output
20132026
most citedHow to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70

361 citations

79 papers

gr-qc2026

A framework for creating galaxy models in the geometry of the conservation group with dark matter halos and flat rotation curves

Edward Lee Green

Pandres has developed a theory which extends the geometrical structure of a real four-dimensional space-time via a field of orthonormal tetrads with an enlarged covariance group. T…

cond-mat.stat-mech2026

Accelerating Multicanonical Sampling with Irreversibility

Thomas Vogel, Ying Wai Li

Flat-histogram Monte Carlo simulations are well-established, robust methods to perform random walks in a physical observable or parameter space, making them suitable for finding gr…

hep-ph2025★ 2 cited

Weak Charge Form Factor Determination at the Electron-Ion Collider

Hooman Davoudiasl, Hongkai Liu, Sonny Mantry +1

Determining the weak charge form factor, , of nuclei over a continuous range of momentum transfers, GeV, is essential for mapping out the…

math.AP2025

On compressible fluid flows of Forchheimer-type in rotating heterogeneous porous media

Emine Celik, Luan Hoang, Thinh Kieu

We study the dynamics of compressible fluids in rotating heterogeneous porous media. The fluid flow is of {F}orchheimer-type and is subject to a mixed mass and volumetric flux boun…

hep-ph2025

Jet Charge with Global Event Shapes: Probing Quark Flavor Dynamics

Yang-Ting Chien, Sonny Mantry

We propose measuring the jet electric charge of jet regions, defined within the framework of global event shapes, as a probe of quark flavor dynamics within the nucleon and the had…

astro-ph.SR2025

Discovery of the pre-main-sequence eclipsing binary MML 48

Y. Gómez Maqueo Chew, L. Hebb, H. C. Stempels +12

We present the discovery of the eclipsing binary MML 48, which is a member of Upper Centaurus Lupus, has an associated age of 16 Myr, and is composed of two young, low-mass stars.…

cond-mat.soft2025★ 2 cited

Confusion-driven machine learning of structural phases of a flexible, magnetic Stockmayer polymer

Dilina Perera, Samuel McAllister, Joan Josep Cerdà +1

We use a semi-supervised, neural-network based machine learning technique, the confusion method, to investigate structural transitions in magnetic polymers, which we model as chain…

astro-ph.GA2025

H-, He-like recombination spectra -- V: On the dependence of the simulated line intensities on the number of electronic levels of the atoms

F. Guzmán, M. Chatzikos, G. Ferland

This paper presents a study of the dependence of the simulated intensities of recombination lines from hydrogen and helium atoms on the number of -resolved principal quantum…

astro-ph.GA2024★ 1 cited

Recovering the properties of the interstellar medium through integrated spectroscopy: application to the z~0 ECO volume-limited star-forming galaxy sample

V. Lebouteiller, C. T. Richardson, M. S. Polimera +7

Deriving physical parameters from integrated galaxy spectra is paramount to interpret the cosmic evolution of star formation, chemical enrichment, and energetic sources. We develop…

astro-ph.GA2024★ 3 cited

Identification and Quenching of Nugget Galaxies in the RESOLVE Survey at z = 0

Derrick S. Carr, Sheila J. Kannappan, Mark A. Norris +7

We present a complete census of candidate nuggets, i.e., dense galaxies likely formed by compaction with intense gas influx, within the volume-limited REsolved Spectrosc…

hep-ph2024★ 6 cited

The DIS 1-Jettiness Event Shape at NLL+

Haotian Cao, Zhong-Bo Kang, Xiaohui Liu +1

We present results for the and 1-Jettiness global event shape distributions, for Deep Inelastic Scattering (DIS), at the NLL + level of accurac…

math.AP2023★ 6 cited

Anisotropic flows of Forchheimer-type in porous media and their steady states

Luan Hoang, Thinh Kieu

We study the anisotropic Forchheimer-typed flows for compressible fluids in porous media. The first half of the paper is devoted to understanding the nonlinear structure of the ani…

gr-qc2023★ 9 cited

Nuclear physics with gravitational waves from neutron stars disrupted by black holes

Teagan A. Clarke, Lani Chastain, Paul D. Lasky +1

Gravitational waves from neutron star-black hole (NSBH) mergers that undergo tidal disruption provide a potential avenue to study the equation of state of neutron stars and hence t…

astro-ph.EP2023★ 34 cited

The TIME Table: Rotation and Ages of Cool Exoplanet Host Stars

Eric Gaidos, Zachary Claytor, Ryan Dungee +2

Age is a stellar parameter that is both fundamental and difficult to determine. Among middle-aged M dwarfs, the most prolific hosts of close-in and detectable exoplanets, gyrochron…

astro-ph.SR2022★ 37 cited

TESS Hunt for Young and Maturing Exoplanets (THYME) IX: a 27 Myr extended population of Lower-Centaurus Crux with a transiting two-planet system

Mackenna L. Wood, Andrew W. Mann, Madyson G. Barber +35

We report the discovery and characterization of a nearby (~ 85 pc), older (27 +/- 3 Myr), distributed stellar population near Lower-Centaurus-Crux (LCC), initially identified by se…

math.AP2022

Classical Solutions of the Fornberg-Whitham Equation

Georgia Burkhalter, Ryan C. Thompson, Madison Waldrep

In this paper, we prove well-posedness in (a.k.a. classical solutions) of the Fornberg-Whitham equation. To achieve this objective, we study its weak formulation…

astro-ph.GA2022★ 28 cited

Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe

Sarah Casura, Jochen Liske, Aaron S. G. Robotham +10

We derive single Sérsic fits and bulge-disk decompositions for 13096 galaxies at redshifts z < 0.08 in the GAMA II equatorial survey regions in the Kilo-Degree Survey (KiDS) g, r a…

astro-ph.HE2022★ 16 cited

X-ray spectroscopy in the microcalorimeter era 4: Optical depth effects on the soft X-rays studied with CLOUDY

Priyanka Chakraborty, Gary Ferland, Marios Chatzikos +4

In this paper, we discuss atomic processes modifying the soft X-ray spectra in from optical depth effects like photoelectric absorption and electron scattering suppressing the soft…

nucl-ex2022★ 10 cited

Proton Compton Scattering from Linearly Polarized Gamma Rays

X. Li, M. W. Ahmed, A. Banu +27

Differential cross sections for Compton scattering from the proton have been measured at scattering angles of , , and in the laboratory frame using…

astro-ph.GA2022★ 34 cited

RESOLVE and ECO: Finding Low-Metallicity Dwarf AGN Candidates Using Optimized Emission-Line Diagnostics

Mugdha S. Polimera, Sheila J. Kannappan, Chris T. Richardson +6

Existing star-forming vs. active galactic nucleus (AGN) classification schemes using optical emission-line diagnostics mostly fail for low-metallicity and/or highly star-forming ga…

astro-ph.EP2022★ 15 cited

Planetesimals Around Stars with TESS (PAST): II. An M Dwarf "Dipper" Star with a Long-Lived Disk in the TESS Continuous Viewing Zone

Eric Gaidos, Andrew W. Mann, Bárbara Rojas-Ayala +6

Studies of T Tauri disks inform planet formation theory; observations of variability due to occultation by circumstellar dust are a useful probe of unresolved, planet-forming inner…

hep-ph2022★ 25 cited

Neutral-Current Electroweak Physics and SMEFT Studies at the EIC

Radja Boughezal, Alexander Emmert, Tyler Kutz +6

We study the potential for precision electroweak (EW) measurements and beyond-the-Standard Model (BSM) searches using cross-section asymmetries in neutral-current (NC) deep inelast…

cond-mat.soft2022★ 11 cited

Supervised and Unsupervised Machine Learning of Structural Phases of Polymers Adsorbed to Nanowires

Quinn Parker, Dilina Perera, Ying Wai Li +1

We identify configurational phases and structural transitions in a polymer nanotube composite by means of machine learning. We employ various unsupervised dimensionality reduction…

astro-ph.GA2022★ 249 cited

Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions

Simon P. Driver, Sabine Bellstedt, Aaron S. G. Robotham +67

In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248682 galaxy spectra, and, in combination with earli…