Journal: Monthly Notices of the Royal Astronomical Society
Publication
Escaping stars from young low-N clusters
With the use of N-body calculations, the numbers and properties of escaping stars from low-N (N= 100 and 1000) young embedded star clusters prior to gas...
Establishing the level of cylindrical rotation in boxy/peanut bulges
We present SAURON integral-field observations of a sample of 12 mid-to-high-inclination disc galaxies, to unveil hidden bars on the basis of their kinematics, i...
Estimating fundamental parameters of nearby M dwarfs from SPIRou spectra
We present the results of a study aiming at retrieving the fundamental parameters of M dwarfs from spectra secured with SPIRou, the near-infrared high...
Estimating the atmospheric properties of 44 M dwarfs from SPIRou spectra
We describe advances on a method designed to derive accurate parameters of M dwarfs. Our analysis consists in comparing high-resolution infrared spectra...
Estimating the bispectrum of the Very Small Array data
We estimate the bispectrum of the Very Small Array data from the compact and extended configuration observations released in 2002 December, and compare our...
Estimating the impact of recombination uncertainties on the cosmological parameter constraints from cosmic microwave background experiments
We use our most recent training set for the RICO code to estimate the impact of recombination uncertainties on the posterior probability distributions which...
Estimations of the magnetic field strength in the torus of IC 5063 using near-infrared polarimetry
An optically and geometrically thick torus obscures the central engine of active galactic nuclei (AGN) from some lines of sight. From a magnetohydrodynamical...
ETHOS 1: a high-latitude planetary nebula with jets forged by a post-common-envelope binary central star
We report on the discovery of ETHOS 1 (PN G068.1+11.0), the first spectroscopically confirmed planetary nebula (PN) from a survey of the SuperCOSMOS Science...
Euclid preparation - XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band images
Next-generation telescopes, like Euclid, Rubin/LSST, and Roman, will open new windows on the Universe, allowing us to infer physical properties for tens of...