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Found 6 papers, 2 papers with code
Super-Resolving Beyond Satellite Hardware Using Realistically Degraded Images
Modern deep Super-Resolution (SR) networks have established themselves as valuable techniques in image reconstruction and enhancement.
Cosmic Ray Extremely Distributed Observatory
The Cosmic Ray Extremely Distributed Observatory (CREDO) is a newly formed, global collaboration dedicated to observing and studying cosmic rays (CR) and cosmic ray ensembles (CRE): groups of a minimum of two CR with a common primary interaction vertex or the same parent particle.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics
Recognition and classification of the cosmic-ray events in images captured by CMOS/CCD cameras
Our method consists of analyzing the shape of traces present in images recorded by a camera sensor and metadata related to an image like camera model, GPS location of camera, vertical and horizontal orientation of a camera sensor, timestamp of image acquisition, and other events recognized near-by sensors.
Instrumentation and Methods for Astrophysics
Model dispersion with PRISM; an alternative to MCMC for rapid analysis of models
However, PRISM can additionally be used as a standalone alternative to MCMC for model analysis, providing insight into the behavior of complex scientific models.
Instrumentation and Methods for Astrophysics Computational Physics
The accretion history of dark matter halos III: A physical model for the concentration-mass relation
We present a semi-analytic, physically motivated model for dark matter halo concentration as a function of halo mass and redshift.
Cosmology and Nongalactic Astrophysics
The physics driving the cosmic star formation history
Galaxies form stars in a self-regulated fashion at a rate controlled by the balance between, on the one hand, feedback from massive stars and black holes and, on the other hand, gas cooling and accretion.
Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
