D. Physics

Euclid Preparation. TBD. Galaxy colour selections with Euclid and ground photometry for cluster weak-lensing analyses

Cea, Cosmology, Case Western Reserve University, 2023, 2311.16239.

The first power spectrum limit on the 21-cm signal of neutral hydrogen during the Cosmic Dawn at z = 20–25 from LOFAR

University College London, D. O. Astronomy, Max-Planck Institute for Astrophysics, 2018, Monthly Notices of the Royal Astronomical Society.

OGLE-2009-BLG-076S: THE MOST METAL-POOR DWARF STAR IN THE GALACTIC BULGE

D. Physics, Usa, D. Astronomy, 2009, 0906.2235.

Accurate spectra for high energy ions by advanced time-of-flight diamond-detector schemes in experiments with high energy and intensity lasers

University of Pisa, INFN-LNF, Universidade de Lisboa, 2020, Scientific Reports.

THREE-DIMENSIONAL STELLAR KINEMATICS AT THE GALACTIC CENTER: MEASURING THE NUCLEAR STAR CLUSTER SPATIAL DENSITY PROFILE, BLACK HOLE MASS, AND DISTANCE

Department of Physics, University of Toronto, Stockholm University, 2013, 1311.0886.

Temperature dependence of the magnon-phonon interaction in hybrids of high-overtone bulk acoustic resonators with ferromagnetic thin films

Erlangen, Bayerische Akademie der Wissenschaften, Physics Department, 2023, Physical Review Applied.

Generating synthetic star catalogs from simulated data for next-gen observatories with py-ananke

U. Pennsylvania, C. I. O. Technology., S. S. Institute, 2023, 2312.02268.

J-PLUS: The Javalambre Photometric Local Universe Survey

M. C. Díaz-Martín, J. L. Lamadrid, Pittsburgh, 2015, Astronomy & Astrophysics.

ALMA detection of the dusty object silhouetted against the S0 galaxy NGC 3269 in the Antlia cluster

Helsinki, Stockholm, U. Helsinki, 2020, Astronomy & Astrophysics.

THE RELATIONSHIP BETWEEN THE DUST AND GAS-PHASE CO ACROSS THE CALIFORNIA MOLECULAR CLOUD

Vienna, M. Lombardi, J. Alves, 2015, 1503.03564.