output
20202026
most citedExpanding Explainability: Towards Social Transparency in AI systems

497 citations

246 papers

astro-ph.SR2026

SN 2021pfs: A Type Ia Supernova Likely Affected by Progenitor Metallicity, as Revealed by Comparison with Its Twin Counterpart

Abdusamatjan Iskandar, Xiaofeng Wang, Ali Esamdin +16

We present extensive photometric and spectroscopic observations of the normal type Ia supernovae (SNe Ia) 2021pfs, which occurred in the Seyfert 2 galaxy NGC 5427 at a redshift 0.0…

hep-ph2026

Analysis of Nuclear Fragmentation Functions for Pions with and Dependence

Mengyang Li, Zijian Ye, Jun Gao +3

We present a QCD analysis of pion nuclear fragmentation functions (nFFs), which encode nuclear modifications to hadronization in high-energy nuclear collisions. Within this framewo…

astro-ph.HE2026

Las Cumbres Observatory Gravitational-Wave Follow-up in the Third and Fourth Observing Runs: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy

Ido Keinan, Iair Arcavi, D. Andrew Howell +34

We present a summary of gravitational-wave (GW) follow-up using the Las Cumbres Observatory global network of telescopes during the third (O3) and fourth (O4) observing runs of the…

nucl-ex2026

New limits on the Pauli forbidden transitions in 12C nuclei obtained with the complete Borexino dataset

Borexino collaboration, D. Basilico, G. Bellini +70

The Pauli exclusion principle (PEP) was tested for nucleons in nuclei using the Borexino dataset from 2007 to 2021. %the complete Borexino detector data. The approach…

hep-lat2026

Variance reduction in lattice QCD observables via normalizing flows

Ryan Abbott, Denis Boyda, Yang Fu +5

Normalizing flows can be used to construct unbiased, reduced-variance estimators for lattice field theory observables that are defined by a derivative with respect to action parame…

astro-ph.HE2026★ 4 cited

Spectral and photometric variability of SS 433 observed with XRISM and simultaneous optical and near-infrared telescopes

Yusuke Sakai, Shinya Yamada, Yuta Okada +36

We present results from coordinated multiwavelength observations of the SS 433, obtained with XRISM, optical telescopes, and near-infrared camera during 2024 April and 2025 March.…

astro-ph.HE2026

The nearby He-rich superluminous supernova SN 2021bnw during photospheric phases

A. Fiore, A. Kozyreva, L. Yan +40

Aim. We present and interpret the data of the nearby hydrogen-deficient but helium-rich superluminous supernova SN 2021bnw which reached a magnitude of -20.7 at maximum luminosity…

astro-ph.IM2026

Opportunities in AI/ML for the Rubin LSST Dark Energy Science Collaboration

LSST Dark Energy Science Collaboration, Eric Aubourg, Camille Avestruz +63

The Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) will produce unprecedented volumes of heterogeneous astronomical data (images, catalogs, and alerts) that cha…

astro-ph.GA2026

CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations

M. Silvestrini, C. Tortora, V. Busillo +9

Small-scale discrepancies in the standard Lambda cold dark matter paradigm have motivated the exploration of alternative dark matter (DM) models, such as warm dark matter (WDM). We…

astro-ph.HE2026

A multiwavelength view of the nearby Calcium-Strong Transient SN 2025coe in the X-Ray, Near-Infrared, and Radio Wavebands

Sahana Kumar, Raphael Baer-Way, Aravind P. Ravi +18

Calcium-strong transients (CaSTs) are a subclass of faint and rapidly evolving supernovae (SNe) that exhibit strong calcium features and notably weak oxygen features. The small but…

astro-ph.CO2025

Bridging Simulations and EFT: A Hybrid Model of the Lyman-Alpha Forest Field

Roger de Belsunce, Boryana Hadzhiyska, Mikhail M. Ivanov

The Lyman-alpha (Lya) forest is a unique probe of cosmology and the intergalactic medium at high redshift and small scales. The statistical power of the ongoing Dark Energy Spectro…

astro-ph.CO2025

A Fully Photometric Approach to Type Ia Supernova Cosmology in the LSST Era: Host Galaxy Redshifts and Supernova Classification

Ayan Mitra, Richard Kessler, Rebecca C. Chen +9

The upcoming Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) is expected to discover nearly a million Type Ia supernovae (SNeIa), offering an unprecedented oppor…

cond-mat.str-el2025

Refining Heuristic Predictors of Fractional Chern Insulators using Machine Learning

Oriol Mayné i Comas, André Grossi Fonseca, Sachin Vaidya +1

We develop an interpretable, data-driven framework to quantify how single-particle band geometry governs the stability of fractional Chern insulators (FCIs). Using large-scale exac…

astro-ph.HE2025★ 4 cited

Characterization of type Ibn SNe

D. Farias, C. Gall, V. A. Villar +29

Type Ibn supernovae (SNe) are characterized by narrow helium (He I) lines from photons produced by the unshocked circumstellar material (CSM). About 80 SNe Ibn have been discovered…

astro-ph.HE2025

Large Language Model-driven Analysis of General Coordinates Network (GCN) Circulars

Vidushi Sharma, Ronit Agarwala, Judith L. Racusin +9

The General Coordinates Network (GCN) is NASA's time-domain and multimessenger alert system. GCN distributes two data products: automated "Notices" and human-generated "Circulars"…

quant-ph2025

Information Processing in Quantum Thermodynamic Systems: an Autonomous Hamiltonian Approach

Shou-I Tang, Emery Doucet, Akram Touil +2

Extending the quantum formulation of [Phys. Rev. X 3, 041003 (2013)] to a more general setting for studying the thermodynamics of information processing including initial correlati…

astro-ph.HE2025

SN 2021tsz: A luminous, short photospheric phase Type II supernova in a low-metallicity host

R. Dastidar, G. Pignata, N. Dukiya +14

We present the analysis of the luminous Type II Supernova (SN) 2021tsz, which exploded in a low-luminosity galaxy. It reached a peak magnitude of -18.88 0.13 mag in the b…

astro-ph.CO2025★ 2 cited

On the sensitivity of different galaxy properties to warm dark matter

Belén Costanza, Bonny Y. Wang, Francisco Villaescusa-Navarro +7

We study the impact of warm dark matter (WDM) particle mass on galaxy properties using 1,024 state-of-the-art cosmological hydrodynamical simulations from the DREAMS project. We be…

astro-ph.GA2025

How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood

Tal Shpigel, Dylan Folsom, Mariangela Lisanti +3

The dark matter flux in a direct detection experiment depends on its local speed distribution. This distribution has been inferred from simulations of Milky Way-like galaxies, but…

astro-ph.HE2025★ 12 cited

GRB 250702B: Discovery of a Gamma-Ray Burst from a Black Hole Falling into a Star

Eliza Neights, Eric Burns, Chris L. Fryer +52

Gamma-ray bursts are the most luminous electromagnetic events in the universe. Their prompt gamma-ray emission has typical durations between a fraction of a second and several minu…

hep-th2025★ 1 cited

Tripartite Correlation Signal from Multipartite Entanglement of Purification

Ning Bao, Keiichiro Furuya, Joydeep Naskar

We propose a signal for genuine tripartite entanglement in finite-dimensional quantum systems and for holographic systems. We prove that is non-…

hep-ph2025★ 1 cited

Observable Optimization for Precision Theory: Machine Learning Energy Correlators

Arindam Bhattacharya, Katherine Fraser, Matthew D. Schwartz

The practice of collider physics typically involves the marginalization of multi-dimensional collider data to uni-dimensional observables relevant for some physics task. In any cas…

astro-ph.CO2025★ 2 cited

The THESAN project: environmental drivers of Local Group reionization

Yu Zhao, Aaron Smith, Rahul Kannan +5

The timing of cosmic reionization across Local Group (LG) analogues provides insights into their early histories and surrounding large-scale structure. Using the radiation-hydrodyn…

astro-ph.HE2025

Radiative Transfer Modeling of Stripped-Envelope Supernovae. I: A Grid for Ejecta Parameter Inference

S. Karthik Yadavalli, V. Ashley Villar, Abigail Polin +3

We present 1,800 multiwavelength Type Ib/c supernovae light curve models obtained by running the radiation transport code Sedona and varying the mass distribution, velocity profile…