output
19912026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

8,802 papers

astro-ph.HE2026

Spectral-Timing Evolution of the Black Hole X-ray Binary LMC X-3: An XPoSat View

Sayantan Bhattacharya, Aman Kaushik, Sudip Bhattacharyya

LMC X-3 is a persistent black hole high-mass X-ray binary and serves as an important laboratory for studying accretion disk evolution across different spectral states. We present a…

cond-mat.soft2026★ 7 cited

Compression-controlled dynamic buckling in thin soft sheets

Harsh Jain, Shankar Ghosh, Kirti Chandra Sahu

We investigate experimentally the dynamic phase transition from compressed to buckled phases for thin sheets of rubber. We find that the rubber strips enter a highly compressed, me…

astro-ph.GA2026

Finding the evolutionary link between ULIRGs and radio galaxies

Ayisha Fida, Sumana Nandi, Mousumi Das +4

Ultraluminous infrared galaxies (ULIRGs) are the remnants of the major mergers of gas-rich galaxies. They are dusty systems and are extremely luminous in the infrared. Both starbur…

astro-ph.HE2026

Transmutation Timescales for Dark Matter Induced Collapse of Compact Stars into Black Holes

H. A. Adarsha, Chandrachur Chakraborty, Sudip Bhattacharyya

Ultra-heavy asymmetric dark matter (DM) particles captured by compact stars can thermalize, self-gravitate, and collapse to form an endoparasitic black hole (EBH), whose subsequent…

cs.IT2026

Authentication over Arbitrarily Varying Channels with Causal Adversaries

Mayank Bakshi, Vinod M. Prabhakaran, Bikash Kumar Dey +1

We study authentication over a discrete memoryless arbitrarily varying channel (AVC) in which the adversary selects the channel state causally based on past channel outputs. We pro…

astro-ph.CO2026

Filaments within filaments: unraveling the hierarchy of the cosmic web

Saee Dhawalikar, Aseem Paranjape, Shadab Alam

Cosmic filaments are the most striking feature of the hierarchical cosmic web. Yet, their own sub-structure remains unexplored, unlike the well-known, universal halo/sub-halo hiera…

astro-ph.HE2026

Tilted thin accretion disks in the full Kerr spacetime and their implications

K. S. Sruthy, Chandrachur Chakraborty, Sudip Bhattacharyya

We derive a steady-state warped-disk equation in the full Kerr spacetime to study the tilt dynamics of a thin, viscous accretion disk around a spinning collapsed object. The formul…

astro-ph.SR2026

A Quiet Host in an Active Planet-Forming Disk: Optical Spectroscopy of WISPIT 2

C. Swastik, M. Bestha, L. S. Sonith +11

WISPIT 2 is a young pre-main-sequence star hosting a multi-ringed transition disk and two directly imaged protoplanets, including the accreting WISPIT 2b, making it the closest kno…

astro-ph.IM2026

Enhancing the Cherenkov Telescope Array Observatory high-level performance through an event-type-based analysis

Juan Bernete, Silvia García-Soto, Tarek Hassan +4

The analysis traditionally employed by Imaging Atmospheric Cherenkov Telescopes involves optimizing quality cuts to select a sub-sample of high-quality events. These events are use…

astro-ph.HE2026

The SPOTLIGHT Pulsar Search Pipeline: A GPU-Accelerated FFT Approach

Jyotirmoy Das, Jayanta Roy, Nishant Pradeep Deo +20

We present the pulsar search component of SPOTLIGHT (Survey for sPoradic radiO bursTs via a commensaL multI-beam Gpu-powered Hpc at the gmrT), a GPU-accelerated commensal backend o…

astro-ph.IM2026

The Deep Learning Cosmic Ray Energy Reconstruction Pipeline for the GRAPES-3 Experiment

Sambit Sarkar, Mansi Talwar, Pravata K. Mohanty

The mass independent energy reconstruction of cosmic rays is crucial for understanding their origin, acceleration, and propagation. Precise measurement of the primary energy can al…

astro-ph.IM2026

Machine learning pipeline for identifying tracks of muons and hadrons at GRAPES-3 muon telescope

Mansi Talwar, Sambit Sarkar, Pravata K. Mohanty

The GRAPES-3 experiment is a ground-based extensive air shower array which consists of approximately closely packed plastic scintillator detectors and a large area muon teles…

astro-ph.SR2026

The Variability of Radio Stars

Laura N. Driessen, Alex Andersson, Joseph R. Callingham +6

Stellar radio emission is highly variable with stellar flares lasting from milliseconds to hours. For some stars, their flares or bursts can repeat once every couple of hours, whil…

astro-ph.GA2026

Radio emission from ultra-diffuse galaxies residing in galaxy clusters

Dharam V. Lal, Jeyasiona Murugesh

Ultra-diffuse galaxies (UDGs), defined by their extremely low surface brightness (-band mag arcsec) and large effective radii (3--10 arcsec), remain one of…

cond-mat.mes-hall2026

Superconducting cavity probes sliding ferroelectricity in small-angle twisted WSe

Krishnendu Maji, Supriya Mandal, Sriram H. +8

Ferroelectricity is a property of materials that exhibit spontaneous charge polarization. Ferroelectricity in 2D materials is interesting because of their applications in memory de…

astro-ph.GA2026

Star Formation at the Periphery of a Molecular Superbubble: The Case of G12.79+0.43

Arun Seshadri, Veena V. S., Sarita Vig +1

We present a multiwavelength investigation of the molecular cloud complex G12.79+0.43, which extends over on the sky. Several infrared- and radio-bright regions are arran…

cond-mat.str-el2026

Tunable Chaos in the Finite Mean SYK Model

Arkaprava Mukherjee, Sumilan Banerjee, Sandip P. Trivedi +1

The complex Sachdev-Ye-Kitaev (SYK) model, featuring fermions with all-to-all interactions, serves as a dual paradigm for understanding non-Fermi liquid behavior and the holographi…

astro-ph.SR2026

Summary of the First Year of the Space Weather Around Young Suns Program: 900 Hours of Low-frequency Radio and Optical Data Dedicated to Young, Solar-type Stars

Ivey Davis, Gregg Hallinan, Nikita Kosogorov +51

The Space Weather Around Young Suns (SWAYS) program was introduced in \citet{Davis2025} as a multi-wavelength monitoring program for studying the activity and particle environments…

astro-ph.CO2026

Pantheon+ supernovae corrected for progenitor age indicate the universe is decelerating

Animesh Sah, Mohamed Rameez, Subir Sarkar

We examine the impact of progenitor age-dependent luminosity evolution of Type Ia supernovae on a cosmographic measurement of the deceleration parameter . Our recent redshift…

astro-ph.HE2026

Constraining Orbital Eccentricity of a Supermassive Black Hole Binary Candidate PKS 2131-0211

Avinash Kumar Paladi, A. Gopakumar, Sushmita Agarwal +1

A detailed analysis of the decades-long radio light curve of blazar PKS 2131-021 showed epochs of sinusoidal variations in the radio flux density time-series as detailed in O'Neill…

astro-ph.GA2026★ 1 cited

uGMRT and MeerKAT observation of RXCJ0232-4420: a quiet cluster with a giant radio halo

Pralay Biswas, Ramananda Santra, Ruta Kale +1

Giant radio halos are the Mpc-scale extended sources associated with the merging clusters, while the mini-halos are preferentially associated with cool-core clusters. Both trace th…

cond-mat.supr-con2026

Phase diagram of the vortex state in an amorphous Re6Zr thin film exhibiting inverse melting

Pritam Das, Subhamita Sengupta, Anjan Jana +6

In Type II superconductors, the vortex lattice can exhibit "inverse melting," transitioning from a liquid to a crystalline solid as temperature increases. While recently observed v…

astro-ph.HE2026

A NICER and AstroSat view of the neutron star low-mass X-ray binary 1A 1246-588

Vaidehi Poojyam, Vikas Mistry, Yash Bhargava +2

Neutron star (NS) low-mass X-ray binary (LMXB) systems depict a variety of X-ray spectral and timing features, which can be useful to probe the accretion-ejection mechanism in the…

gr-qc2026★ 2 cited

GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1839

GW240925 and GW250207 are two loud gravitational-wave signals from binary black hole coalescences observed with network signal-to-noise ratios and , respectively…