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H{alpha} equivalent widths of 36 Lyn (HD 79158)
This paper reports the photospheric, magnetic and circumstellar gas characteristics of the magnetic B8p star 36 Lyncis (HD 79158). Using archival data and new polarised and... -
Earthbound interplanetary shocks
This table contains space weather data based on 360 interplanetary shocks (forward and reverse) observed by ACE during the 80 month time period from January 1998 to August 2004.... -
Stellar magnetic rotational phase curves
Magnetized stars usually exhibit periodic variations of the effective (longitudinal) magnetic field B_e_ caused by their rotation. We present a catalog of magnetic rotational... -
Isolated massive white dwarfs catalog
We present the catalogue of 112 massive isolated white dwarfs, both magnetic and nonmagnetic, with masses M>0.8M_{sun}_. Mass determinations and other parameters of white... -
Magnetic field in V2052 Oph
V2052 Oph is a {beta} Cep star with vsini~60km/s. The behavior of its stellar wind was studied in the ultraviolet wavelength region with the IUE satellite. It revealed periodic... -
X-ray emission in cool main sequence stars
The maximum amplitude A_max_ of spot-induced brightness variations from long-term V-band photometry and the ratio L_X_/L_bol_ between X-ray and bolometric luminosities are... -
Rotation and magnetic field in omega Ori
Omega Ori is a B2IIIe star for which rotational modulation and non-radial pulsations (NRP) have been recently investigated from two independent observational campaigns in 1998... -
Catalogue of stellar effective magnetic fields
We present the catalogue of averaged quadratic effective magnetic fields for 596 main sequence and giant stars. The catalogue is derived from measurements of the stellar... -
Cyclotron lines in Vela X-1
Fitting parameters for the phase resolved spectra of the 2000 and 1998 observation are given. The model in use is the Negative Positive EXponential (NPEX) model (with Gamma_2_... -
Starspot cycles of six young solar analogues
A long-term photometric monitoring of a selected sample of solar analogues has been carried out since early nineties as part of "The Sun in tim" project, which is aimed at a... -
Magnetic field structure in W51A
We present 850{mu}m imaging polarimetry of the W51A massive star forming region performed with SCUBA on the James Clerk Maxwell Telescope (JCMT) situated close to the summit of... -
An analysis of the Ap binary HD 81009
File table2.dat contains the 74 new measured radial velocities of the primary component of the SB2 HD 81009. -
Catalog of Magnetic Field Measurements
The catalog contains references to all measurements of stellar magnetic fields published in the literature between 1958 and 1981. The catalog provides for each object... -
PolarBase spectropolarimetric database (ESPaDOnS, NARVAL)
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... -
MESSENGER Magnetometer KT17 Model Mercury Solar Orbital (MSO) Residual Data
This data collection contains the DELTA_B RDR files in the Mercury Solar Orbital (MSO) coordinates system. -
MESSENGER Magnetometer KT17 Model Mercury Solar Orbital (MSO) Residual Data
This data collection contains the DELTA_B RDR files in the Mercury Solar Orbital (MSO) coordinates system. -
RM sky models for E18B at z=0.1
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.... -
100 simulated line of sights up to z=1
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... -
Simulated cosmic volume - astrophysical seeding scenario
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... -
Simulated cosmic volume - Primordial magnetic seeding models.
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...