    2023

  • Issue of the periodical within the volume

    5

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    26

  • Pages from-to

    021

  • UT code for WoS article

    001038638500010

  • EID of the result in the Scopus database

    2-s2.0-85159475261