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From the 3 of 30 papers with an AI index.

most citedData Release 1 of the Dark Energy Spectroscopic Instrument

29 citations

21 papers

astro-ph.GA2026

Mixing stochasticity relinquishes evidence for magnetorotational hypernovae

Anmol Aggarwal, Ralph Schoenrich

A recent work claimed by fitting the observed elemental abundance pattern of a halo star with the total yields from single super-/hypernova events that only a magnetorotational hyp…

astro-ph.IM2026

Early Exploration of the Scientific Discovery Space for the Habitable Worlds Observatory

Courtney D. Dressing, Danica Adams, Evelyne Alecian +324

The paper summarizes 70 science cases for the proposed NASA Habitable Worlds Observatory, outlining the observational needs across four scientific pillars and detailing required ca…

astro-ph.IM2026

The Kepler and TESS Asteroseismic Consortia - A Historical Overview

Mikkel N. Lund, Tiago L. Campante

This overview is, in short, about people. About an idea that grew into a consortium, then a community, and finally a way of doing asteroseismology in the space era. The Kepler Aste…

astro-ph.EP2026

Evolution and Observable Properties of Rocky Planet Atmospheres

Marie-Luise Steinmeyer, Lena Noack, Philipp Baumeister +9

This review summarizes current knowledge of rocky exoplanet atmospheres, covering their formation, escape processes, long‑term interaction with the surface and interior, and the ro…

astro-ph.SR20261 cited

Pre-flare and active region plasma flows and structure seen by the short wavelength camera on SOLAR-C/EUVST

James McKevitt, Sarah Matthews, David H. Brooks +20

The paper uses forward modelling of the SOLAR-C/EUVST short‑wavelength camera to show how its high‑resolution EUV spectroscopy can resolve fine plasma flows and individual flux tub…

astro-ph.HE2026

Magnetospheric flows in X-ray pulsars II: Heating, cooling and ionization degree at sub-critical accretion

Alexander A. Mushtukov, Alexander Y. Potekhin, Valery F. Suleimanov +2

Magnetospheric accretion flows in X-ray pulsars shape their spectra, polarization, and variability. We model the thermal balance of the flow enveloping the neutron star magnetosphe…