51 citations · 115 across the 7 of their papers we have counts for
7 papers
What does it mean to take the mean? The effect of the averaging scale on the characterization of interstellar turbulence
A. Konstantinou, E. Ntormousi, K. Tassis
In interstellar medium studies, separating ordered and random velocity or magnetic fields is essential for interpreting turbulence in both simulations and observations. We investig…
Gas-phase metallicity gradients in galaxies at
G. Venturi, S. Carniani, E. Parlanti +18
The study of gas-phase metallicity and its spatial distribution at high redshift is crucial to understand the processes that shaped the growth and evolution of galaxies in the earl…
Time evolution of the galactic relation: the impact of the magnetic field morphology
A. Konstantinou, E. Ntormousi, K. Tassis +1
One of the most frequently used indicators to characterize the magnetic field's influence on star formation is the relation between magnetic field strength and gas density ( r…
Bright-Moon Sky as a Wide-Field Linear Polarimetric Flat Source for Calibration
S. Maharana, S. Kiehlmann, D. Blinov +20
Next-generation wide-field optical polarimeters like the Wide-Area Linear Optical Polarimeters (WALOPs) have a field of view (FoV) of tens of arcminutes. For efficient and accurate…
Starlight-polarization-based tomography of the magnetized interstellar medium: PASIPHAE's line-of-sight inversion method
V. Pelgrims, G. V. Panopoulou, K. Tassis +20
We present the first Bayesian method for tomographic decomposition of the plane-of-sky orientation of the magnetic field with the use of stellar polarimetry and distance. This stan…
The effect of cosmic variance on the characteristics of dust polarization power spectra
V. Pelgrims, E. Ntormousi, K. Tassis
In the context of cosmic microwave background polarization studies and the characterization of the Galactic foregrounds, the power spectrum analysis of the thermal dust polarizatio…
SMILE: Search for MIlli-LEnses
C. Casadio, D. Blinov, A. C. S. Readhead +17
Dark Matter (DM) halos with masses below , which would help to discriminate between DM models, may be detected through their gravitational effect on distant…