Ana Martina Botti

First Direct-Detection Results on Sub-GeV Dark Matter Using the SENSEI Detector at SNOLAB

SENSEI at SNOLAB: Single-Electron Event Rate and Implications for Dark Matter

Search by the SENSEI Experiment for Millicharged Particles Produced in the NuMI Beam

Confirmation of the spectral excess in DAMIC at SNOLAB with skipper CCDs

Single-Quantum Measurement With a Multiple-Amplifier Sensing Charge-Coupled Device

Searching for millicharged particles with 1 kg of Skipper-CCDs using the NuMI beam at Fermilab

Limits to Gauge Coupling in the Dark Sector Set by the Nonobservation of Instanton-Induced Decay of Super-Heavy Dark Matter in the Pierre Auger Observatory Data

Cosmological implications of photon-flux upper limits at ultrahigh energies in scenarios of Planckian-interacting massive particles for dark matter

Skipper-CCD sensors for the Oscura experiment: requirements and preliminary tests

EXCESS workshop: Descriptions of rising low-energy spectra

Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

SENSEI: Characterization of Single-Electron Events Using a Skipper Charge-Coupled Device

A Search for Photons with Energies Above 2 × 10¹⁷ eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory

Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory

The energy spectrum of cosmic rays beyond the turn-down around $$\varvec{10^{17}}$$ eV as measured with the surface detector of the Pierre Auger Observatory

Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory

Deep-learning based reconstruction of the shower maximum X$_{max}$ using the water-Cherenkov detectors of the Pierre Auger Observatory

Extraction of the muon signals recorded with the surface detector of the Pierre Auger Observatory using recurrent neural networks

Measurement of the cosmic-ray energy spectrum above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>18</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math>using the Pierre Auger Observatory

Features of the Energy Spectrum of Cosmic Rays above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>18</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> Using the Pierre Auger Observatory

Cosmic-Ray Anisotropies in Right Ascension Measured by the Pierre Auger Observatory

Direct measurement of the muonic content of extensive air showers between $$\mathbf { 2\times 10^{17}}$$ and $$\mathbf {2\times 10^{18}}~$$eV at the Pierre Auger Observatory

A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory

Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray Sources^*

Large-scale Cosmic-Ray Anisotropies above 4 EeV Measured by the Pierre Auger Observatory

Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory

Observation of a large-scale anisotropy in the arrival directions of cosmic rays above 8 × 10 ¹⁸ eV

Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory

Inferences on mass composition and tests of hadronic interactions from 0.3 to 100 EeV using the water-Cherenkov detectors of the Pierre Auger Observatory