From the 2 of 36 papers with an AI index.
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- Ludwig-Maximilians-Universität MünchenDE22 papers
- University College LondonGB22 papers
- University of OsloNO22 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT21 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di NapoliIT21 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT21 papers
- Université Paris CitéFR21 papers
- Université Paris-SaclayFR21 papers
- University of BolognaIT21 papers
- University of BonnDE21 papers
- University of CopenhagenDK21 papers
- University of GenevaCH21 papers
36 papers
SATisfying the High School Identities but not Wilkie's Identity
Agon Hajdari, Johannes Niederhauser
We settle an open question related to Tarski's High School Algebra problem by showing that no 11-element algebra can satisfy the High School Identities while refuting Wilkie's iden…
Intermediate scattering function of Brownian particles in a tilted cosine potential
Regina Rusch, Thomas Franosch
We solve the Fokker-Planck equation for a Brownian particle in a tilted cosine potential and derive the intermediate scattering function (ISF), which captures the full spatio-tempo…
Discovery of the Bootis phenomenon in an early B-type star
J. Olbermann, P. Aschenbrenner, N. Przybilla
Chemically peculiar A-type stars of the Boo class are characterised by depletions of refractory elements and normal volatile species. Their formation channel(s) have not yet be…
Cepheid metallicities from low-resolution near-infrared spectra: validation against the optical reference scale
M. A. Urbaneja, R. P. Kudritzki, N. Przybilla
Classical Cepheid metallicities trace recent chemical enrichment and help assess systematics in Cepheid-based distance measurements. They are derived mainly from high-resolution op…
Euclid: Inferring star-formation history via cross-correlations of photometric clustering and shear with the cosmic infrared background
J. Han, S. Camera, M. Migliaccio +146
The cosmic infrared background, sourced by dust heated by star-forming activity, encodes the integrated history of the star-formation distribution over a large swathe of cosmic tim…
Euclid: Calibrating distances from surface brightness fluctuations with Early Release Observations of the Fornax cluster
R. Habas, M. Cantiello, G. Riccio +169
Surface brightness fluctuations (SBF), the pixel-to-pixel variations in flux that arise from the statistical distribution of stars in galaxy images, provide a powerful tool to meas…