activity
20242026
collaborators

7 papers

astro-ph.SR2026

Magnetic fields in Massive Star-Forming Regions (MagMaR). VIII. Magnetic field overrun by gravity in GGD 27's accretion streamers

M. Fernández-López, J. A. López-Vázquez, J. M. Girart +20

Context. Accretion streamers connected to protostellar disks and/or envelopes are thought to transport material across several thousand of au. Whether the motions of the gas compri…

astro-ph.GA2026

The new era of Lyman alpha emitters (LAEs): Efficiency in the selection criteria

P. Layana-Astudillo, I. Laferte-Urrutia, L. Guaita +6

The ODIN survey has detected thousands of Lyman-alpha emitting galaxies across seven sky fields, covering nearly one hundred square degrees. One of these regions is the SHELA field…

math.RT2026

Interval Multiplicities of Persistence Modules

Hideto Asashiba, Enhao Liu

For any persistence module over a finite poset , and any interval of , we give a formula for the multiplicity of the interval module $V_I…

math.RT2026

Interval Replacements of Persistence Modules

Hideto Asashiba, Etienne Gauthier, Enhao Liu

We define two notions. The first one is a for a finite poset that assigns each interval subposet to an order-preserving map $ξ_I…

astro-ph.CO2026

Euclid preparation. LXXXV. Toward a DR1 application of higher-order weak lensing statistics

Euclid Collaboration, S. Vinciguerra, F. Bouchè +284

This is the second paper in the HOWLS (higher-order weak lensing statistics) series exploring the usage of non-Gaussian statistics for cosmology inference within Euclid. With respe…

astro-ph.CO2025

Mitigation of nonlinear galaxy bias with a theoretical-error likelihood

Abdias Aires, Nickolas Kokron, Rogerio Rosenfeld +2

Stage-IV galaxy surveys will measure correlations at small cosmological scales with high signal-to-noise ratio. One of the main challenges of extracting information from small scal…