Nabila Aghanim

TL;DR: In this article, the authors used the generalized needlet internal linear combination (GNILC) method, which uses spatial information (the angular power spectra) to disentangle the Galactic thermal dust emission from cosmic infrared background (CIB) anisotropies.

TL;DR: In this paper, the presence of secondary anisotropies is not taken into account in Cosmic Microwave Background analyses, and an exact analytical expression for computing the biases on parameters when any additive signal is neglected in the analysis is developed.

TL;DR: In this article, the magnetic field in the Rosette nebula is modeled as a uniform shell of swept-up ISM, which is assumed to evolve from an initially uniform configuration following the expansion of ionized gas and the formation of a shell.

TL;DR: In this paper, the stellar-to-halo mass relationship (SHMR) was determined using a parametric abundance matching technique using precise galaxy stellar mass function measurements in the COSMOS field, and the authors considered the principal sources of uncertainty in their stellar mass measurements and also the variation in halo mass estimates in the literature.

TL;DR: In this paper, a cross-correlation study between the kinetic Sunyaev-Zel'dovich effect and the cosmological 21 cm signal was performed using a simulated reionization history in 100 h(-1) Mpc scale N-body simulations with radiative transfer.