activity
20242026
collaborators

11 papers

astro-ph.CO2026

Impact and measurability of linear relativistic effects in galaxy surveys

Robin Y. Wen, Henry S. Grasshorn Gebhardt, Olivier Doré

The three-dimensional galaxy power spectrum is a powerful probe of primordial non-Gaussianity (PNG) and additional general relativistic (GR) effects on large scales, which can be c…

astro-ph.GA2026

SPHEREx mapping of diffuse PAH and H II emission in the Galactic plane

Giulia Murgia, Ari J. Cukierman, Brandon S. Hensley +29

We present preliminary SPHEREx maps of diffuse Galactic emission tracing polycyclic aromatic hydrocarbons (PAHs) and ionized hydrogen gas, and we study their relationship across th…

astro-ph.CO2026

Demonstrating the Use of the Spherical Fourier Bessel Basis for Large Scale Clustering Systematics Discovery and Mitigation with eBOSS

Sean Bruton, James R. Cheshire, Olivier Doré +2

The Spherical Fourier-Bessel (SFB) basis, in separating the angular and radial modes of the power spectrum, permits a targeted identification and mitigation of systematics in clust…

astro-ph.GA2026

SPHEREx Wide-Field Infrared Spectral Mapping of Interstellar Ices and Polycyclic Aromatic Hydrocarbons

Joseph L. Hora, Jinyoung K. Noh, Gary J. Melnick +32

We present some of the first infrared spectral maps acquired by SPHEREx. These maps, which to our knowledge are the largest of their type ever compiled in the near-infrared, reveal…

astro-ph.CO2026

Large-scale Modeling of the Observed Power Spectrum Multipoles

Robin Y. Wen, Henry S. Grasshorn Gebhardt, Chen Heinrich +1

Current and upcoming large-scale structure surveys are pushing toward increasingly wide angular coverage, where wide-angle effects (arising from the varying line of sight across th…

astro-ph.IM2025

The SPHEREx Satellite Mission

James J. Bock, Asad M. Aboobaker, Joseph Adamo +111

SPHEREx, a NASA explorer satellite launched on 11 March 2025, is carrying out the first all-sky near-infrared spectral survey. The satellite observes in 102 spectral bands from 0.7…