Showing 21–40 of 67 results
/ Date/ Name
Aug 19, 2019Absence of a thick atmosphere on the terrestrial exoplanet LHS 3844bAug 16, 2019S and VV Corona Australis: Spectroscopic Variability in Two Young Binary Star SystemsFeb 14, 2019Visual Orbits of Spectroscopic Binaries with the CHARA Array. I. HD 224355May 8, 2018Particle identification studies with a full-size 4-GEM prototype for the ALICE TPC upgradeApr 13, 2018Highly Volcanic Exoplanets, Lava Worlds, and Magma Ocean Worlds: An Emerging Class of Dynamic Exoplanets of Significant Scientific PriorityApr 13, 2018Exoplanet Science Priorities from the Perspective of Internal and Surface Processes for Silicate and Ice Dominated WorldsMar 7, 2017Asymmetries on red giant branch surfaces from CHARA/MIRC optical interferometryFeb 3, 2017Measurements of $e^+e^-$ pairs from open heavy flavor in $p$+$p$ and $d$+$A$ collisions at $\sqrt{s_{NN}}=200$ GeVJan 14, 2016Surface Albedo and Spectral Variability of CeresSep 25, 2015Azimuthally anisotropic emission of low-momentum direct photons in Au$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeVSep 15, 2015Dielectron production in Au$+$Au collisions at $\sqrt{s_{NN}}$=200 GeVSep 15, 2015Centrality-dependent modification of jet-production rates in deuteron-gold collisions at $\sqrt{s_{NN}}$=200 GeVJul 22, 2015Measurements of elliptic and triangular flow in high-multiplicity $^{3}$He$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeVJun 26, 2015$φ$ meson production in $d$$+$Au collisions at $\sqrt{s_{_{NN}}}=200$ GeVApr 20, 2015Systematic study of charged-pion and kaon femtoscopy in Au$+$Au collisions at $\sqrt{s_{_{NN}}}$=200 GeVSep 2, 2014Search for dark photons from neutral meson decays in $p$$+$$p$ and $d$$+$Au collisions at $\sqrt{s_{_{NN}}}$=200 GeVJul 28, 2014The SAMI Galaxy Survey: instrument specification and target selectionJul 22, 2014The SAMI Galaxy Survey: Early Data ReleaseMay 16, 2014Low-mass vector-meson production at forward rapidity in $p$$+$$p$ collisions at $\sqrt{s}=200$ GeVMay 14, 2014Measurement of $K_S^0$ and $K^{*0}$ in $p$$+$$p$, $d$$+$Au, and Cu$+$Cu collisions at $\sqrt{s_{_{NN}}}=200$ GeV