3 papers
astro-ph.IM2025
Validation of optical pathlength stability in a LISA test-bench demonstrator
Shivani Harer, Maxime Vincent, Hubert Halloin +40
The Laser Interferometer Space Antenna (LISA) observatory is a future L3 mission of the European Space Agency (ESA) to detect gravitational waves, set to launch in 2035. The detect…
physics.ins-det2025
Euclid: Methodology for derivation of IPC-corrected conversion gain of nonlinear CMOS APS
J. Le Graet, A. Secroun, M. Tourneur-Silvain +121
We introduce a fast method to measure the conversion gain in Complementary Metal-Oxide-Semiconductors (CMOS) Active Pixel Sensors (APS), which accounts for nonlinearity and interpi…
astro-ph.CO2025
Inferring astrophysics and cosmology with individual compact binary coalescences and their gravitational-wave stochastic background
S. Ferraiuolo, S. Mastrogiovanni, S. Escoffier +1
Gravitational waves (GWs) from compact binary coalescences (CBCs) provide a new avenue to probe the cosmic expansion, in particular the Hubble constant . The spectral sirens m…