output
20072024
most citedHeavy quarkonium: progress, puzzles, and opportunities

1.8k citations

Showing 2020Show all

18 papers · 1 filter

astro-ph.GA20205 cited

CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models

Patrick Simon, Stefan Hilbert

Galaxy models predict a tight relation between the clustering of galaxies and dark matter on cosmological scales, but predictions differ notably in the details. We used this opport…

astro-ph.GA2020

Identifying and Repairing Catastrophic Errors in Galaxy Properties Using Dimensionality Reduction

Beryl Hovis-Afflerbach, Charles L. Steinhardt, Daniel Masters +1

Our understanding of galaxy evolution is derived from large surveys designed to maximize efficiency by only observing the minimum amount needed to infer properties for a typical ga…

astro-ph.EP202047 cited

A highly non-Keplerian protoplanetary disc: Spiral structure in the gas disc of CQ Tau

Lisa Wölfer, Stefano Facchini, Nicolas T. Kurtovic +9

In the past years, high angular resolution observations have revealed that circumstellar discs appear in a variety of shapes with diverse substructures being ubiquitous. This has g…

nucl-th202050 cited

In-medium effects in strangeness production in heavy-ion collisions at (sub-)threshold energies

Taesoo Song, Laura Tolos, Joana Wirth +2

We study the in-medium effects in strangeness production in heavy-ion collisions at (sub-)\-threshold energies of 1 - 2 A GeV based on the microscopic Parton-Hadron-String Dynamics…

astro-ph.HE202013 cited

Exploration of Aspherical Ejecta Properties in Type Ia Supernova: Progenitor Dependence and Applications to Progenitor Classification

Shing-Chi Leung, Roland Diehl, Ken'ichi Nomoto +1

Several explosions of thermonuclear supernovae (SNe Ia) have been found to exhibit deviations from spherical symmetry upon closer inspection. Examples are the gamma-ray lines from…

astro-ph.SR20209 cited

Leveraging HST with MUSE: II. Na-abundance variations in intermediate age star clusters

S. Martocchia, S. Kamann, S. Saracino +13

Ancient (10 Gyr) globular clusters (GCs) show chemical abundance variations in the form of patterns among certain elements, e.g. N correlates with Na and anti-correlates with O.…