Asosiy kontentga oʻtish
AkademIndex

Mahsulotlar

Ishlab chiquvchilar uchun

AkademBaseEkotizim uchun ochiq API

A. Bueno

5 ta ish

Granada U., Theor. Phys. Astrophys

  1. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory

    Adila Abdul Halim, P. Abreu, M. Aglietta +97

    MaqolaAstrophysics and Cosmic PhenomenaThe Astrophysical Journal20241 iqtibos
    ABI

  2. Search for photons above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>18</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory

    Adila Abdul Halim, P. Abreu, M. Aglietta +97

    MaqolaAstrophysics and Cosmic PhenomenaPhysical review. D/Physical review. D.20240 iqtibos
    ABI

  3. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory

    Adila Abdul Halim, P. Abreu, M. Aglietta +96

    MaqolaDark Matter and Cosmic PhenomenaPhysical review. D/Physical review. D.20240 iqtibos
    ABI

  4. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory

    Adila Abdul Halim, P. Abreu, M. Aglietta +96

    MaqolaAstrophysics and Cosmic PhenomenaPhysical Review Letters20250 iqtibos
    ABI

  5. Energy Spectrum of Ultrahigh-Energy Cosmic Rays across Declinations <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mo>−</mml:mo> <mml:mn>9</mml:mn> <mml:mn>0</mml:mn> <mml:mi>°</mml:mi> </mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mo>+</mml:mo> <mml:mn>44.8</mml:mn> <mml:mi>°</mml:mi> </mml:math> as Measured at the Pierre Auger Observatory

    Adila Abdul Halim, P. Abreu, M. Aglietta +96

    MaqolaAstrophysics and Cosmic PhenomenaPhysical Review Letters20250 iqtibos
    ABI