output
19952026
most citedUniaxial Strain in Graphene by Raman Spectroscopy: G peak splitting, Gruneisen Parameters and Sample Orientation

2k citations

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79 papers · 1 filter

astro-ph.SR2024

Fast optical variability in Supergiant X-ray binaries

D. Di Filippantonio, P. Reig, J. Fabregat

The main goal of this work is to investigate the fast photometric variability of the optical counterparts to supergiant X-ray binaries and to compare the general patterns of such v…

astro-ph.HE2024★ 1 cited

Time-dependent modelling of short-term variability in the TeV-blazar VER J0521+211 during the major flare in 2020

MAGIC Collaboration, S. Abe, J. Abhir +228

The BL Lacertae object VER J0521+211 underwent a notable flaring episode in February 2020. A short-term monitoring campaign, led by the MAGIC (Major Atmospheric Gamma Imaging Chere…

cs.CV2024★ 21 cited

A Full Transformer-based Framework for Automatic Pain Estimation using Videos

Stefanos Gkikas, Manolis Tsiknakis

The automatic estimation of pain is essential in designing an optimal pain management system offering reliable assessment and reducing the suffering of patients. In this study, we…

math.NA2024★ 149 cited

Elliptic reconstruction and a posteriori error estimates for fully discrete linear parabolic problems

Omar Lakkis, Charalambos Makridakis

We derive aposteriori error estimates for fully discrete approximations to solutions of linear parabolic equations on the space-time domain. The space discretization uses finite el…

astro-ph.GA2024★ 6 cited

Overdensity of Lyman-Break Galaxy Candidates Around Hot Dust-Obscured Galaxies

Dejene Zewdie, Roberto J. Assef, Trystan Lambert +15

Hot dust-obscured galaxies (Hot DOGs), are a family of hyper-luminous, heavily obscured quasars. A number of studies have shown that these objects reside in significantly overdense…

cond-mat.mes-hall2024

Moduli spaces and breather dynamics of analytic solutions in Heisenberg exchange-free chiral magnets

Bruno Barton-Singer, Stefano Bolognesi, Sven Bjarke Gudnason +1

We investigate the special case of the chiral magnet with vanishing Heisenberg exchange energy, whose axisymmetric Skyrmion solution has previously been found. The dynamical equati…

cond-mat.mes-hall2024★ 2 cited

First-principles derived force field for h-BN monolayer nanostructures: Applications to sheets, nanotubes and nanotori

Aristotelis P. Sgouros, Markos Arapchatzis, Nektarios N. Lathiotakis +2

In this work, we present an empirical force field for hexagonal boron nitride (hBN) monolayers, derived via a bottom-up strategy from first principles calculations. We aim to deliv…

astro-ph.CO2024

Searching for a signature of turnaround in galaxy clusters with convolutional neural networks

Nikolaos Triantafyllou, Giorgos Korkidis, Vasiliki Pavlidou +1

Galaxy clusters are important cosmological probes that have helped to establish the CDM paradigm as the standard model of cosmology. However, recent tensions between diff…

astro-ph.IM2024★ 2 cited

The WALOP-North Instrument I: Optical Design, Filter Design, Calibration

John A. Kypriotakis, Siddharth Maharana, Ramya M. Anche +18

The Wide Area Linear Optical Polarimeter North (WALOP-North) is an optical polarimeter designed for the needs of the PASIPHAE survey. It will be installed on the 1.3m telescope at…

physics.app-ph2024★ 2 cited

Highly-stable, eco-friendly and selective Cs2AgBiBr6 perovskite-based ozone sensor

Aikaterini Argyrou, Rafaela Maria Giappa, Emmanouil Gagaoudakis +5

Lead halide perovskites have attracted considerable attention as potential gas sensing elements due to their unique ability to detect and respond to an external stimulus with measu…

astro-ph.GA2024★ 18 cited

Molecular gas stratification and disturbed kinematics in the Seyfert galaxy MCG-05-23-16 revealed by JWST and ALMA

D. Esparza-Arredondo, C. Ramos Almeida, A. Audibert +30

Understanding the processes that drive the morphology and kinematics of molecular gas in galaxies is crucial for comprehending star formation and, ultimately, galaxy evolution. Usi…

astro-ph.HE2024

Spectroscopic Modeling of Luminous Transients Powered by H-Rich and He-Rich Circumstellar Interaction

Gururaj A. Wagle, Emmanouil Chatzopoulos, Michael J. Baer

In this study, we perform detailed spectroscopic modeling to analyze the interaction of circumstellar material (CSM) with ejecta in both hydrogen-rich and hydrogen-poor superlumino…

astro-ph.GA2024★ 5 cited

The ALMA-CRISTAL Survey: Complex kinematics of the galaxies at the end of the Reionization Era

K. Telikova, J. González-López, M. Aravena +18

The history of gas assembly in early galaxies is reflected in their complex kinematics. While a considerable fraction of galaxies at z~5 are consistent with rotating disks, current…

astro-ph.HE2024★ 4 cited

Multi-wavelength study of OT 081: broadband modelling of a transitional blazar

MAGIC Collaboration, H. Abe, S. Abe +270

OT 081 is a well-known, luminous blazar that is remarkably variable in many energy bands. We present the first broadband study of the source which includes very-high-energy (VHE, $…

physics.optics2024★ 1 cited

Wettability and Color Change of Copper by Controlling Area Fraction of Laser Ablated Surface

Mantas Gaidys, Stella Maragkaki, Alexandros Mimidis +6

In this research, wettability control by area fraction of laser ablated surface of copper is presented. The functional surfaces with full wettability control from highly hydrophili…

astro-ph.HE2024★ 15 cited

A wiggling filamentary jet at the origin of the blazar multi-wavelength behaviour

C. M. Raiteri, M. Villata, M. I. Carnerero +96

Blazars are beamed active galactic nuclei known for their strong multi-wavelength variability on timescales from years down to minutes. We aim to investigate the suitability of the…

astro-ph.HE2024★ 7 cited

Insights from the first flaring activity of a high-synchrotron-peaked blazar with X-ray polarization and VHE gamma rays

MAGIC Collaboration, K. Abe, S. Abe +250

We study a flaring activity of the HSP Mrk421 that was characterized from radio to very-high-energy (VHE; E TeV) gamma rays with MAGIC, Fermi-LAT, Swift, XMM-Newton and sever…

cs.CV2024★ 3 cited

Enhancing Action Recognition by Leveraging the Hierarchical Structure of Actions and Textual Context

Manuel Benavent-Lledo, David Mulero-Pérez, David Ortiz-Perez +2

We propose a novel approach to improve action recognition by exploiting the hierarchical organization of actions and by incorporating contextualized textual information, including…

cs.CY2024★ 1 cited

Before & After: The Effect of EU's 2022 Code of Practice on Disinformation

Emmanouil Papadogiannakis, Panagiotis Papadopoulos, Nicolas Kourtellis +1

Over the past few years, the European Commission has made significant steps to reduce disinformation in cyberspace. One of those steps has been the introduction of the 2022 "Streng…

astro-ph.SR2024★ 3 cited

Emulators for stellar profiles in binary population modeling

Elizabeth Teng, Ugur Demir, Zoheyr Doctor +14

Knowledge about the internal physical structure of stars is crucial to understanding their evolution. The novel binary population synthesis code POSYDON includes a module for inter…

astro-ph.CO2024★ 2 cited

Distribution-free uncertainty quantification for inverse problems: application to weak lensing mass mapping

Hubert Leterme, Jalal Fadili, Jean-Luc Starck

In inverse problems, distribution-free uncertainty quantification (UQ) aims to obtain error bars with coverage guarantees that are independent of any prior assumptions about the da…

astro-ph.GA2024★ 5 cited

Strong turbulence and magnetic coherent structures in the interstellar medium

Evangelia Ntormousi, Loukas Vlahos, Anna Konstantinou +1

Magnetic turbulence is classified as weak or strong based on the relative amplitude of the magnetic field fluctuations compared to the mean field. These two classifications have di…

astro-ph.GA2024★ 4 cited

CO spectra of the ISM in the Host Galaxies of the Most Luminous WISE-Selected AGNs

Lee R. Martin, Andrew W. Blain, Tanio Díaz-Santos +7

We present observations of mid-J J=4-3 or J=5-4 carbon monoxide (CO) emission lines and continuum emission from a sample of ten of the most luminous log(L/L_solar)~14 Hot Dust-Obsc…

astro-ph.IM2024★ 3 cited

The Method of Searching for Rotations of the Polarization Position Angle of Quasars

S. S. Savchenko, D. A. Morozova, S. G. Jorstad +11

Observations of quasars show that the polarization position angle of the emission coming from them varies greatly over time, including periods called rotations during which the ang…