Exploring cosmic origins with CORE: The instrument
We describe a space-borne, multi-band, multi-beam polarimeter aiming at a precise and accurate measurement of the polarization of the Cosmic Microwave...
Exploring galaxy evolution time-scales in clusters: insights from the projected phase space
Galaxies infalling into clusters undergo both star formation quenching and morphological transformation due to environmental effects. We investigate these...
Exploring Magnetic Loops and Serpentine Fields in the Quiet Sun with the GRIS-IFU
Synthetic observations produced from radiative magnetohydrodynamic simulations have predicted that higher polarization fractions in the quiet solar photosphere...
Exploring massive star early evolution: the case of the Herschel 36 A triple system
Theoretical models show that some massive stars have not yet arrived at the zero-age main sequence (ZAMS) at the end of the accretion phase. At that time, they...
Exploring nine simultaneously occurring transients on April 12th 1950
Nine point sources appeared within half an hour on a region within ∼? 10 arcmin of a red-sensitive photographic plate taken in April 1950 as part of the...
Exploring spectropolarimetric inversions using neural fields: Solar chromospheric magnetic field under the weak-field approximation
Context. Full-Stokes polarimetric datasets, originating from slit-spectrograph or narrow-band filtergrams, are routinely acquired nowadays. The data rate is...
Exploring the circumstellar environment of the young eruptive star V2492 Cygni
Context. V2492 Cyg is a young eruptive star that went into outburst in 2010. The near-infrared color changes observed since the outburst peak suggest that the...
Exploring the contamination of the DES-Y1 cluster sample with SPT-SZ selected clusters
We perform a cross validation of the cluster catalogue selected by the red-sequence Matched-filter Probabilistic Percolation algorithm (redMaPPer) in Dark...
Exploring the correlation between dark matter, intracluster light, and globular cluster distribution in SMACS0723
We present a free-form model of SMACS0723, the first cluster observed with JWST. This model does not make any strong assumptions on the distribution of mass...