ESC observations of SN 2005cf I Photometric evolution of a normal Type Ia supernova

All time series used in this work (RV, activity indices and light curves from CARMENES, MAROON-X, HARPS, HIRES, MuSCAT2, LCOGT, SuperWASP, ASAS-SN, TJO, and TESS) are available at

Ancestral sequence reconstruction (ASR) and resurrection (i.e. functional expression in a heterologous host) allows enzymes with different properties to be disclosed while its

In this paper, we characterize the vanishing of such invariants for a

When the evolution of the drop takes place at constant angular momentum, as is the case when the drop is mechanically isolated, and axial symmetry is imposed, we always converge to

However, given the present scenario of scarce allosteric-site data, we decided to perform a large-scale analysis of protein ligand-binding pockets, as these

3 we show the photometric and astrometric uncertainties obtained along with the Ks-luminosity function (KLF). We detected 1618 stars and the detection limit, that we define as the

- a propeller model (with a fraction of the mass accreted) accounts for the bolometric high energy luminosity and qualitatively explains the radio and the gamma-ray emission;. -

This Raman image is colour-coded, where the intensity of the colour is correlated with the Raman intensity of three different bands: the A 1g mode of spinel Co 3 O 4 oxide (solid