Showing 81–100 of 331 results
/ Date/ Name
Nov 24, 2023The Power Board of the KM3NeT Digital Optical Module: design, upgrade, and productionNov 8, 2023TESS photometry of the nova eruption in V606 Vul: asymmetric photosphere and multiple ejections?Nov 7, 2023The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5Nov 7, 2023Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeTOct 30, 2023Introducing instance label correlation in multiple instance learning. Application to cancer detection on histopathological imagesOct 27, 2023Physical properties of Centaur (60558) 174P/Echeclus from stellar occultationsOct 20, 2023A hot mini-Neptune and a temperate, highly eccentric sub-Saturn around the bright K-dwarf TOI-2134Sep 18, 2023TESS Spots a Super-Puff: The Remarkably Low Density of TOI-1420bSep 12, 2023Mass ratio of single-line spectroscopic binaries with visual orbits using Bayesian inference and suitable priorsSep 6, 2023Prospects for combined analyses of hadronic emission from $γ$-ray sources in the Milky Way with CTA and KM3NeTAug 21, 20233D Correlations in the Lyman-$α$ Forest from Early DESI DataAug 15, 2023A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS$_4$ measured from stellar occultationsAug 7, 2023Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and VirgoJul 28, 2023A search for new physics in low-energy electron recoils from the first LZ exposureJul 2, 2023Decay widths and mass spectra of single bottom baryonsJun 9, 2023Optimal 1D Ly$α$ Forest Power Spectrum Estimation -- III. DESI early dataJun 9, 2023The Lyman-$α$ forest catalog from the Dark Energy Spectroscopic Instrument Early Data ReleaseJun 9, 2023The Early Data Release of the Dark Energy Spectroscopic InstrumentJun 9, 2023Validation of the Scientific Program for the Dark Energy Spectroscopic InstrumentMay 9, 2023Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case Studies