output
20022026
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations

Showing 2025 · astro-ph.EPShow all

6 papers · 2 filters

astro-ph.EP2025

Detecting false positives with PLATO using double-aperture photometry and centroid shifts

F. Gutiérrez-Canales, R. Samadi, A. Birch +6

PLATO will discover exoplanets around Sun-like stars through transit photometry and characterize their host stars using asteroseismology. Since photometry for most PLATO targets wi…

astro-ph.EP2025

The MATISSE view of the inner region of the RY Tau protoplanetary disk

J. S. Martin, J. Kobus, J. Varga +44

The T-Tauri type young stellar object RY Tau exhibits a dust depleted inner cavity characteristic of a transition disk. We constrain the spatial distribution and mineralogy of dust…

astro-ph.EP2025★ 7 cited

MINDS. Strong oxygen depletion in the inner regions of a very low-mass star disk?

Jayatee Kanwar, Inga Kamp, Peter Woitke +10

JWST is discovering a plethora of species in planet-forming disks around very low-mass stars such as C2H2, C6H6, C4H2, CH3 etc. The column densities of these species retrieved from…

astro-ph.EP2025★ 13 cited

The vertical structure of debris discs and the role of disc gravity: A primer using a simplified model

Antranik A. Sefilian, Kaitlin M. Kratter, Mark C. Wyatt +4

Debris discs provide valuable insights into the formation and evolution of exoplanetary systems. Their structures are commonly attributed to planetary perturbations, serving as pro…

astro-ph.EP2025★ 12 cited

Stellar Models Also Limit Exoplanet Atmosphere Studies in Emission

Thomas J. Fauchez, Elsa Ducrot, Benjamin V. Rackham +3

Stellar contamination has long been recognized as a major bottleneck in transmission spectroscopy, limiting our ability to accurately characterize exoplanet atmospheres-particularl…

astro-ph.EP2025★ 27 cited

The PLATO field selection process. II. Characterization of LOPS2, the first long-pointing field

V. Nascimbeni, G. Piotto, J. Cabrera +26

PLAnetary Transits and Oscillations of stars (PLATO) is an ESA M-class mission to be launched by the end of 2026 to discover and characterize transiting planets around bright and n…