output
19942026
most citedGATE : a simulation toolkit for PET and SPECT

2.2k citations

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51 papers · 1 filter

astro-ph.GA2025

Observations of AGN-driven feedback: dynamics and ionization of the filaments in M87

Camille Poitras, Marie-Lou Gendron-Marsolais, Valeria Olivares +9

We present a comprehensive kinematic and ionization analysis of the warm ionized filaments ( K) in M87, the central galaxy of the Virgo cluster, using new integral field spec…

cond-mat.mes-hall2025★ 1 cited

Quantum geometry, localization, and topological bounds of spin fluctuations

Carlos Saji, Roberto E. Troncoso

We study how topological crystalline defects--dislocations--reshape the real-space quantum geometric tensor and act as tunable sources of quantum geometry. We show that dislocation…

astro-ph.HE2025★ 1 cited

PSR J0537-6910: Exponential recoveries detected for 12 glitches

E. Zubieta, C. M. Espinoza, D. Antonopoulou +4

Pulsar glitches are unresolved increments of the rotation rate that sometimes trigger an enhancement of the spin-down rate. On occasions, the augmented spin-down decays gradually i…

astro-ph.SR2025★ 2 cited

Interferometric view into RT Pav's long secondary period. binary vs oscillatory convective modes

B. Courtney-Barrer, X. Haubois, P. Wood +6

Long secondary periods (LSPs) occur in about one-third of evolved stars, yet their origin remains unclear. The leading explanations are oscillatory convective modes and a binary co…

astro-ph.IM2025

A review on fundamental bounds and estimators for photometry and astrometry of celestial point sources using array detectors, from first principles

Sebastián Espinosa, Rene A. Mendez, Jorge F. Silva +1

Precise astrometric and photometric measurements of celestial point sources are fundamental to modern astronomy. These measurements, used to determine object positions, motions, an…

astro-ph.HE2025

New and updated timing models for seven young energetic X-ray pulsars, including the Big Glitcher PSR J0537-6910

Wynn C. G. Ho, Lucien Kuiper, Cristobal M. Espinoza +6

We present new timing models and update our previous ones for the rotational evolution of seven young energetic pulsars, including four of the top five in spin-down luminosity Edot…