output
20182026
most citedDiscovery of strongly variable X-ray polarization in the neutron star low-mass X-ray binary transient XTE J1701462

50 citations

25 papers

astro-ph.SR2026

An Eccentric Massive Protobinary Assembled via a Core-merger Parabolic Encounter

Yao Wang, Yichen Zhang, Rubén Fedriani +14

Most massive stars form in binary systems, which profoundly influence their subsequent evolution. However, how such systems form remains poorly understood, with several competing s…

nucl-th2026

Nuclear Mass Models with Deformation Optimized and Diagnosed by Bayesian Analysis with Markov Chain Monte Carlo

Xiangnan Lee, Yi Hua Lam, Zi-Ao Zhang +1

We employ a full Bayesian analysis with adaptive Metropolis-Hastings Markov chain Monte Carlo (BA-MCMC) sampling to systematically study the posterior probability distributions of…

cond-mat.str-el2026

Majorana-assisted nonlocal spin correlation in quasi-one-dimensional Kitaev spin liquids

Yuki Yamazaki, Shingo Kobayashi, Akira Furusaki

We propose Majorana-assisted nonlocal spin correlation as a manifestation of Majorana nonlocality in quasi-one-dimensional (1D) Kitaev spin liquids. Focusing on the flux-free secto…

math-ph2025

Superconductivity and Low Energy Excitations in an Attractive Hubbard Model

Yukimi Goto, Tohru Koma, Hironobu Yoshida

We study an attractive Hubbard model on bipartite lattices. In the grand canonical formalism,we prove the existence of superconducting long-range order in the ground state on Lieb…

cs.CL2025

Research Borderlands: Analysing Writing Across Research Cultures

Shaily Bhatt, Tal August, Maria Antoniak

Improving cultural competence of language technologies is important. However most recent works rarely engage with the communities they study, and instead rely on synthetic setups a…

astro-ph.GA2025★ 2 cited

Starburst-Driven Galactic Outflows -- Unveiling the Suppressive Role of Cosmic Ray Halos

Leonard E. C. Romano, Ellis R. Owen, Kentaro Nagamine

Aims. We investigate the role of cosmic ray (CR) halos in shaping the properties of starburst-driven galactic outflows. Methods. We develop a microphysical model for galactic outfl…

cs.RO2024★ 1 cited

Model Checking and Verification of Synchronisation Properties of Cobot Welding

Yvonne Murray, Henrik Nordlie, David A. Anisi +2

This paper describes use of model checking to verify synchronisation properties of an industrial welding system consisting of a cobot arm and an external turntable. The robots must…

astro-ph.EP2024

Water vapor as a probe of the origin of gas in debris disks

Yasuhiro Hasegawa, Riouhei Nakatani, Isabel Rebollido +5

Debris disks embrace the formation and evolution histories of planetary systems. Recent detections of gas in these disks have received considerable attention, as its origin ties up…

astro-ph.GA2024★ 5 cited

The SOFIA Massive (SOMA) Star Formation Q-band follow-up I. Carbon-chain chemistry of intermediate-mass protostars

Kotomi Taniguchi, Prasanta Gorai, Jonathan C. Tan +10

Evidence for similar chemical characteristics around low- and high-mass protostars has been found: in particular, a variety of carbon-chain species and complex organic molecules (C…

astro-ph.GA2024★ 3 cited

The factors that influence protostellar multiplicity I: Gas temperature, density, and mass in Perseus with Nobeyama

N. M. Murillo, C. M. Fuchs, D. Harsono +9

Protostellar multiplicity is common at all stages and mass ranges. However, the factors that determine the multiplicity of protostellar systems have not been systematically charact…

astro-ph.HE2024★ 35 cited

IXPE observation of PKS 2155-304 reveals the most highly polarized blazar

Pouya M. Kouch, Ioannis Liodakis, Riccardo Middei +133

We report the X-ray polarization properties of the high-synchrotron-peaked (HSP) blazar PKS 2155304 based on observations with the Imaging X-ray Polarimetry Explorer (IXPE). We…

astro-ph.HE2024★ 13 cited

Joint ALMA/X-ray monitoring of the radio-quiet type 1 AGN IC 4329A

E. Shablovinskaya, C. Ricci, C-S. Chang +20

The origin of a compact millimeter (mm, 100-250 GHz) emission in radio-quiet active galactic nuclei (RQ AGN) remains debated. Recent studies propose a connection with self-absorbed…

astro-ph.GA2024★ 43 cited

Hunt for complex cyanides in protostellar ices with JWST: Tentative detection of CHCN and CHCN

P. Nazari, W. R. M. Rocha, A. E. Rubinstein +20

Nitrogen-bearing complex organic molecules have been commonly detected in the gas phase but not yet in interstellar ices. This has led to the long-standing question of whether thes…

astro-ph.GA2024★ 15 cited

A deep search for large complex organic species toward IRAS16293-2422 B at 3 mm with ALMA

P. Nazari, J. S. Y. Cheung, J. Ferrer Asensio +14

Complex organic molecules (COMs) have been detected ubiquitously in protostellar systems. However, at shorter wavelengths (~0.8mm) it is more difficult to detect larger molecules t…

astro-ph.HE2023★ 12 cited

Pulsar-wind-nebula-powered Galactic center X-ray filament G0.13-0.11: Proof of the synchrotron nature by IXPE

Eugene Churazov, Ildar Khabibullin, Thibault Barnouin +103

We report the discovery of X-ray polarization from the X-ray-bright filament. G0.13-0.11 in the Galactic center (GC) region. This filament features a bright, hard X-ray source that…

astro-ph.SR2023★ 30 cited

The Perseus ALMA Chemical Survey (PEACHES). III. Sulfur-bearing species tracing accretion and ejection processes in young protostars

E. Artur de la Villarmois, V. V. Guzman, Y. -L. Yang +2

(Abridged) Sulfur chemistry is poorly understood in the process of low-mass star and planet formation, where the main carriers of sulfur are still unknown. Despite the fact that si…

astro-ph.GA2023★ 9 cited

FAUST X: Formaldehyde in the Protobinary System [BHB2007] 11: Small Scale Deuteration

Lucy Evans, Charlotte Vastel, Francisco Fontani +16

Context. Deuterium in H-bearing species is enhanced during the early stages of star formation, however, only a small number of high spatial resolution deuteration studies exist tow…

astro-ph.GA2023★ 20 cited

The first detection of SiC in the interstellar medium

S. Massalkhi, I. Jiménez-Serra, J. Martín-Pintado +7

We report the first detection of SiC in the interstellar medium. The molecule was identified through six rotational transitions toward G\,+0.6930.027, a molecular cloud loca…

astro-ph.HE2023★ 50 cited

Discovery of strongly variable X-ray polarization in the neutron star low-mass X-ray binary transient XTE J1701462

Massimo Cocchi, Andrea Gnarini, Sergio Fabiani +105

After about 16 years since its first outburst, the transient neutron star low-mass X-ray binary XTE J1701462 turned on again in September 2022, allowing for the first study of i…

astro-ph.HE2023★ 45 cited

X-ray polarimetry and spectroscopy of the neutron star low-mass X-ray binary GX 9+9: an in-depth study with IXPE and NuSTAR

F. Ursini, R. Farinelli, A. Gnarini +101

We report on a comprehensive analysis of simultaneous X-ray polarimetric and spectral data of the bright atoll source GX 9+9 with the Imaging X-ray Polarimetry Explorer (IXPE) and…

astro-ph.HE2023★ 29 cited

Complex variations of X-ray polarization in the X-ray pulsar LS V +44 17/RX J0440.9+4431

Victor Doroshenko, Juri Poutanen, Jeremy Heyl +109

We report on Imaging X-ray polarimetry explorer (IXPE) observations of the Be-transient X-ray pulsar LS V +44 17/RX J0440.9+4431 made at two luminosity levels during the giant outb…

astro-ph.HE2023★ 24 cited

A polarimetrically oriented X-ray stare at the accreting pulsar EXO 2030+375

Christian Malacaria, Jeremy Heyl, Victor Doroshenko +104

Accreting X-ray pulsars (XRPs) are presumably ideal targets for polarization measurements, as their high magnetic field strength is expected to polarize the emission up to a polari…

nucl-ex2023★ 6 cited

Hypernuclear event detection in the nuclear emulsion with Monte Carlo simulation and machine learning

A. Kasagi, W. Dou, V. Drozd +18

This study developed a novel method for detecting hypernuclear events recorded in nuclear emulsion sheets using machine learning techniques. The artificial neural network-based obj…

astro-ph.HE2023★ 31 cited

X-ray pulsar GRO J100857 as an orthogonal rotator

Sergey S. Tsygankov, Victor Doroshenko, Alexander A. Mushtukov +99

X-ray polarimetry is a unique way to probe the geometrical configuration of highly magnetized accreting neutron stars (X-ray pulsars). GRO J100857 is the first transient X-ray p…