activity
20242026
collaborators

7 papers

astro-ph.CO2026

Field-level likelihood for projected fields: Evolved projected fields from initial projected fields

Kevin Hong, Rugved Pund, Anže Slosar

The evolved cosmological matter density field is fully determined by the initial matter density field at fixed cosmological parameters. However, the two-dimensional cosmological pr…

astro-ph.CO2026

Steeling Weak Lensing Source Galaxy Samples against Systematics using Wide Field Spectroscopy

Joseph DeRose, Noah Weaverdyck, Martin White +3

We investigate the cosmological constraining power of combined weak galaxy lensing and galaxy clustering probes, i.e. -point analyses, assuming flexible models for redshi…

astro-ph.IM2026

Linear map-making with LuSEE-Night

Hugo Camacho, Kaja M. Rotermund, Anže Slosar +32

LuSEE-Night is a pathfinder radio telescope on the lunar far side employing four 3-m monopole antennas arranged as two horizontal cross pseudo-dipoles on a rotational stage and sen…

astro-ph.IM2026

Electrical coupling of a horizontal dipole antenna to a dielectric half-space: applications to radio astronomy from the lunar surface

Kaja M. Rotermund, Aritoki Suzuki, Stuart D. Bale +1

The far side of the Moon, shielded from terrestrial radio frequency interference and beyond the influence of Earth's ionosphere, should offer a uniquely quiet environment for radio…

astro-ph.CO2026

Constraints from CMB lensing tomography with projected bispectra

Lea Harscouet, David Alonso, Andrina Nicola +1

We measure the angular power spectrum and bispectrum of the projected overdensity of photometric DESI luminous red galaxies, and its cross-correlation with maps of the Cosmic Micro…

astro-ph.CO2025

DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars

A. G. Adame, J. Aguilar, S. Ahlen +195

We present the measurements and cosmological implications of the galaxy two-point clustering using over 4.7 million unique galaxy and quasar redshifts in the range divi…