Sensitivity modeling for LiteBIRD
Journal of Low Temperature Physics Springer Nature 211:5-6 (2022) 384-397
Abstract:
LiteBIRD is a future satellite mission designed to observe the polarization of the cosmic microwave background radiation in order to probe the inflationary universe. LiteBIRD is set to observe the sky using three telescopes with transition-edge sensor bolometers. In this work we estimated the LiteBIRD instrumental sensitivity using its current design. We estimated the detector noise due to the optical loadings using physical optics and ray-tracing simulations. The noise terms associated with thermal carrier and readout noise were modeled in the detector noise calculation. We calculated the observational sensitivities over fifteen bands designed for the LiteBIRD telescopes using assumed observation time efficiency.Unveiling the formation of NGC 2915 with MUSE: A counter-rotating stellar disk embedded in a disordered gaseous environment⋆
Astronomy & Astrophysics EDP Sciences 668 (2022) a179
The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole
(2022)
Comprehensive coverage of particle acceleration and kinetic feedback from the stellar mass black hole V404 Cygni
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 518:1 (2022) 1243-1259
The Thousand-Pulsar-Array program on MeerKAT -- IX. The time-averaged properties of the observed pulsar population
(2022)