activity
20132026
most citedPolarized Blazar X-rays imply particle acceleration in shocks

140 citations · 2k across the 60 of their papers we have counts for

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Showing 2021Show all

10 papers · 1 filter

astro-ph.GA2021★ 45 cited

The width of Herschel filaments varies with distance

G. V. Panopoulou, S. E. Clark, A. Hacar +5

Context: Filamentary structures in nearby molecular clouds have been found to exhibit a characteristic width of 0.1 pc, as observed in dust emission. Understanding the origin of th…

astro-ph.CO2021★ 16 cited

Improved Galactic Foreground Removal for B-Modes Detection with Clustering Methods

Giuseppe Puglisi, Gueorgui Mihaylov, Georgia V. Panopoulou +4

Characterizing the sub-mm Galactic emission has become increasingly critical especially in identifying and removing its polarized contribution from the one emitted by the Cosmic Mi…

astro-ph.GA2021★ 14 cited

HI-H transition: exploring the role of the magnetic field

R. Skalidis, K. Tassis, G. V. Panopoulou +6

Atomic gas in the diffuse interstellar medium (ISM) is organized in filamentary structures. These structures usually host cold and dense molecular clumps. The Galactic magnetic fie…

astro-ph.HE2021★ 57 cited

First Predicted Cosmic Ray Spectra, Primary-to-Secondary Ratios, and Ionization Rates from MHD Galaxy Formation Simulations

Philip F. Hopkins, Iryna S. Butsky, Georgia V. Panopoulou +4

We present the first simulations evolving resolved spectra of cosmic rays (CRs) from MeV-TeV energies (including electrons, positrons, (anti)protons, and heavier nuclei), in live k…

astro-ph.GA2021★ 15 cited

Dust in the Wind with Resonant Drag Instabilities: I. The Dynamics of Dust-Driven Outflows in GMCs and HII Regions

Philip F. Hopkins, Anna L. Rosen, Jonathan Squire +4

Radiation-dust driven outflows, where radiation pressure on dust grains accelerates gas, occur in many astrophysical environments. Almost all previous numerical studies of these sy…

astro-ph.GA2021★ 37 cited

Revisiting the distance to radio Loops I and IV using Gaia and radio/optical polarization data

G. V. Panopoulou, C. Dickinson, A. C. S. Readhead +2

Galactic synchrotron emission exhibits large-angular-scale features known as radio spurs and loops. Determining the physical size of these structures is important for understanding…

astro-ph.HE2021★ 19 cited

The Time-Dependent Distribution of Optical Polarization Angle Changes in Blazars

S. Kiehlmann, D. Blinov, I. Liodakis +17

At optical wavelengths, blazar Electric Vector Position Angle (EVPA) rotations linked with gamma-ray activity have been the subject of intense interest and systematic investigation…

astro-ph.IM2021★ 2 cited

WALOP-South: A wide-field one-shot linear optical polarimeter for PASIPHAE survey

Siddharth Maharana, John A. Kypriotakis, A. N. Ramaprakash +20

WALOP (Wide-Area Linear Optical Polarimeter)-South, to be mounted on the 1m SAAO telescope in South Africa, is first of the two WALOP instruments currently under development for ca…

astro-ph.IM2021★ 9 cited

WALOP-South: A Four Camera One Shot Imaging Polarimeter for PASIPHAE Survey. Paper I -- Optical Design

Siddharth Maharana, John A. Kypriotakis, A. N. Ramaprakash +17

The WALOP-South instrument will be mounted on the 1 m SAAO telescope in South Africa as part of the PASIPHAE program to carry out a linear imaging polarization survey of the Galact…

astro-ph.CO2021★ 53 cited

Evidence for Line-of-Sight Frequency Decorrelation of Polarized Dust Emission in Data

V. Pelgrims, S. E. Clark, B. S. Hensley +5

If a single line of sight (LOS) intercepts multiple dust clouds of different spectral energy distributions and magnetic field orientations, the frequency scaling of each of the Sto…