Showing 61–80 of 282 results
/ Date/ Name
Oct 10, 2023Gaia Focused Product Release: Sources from Service Interface Function image analysis -- Half a million new sources in omega CentauriOct 10, 2023Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasarsOct 9, 2023Gaia Focused Product Release: Radial velocity time series of long-period variablesOct 6, 2023Measurement of the CKM angle $γ$ using the $B^{\pm}\rightarrow D^{*} h^{\pm}$ channelsOct 3, 2023Smart pixel sensors: towards on-sensor filtering of pixel clusters with deep learningSep 29, 2023Scintillation characteristics of the EJ-299-02H scintillatorSep 12, 2023Vortex Fiber Nulling for Exoplanet Observations: Implementation and First LightSep 11, 2023Measurement of the CKM angle $γ$ in the $B^0 \to DK^{*0}$ channel using self-conjugate $D \to K_S^0 h^+ h^-$ decaysAug 17, 2023Fundamental Neutron Physics: a White Paper on Progress and Prospects in the USJun 22, 2023Search for $CP$ violation in the phase space of $D^0 \to π^-π^+π^0$ decays with the energy testMay 30, 2023Keck/KPIC Emission Spectroscopy of WASP-33bMay 16, 2023Demonstration of Sub-micron UCN Position Resolution using Room-temperature CMOS SensorMar 29, 2023Impact of cross-section uncertainties on supernova neutrino spectral parameter fitting in the Deep Underground Neutrino ExperimentFeb 13, 2023GRANDMA and HXMT Observations of GRB 221009A -- the Standard-Luminosity Afterglow of a Hyper-Luminous Gamma-Ray BurstJan 10, 2023Detecting exomoons from radial velocity measurements of self-luminous planets: application to observations of HR 7672 B and future prospectsDec 19, 2022Highly-parallelized simulation of a pixelated LArTPC on a GPUNov 21, 2022Open charm production and asymmetry in $p$Ne collisions at $\sqrt{s_{\scriptscriptstyle\rm NN}} =$ 68.5 GeVNov 2, 2022Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detectorOct 12, 2022Nested Dust Shells around the Wolf-Rayet Binary WR 140 observed with JWSTSep 30, 2022Retrieving C and O Abundance of HR 8799 c by Combining High- and Low-Resolution Data