output
19962026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2022Show all

184 papers · 1 filter

astro-ph.CO2022★ 49 cited

The Dark Energy Survey Year 3 and eBOSS: constraining galaxy intrinsic alignments across luminosity and colour space

S. Samuroff, R. Mandelbaum, J. Blazek +104

We present direct constraints on galaxy intrinsic alignments using the Dark Energy Survey Year 3 (DES Y3), the Extended Baryon Oscillation Spectroscopic Survey (eBOSS) and its prec…

astro-ph.GA2022★ 24 cited

JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334

Mehrnoosh Tahani, Pierre Bastien, Ray S. Furuya +142

We study the HII regions associated with the NGC 6334 molecular cloud observed in the sub-millimeter and taken as part of the B-fields In STar-forming Region Observations (BISTRO)…

cs.CR2022★ 1 cited

Resource-Interaction Graph: Efficient Graph Representation for Anomaly Detection

James Pope, Jinyuan Liang, Vijay Kumar +13

Security research has concentrated on converting operating system audit logs into suitable graphs, such as provenance graphs, for analysis. However, provenance graphs can grow very…

cs.CY2022★ 34 cited

Epistemological Equation for Analysing Uncontrollable States in Complex Systems: Quantifying Cyber Risks from the Internet of Things

Petar Radanliev, David De Roure, Pete Burnap +1

To enable quantitative risk assessment of uncontrollable risk states in complex and coupled IoT systems, a new epistemological equation is designed and tested though comparative an…

astro-ph.GA2022★ 15 cited

Linking the dust and chemical evolution: Taurus and Perseus -- New collisional rates for HCN, HNC, and their C, N, and H isotopologues

D. Navarro-Almaida, C. T. Bop, F. Lique +18

HCN, HNC, and their isotopologues are ubiquitous molecules that can serve as chemical thermometers and evolutionary tracers to characterize star-forming regions. Despite their impo…

cs.DC2022★ 260 cited

AI-based Fog and Edge Computing: A Systematic Review, Taxonomy and Future Directions

Sundas Iftikhar, Sukhpal Singh Gill, Chenghao Song +15

Resource management in computing is a very challenging problem that involves making sequential decisions. Resource limitations, resource heterogeneity, dynamic and diverse nature o…

astro-ph.GA2022★ 26 cited

The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament

Tao-Chung Ching, Keping Qiu, Di Li +154

We present 850 m dust polarization observations of the massive DR21 filament from the B-fields In STar-forming Region Observations (BISTRO) survey, using the POL-2 polarimeter a…

astro-ph.CO2022★ 27 cited

Probing Lorentz-violating electrodynamics with CMB polarization

Luca Caloni, Serena Giardiello, Margherita Lembo +4

We perform a comprehensive study of the signatures of Lorentz violation in electrodynamics on the Cosmic Microwave Background (CMB) anisotropies. In the framework of the minimal St…

astro-ph.CO2022★ 5 cited

Non-local contribution from small scales in galaxy-galaxy lensing: Comparison of mitigation schemes

J. Prat, G. Zacharegkas, Y. Park +112

Recent cosmological analyses with large-scale structure and weak lensing measurements, usually referred to as 32pt, had to discard a lot of signal-to-noise from small scale…

math.PR2022★ 8 cited

A fractional Hawkes process II: Further characterization of the process

Cassien Habyarimana, Jane A. Aduda, Enrico Scalas +3

We characterize a Hawkes point process with kernel proportional to the probability density function of Mittag-Leffler random variables. This kernel decays as a power law with expon…

astro-ph.GA2022★ 25 cited

VERTICO III: The Kennicutt-Schmidt relation in Virgo cluster galaxies

M. J. Jiménez-Donaire, T. Brown, C. D. Wilson +19

In this VERTICO science paper we aim to study how the star formation process depends on galactic environment and gravitational interactions in the context of galaxy evolution. We e…

astro-ph.GA2022★ 12 cited

Gas kinematics around filamentary structures in the Orion B cloud

Mathilde Gaudel, Jan H. Orkisz, Maryvonne Gerin +27

Understanding the initial properties of star-forming material and how they affect the star formation process is key. From an observational point of view, the feedback from young hi…

eess.IV2022★ 39 cited

High-precision Density Mapping of Marine Debris and Floating Plastics via Satellite Imagery

Henry Booth, Wanli Ma, Oktay Karakus

Combining multi-spectral satellite data and machine learning has been suggested as a method for monitoring plastic pollutants in the ocean environment. Recent studies have made the…

astro-ph.GA2022★ 5 cited

Differences in chemical evolution between isolated and embedded prestellar cores

F. D. Priestley, A. P. Whitworth, E. Fogerty

Models of prestellar cores often assume that the cores are isolated from their environment - material outside the core boundary plays no role in the subsequent evolution. This is u…

cond-mat.mes-hall2022★ 22 cited

Exploring the phases of 3D artificial spin ice: From Coulomb phase to magnetic monopole crystal

M. Saccone, A. Van den Berg, E. Harding +4

Artificial spin-ices consist of lithographic arrays of single-domain magnetic nanowires organised into frustrated lattices. These geometries are usually two-dimensional, allowing a…

astro-ph.HE2022

A long life of excess: The interacting transient SN 2017hcc

S. Moran, M. Fraser, R. Kotak +29

In this study we present the results of a five-year follow-up campaign of the long-lived type IIn supernova SN 2017hcc, found in a spiral dwarf host of near-solar metallicity. The…

astro-ph.GA2022★ 8 cited

A Herschel study of G214.5-1.8: a young, cold and quiescent giant molecular filament on the shell of a HI superbubble

S. D. Clarke, A. Sanchez-Monge, G. M. Williams +3

We present an analysis of the outer Galaxy giant molecular filament (GMF) G214.5-1.8 (G214.5) using Herschel data. We find that G214.5 has a mass of 16,000 M, yet…

astro-ph.GA2022★ 5 cited

Ionising feedback from an O star formed in a shock-compressed layer

Anthony Whitworth, Felix Priestley, Samuel Geen

We develop a simple analytic model for what happens when an O star (or compact cluster of OB stars) forms in a shock compressed layer and carves out an approximately circular hole…

cond-mat.stat-mech2022★ 11 cited

Kauzmann Paradox: a crossover due to diminishing local excitations

Xin-Yuan Gao, Chin-Yuan Ong, Chun-Shing Lee +3

The configurational entropy of supercooled liquids extrapolates to zero at the Kauzmann temperature, causing a crisis called the Kauzmann paradox. Here, using a class of multicompo…

hep-ph2022★ 7 cited

Probing dark matter with polarimetry techniques

Aldo Ejlli, Sander M. Vermeulen, Eyal Schwartz +2

In this work, we propose polarimetry experiments to search for low-mass (sub-eV) bosonic field dark matter, including axions and axion-like particles. We show that a polarimetry co…

astro-ph.EP2022★ 10 cited

Recovering Phosphine in Venus' Atmosphere from SOFIA Observations

Jane S. Greaves, Janusz J. Petkowski, Anita M. S. Richards +3

Searches for phosphine in Venus' atmosphere have sparked a debate. Cordiner et al. 2022 analyse spectra from the Stratospheric Observatory For Infrared Astronomy (SOFIA) and infer…

astro-ph.GA2022★ 33 cited

An ever-present snail shell triggered by a dark matter wake

Robert J. J. Grand, Rüdiger Pakmor, Francesca Fragkoudi +5

We utilize a novel numerical technique to model star formation in cosmological simulations of galaxy formation - called Superstars - to simulate a Milky Way-like galaxy with $\gtrs…

cond-mat.str-el2022★ 14 cited

Controlling charge density order in 2H-TaSe using a van Hove singularity

W. R. B. Luckin, Y. Li, J. Jiang +7

We report on the interplay between a van Hove singularity and a charge density wave state in 2H-TaSe. We use angle-resolved photoemission spectroscopy to investigate changes…

cs.LG2022★ 82 cited

Predicting air quality via multimodal AI and satellite imagery

Andrew Rowley, Oktay Karakuş

Climate change may be classified as the most important environmental problem that the Earth is currently facing, and affects all living species on Earth. Given that air-quality mon…