activity
20242026
collaborators

10 papers

astro-ph.CO2026

Control variates from Eulerian and Lagrangian perturbation theory: Application to the bispectrum

Nickolas Kokron, Shi-Fan Chen

Control variates have seen recent interest as a powerful technique to reduce the variance of summary statistics measured from costly cosmological -body simulations. Of particula…

astro-ph.CO2026

The Squeezed Bispectrum from CHIME HI Emission and Planck CMB Lensing: Current Sensitivity and Forecasts

CHIME Collaboration, Arnab Chakraborty, Matt Dobbs +18

Line intensity mapping using atomic hydrogen (HI) has the potential to efficiently map large volumes of the universe if the signal can be successfully separated from overwhelmingly…

astro-ph.CO2025

Direct correlation of line intensity mapping and CMB lensing from evolution along the lightcone

Delon Shen, Nickolas Kokron, Emmanuel Schaan

Line intensity mapping (LIM) promises to probe previously inaccessible corners of the faint and high-redshift universe. However, confusion with bright foregrounds is a major challe…

astro-ph.GA2025

Cross-correlation of Luminous Red Galaxies with ML-selected AGN in HSC-SSP III: HOD Parameters for Type I and Type II Quasars

Rodrigo Córdova Rosado, Andy D. Goulding, Jenny E. Greene +4

Understanding the dark matter (DM) halo environment in which galaxies that host active galactic nuclei (AGN) reside is a window into the nature of supermassive black hole (SMBH) ac…

astro-ph.CO2025

How do uncertainties in galaxy formation physics impact field-level galaxy bias?

Mahlet Shiferaw, Nickolas Kokron, Risa H. Wechsler

Our ability to extract cosmological information from galaxy surveys is limited by uncertainties in the galaxy-dark matter halo relationship for a given galaxy population, which are…

astro-ph.CO2025

On the contributions of extragalactic CO emission lines to ground-based CMB observations

Nickolas Kokron, José Luis Bernal, Jo Dunkley

We investigate the potential of CO rotational lines at redshifts being an appreciable source of extragalactic foreground anisotropies in the cosmic microwave background…