263 datasets found

An optical polarimetric catalog for the Small Magelanic Cloud (SMC) is presented. It gives intrinsic and observed polarizations in the V-band for a total of 7207 stars located...

In order to study the initial conditions of massive star formation, we have previously built a sample of 463 high-mass starless clumps (HMSCs) across the inner Galactic plane...

Polarimetry of stars at optical and near-infrared wavelengths is an invaluable tool for tracing interstellar dust and magnetic fields. Recent studies have demonstrated the power...

An electric current is induced by the motion of electrical conducting seawater through the ambient geomagnetic field. The periodic oceanic tidal flow induces an electric current...

This dataset contains ionization and transport values for ultra-hot Jupiter KELT-9b. The transport coefficients are used in the calculation of the atmospheric magnetic field of...

Research data and metadata that was used in the corresponding publication "Fano interference between collective modes in cuprate high-Tc superconductors" (...

100 column data up to z=1 from an MHD cosmological simulation run using ENZO (Bryan+14). All dataset are written in a formatted way. Each column contains: redshift, electron...

This is one subset (300^3 cells) derived from a larger 1024^3 cosmological MHD simulation produced using ENZO on Piz-Daint (CSCS) by F.Vazza& collaborators. In these...

These are 3 subsets (300^3 cells each) derived from larger 1024^3 cosmological MHD simulations produced using ENZO on Piz-Daint (CSCS) by F.Vazza& collaborators. In these...

These are 2 subsets (300^3 cells each) derived from larger 1024^3 cosmological MHD simulations produced using ENZO on Piz-Daint (CSCS) by F.Vazza& collaborators. In these...

Fits files for 3 different projections for a (12.3 Mpc)^3 volume at z=0.1, containing a massive galaxy clusters simulated with ENZO (enzo-project.org). Each pixel is 7.95 kpc....

Tabular data for the cosmic star formation history in cosmological simulations, and of the relative magnetisation output of stellar activity. For meaning of the models please...

This data collection contains the DELTA_B RDR files in the Mercury Solar Orbital (MSO) coordinates system.

Surface-averaged longitudinal magnetic field components have been measured for 15 late-type giants with an accuracy of several Gauss. Cone search capability for table...

Magnetic fields pervade the interstellar medium (ISM), but are difficult to detect and characterize. The new generation of low-frequency radio telescopes, such as the Low...

In solar-type stars, the attenuation of convective blueshift by stellar magnetic activity dominates the RV (radial velocity) variations over the low amplitude signal induced by...

Seismic observations with the space-borne Kepler mission have shown that a number of evolved stars exhibit low-amplitude dipole modes, which is referred to as depressed modes....

One clear manifestation of dynamo action on the Sun is the 22-yr magnetic cycle, exhibiting a polarity reversal and a periodic conversion between poloidal and toroidal fields....

This data collection contains the DELTA_B RDR files in the Mercury Solar Orbital (MSO) coordinates system.

PolarBase is an evolving data base that contains all stellar data collected with the ESPaDOnS and NARVAL high-resolution spectropolarimeters, in their reduced form, as soon as...