activity
20062026
most citedARCADE 2 Measurement of the Extra-Galactic Sky Temperature at 3-90 GHz

338 citations · 1.5k across the 31 of their papers we have counts for

collaborators

33 papers

astro-ph.CO2026

FOSSIL: A future mission for CMB spectral distortion measurements

N. Aghanim, B. Maffei, J. Aumont +96

We present FOSSIL, a proposed space mission which is designed to deliver unprecedented absolute spectroscopic measurements of the sky intensity over a broad frequency range (50GHz…

astro-ph.CO2026

Peering Beyond the Veil of Last Scattering: A View of the Universe with CMB Spectral Distortions

Bryce Cyr, Nabila Aghanim, Ethan Baker +37

The frequency spectrum of the cosmic microwave background is the most precise blackbody ever measured in nature, with deviations constrained at the level of almost one part per mil…

astro-ph.CO2023★ 5 cited

Improving Photometric Redshift Estimation for Cosmology with LSST using Bayesian Neural Networks

Evan Jones, Tuan Do, Bernie Boscoe +3

We present results exploring the role that probabilistic deep learning models can play in cosmology from large-scale astronomical surveys through photometric redshift (photo-z) est…

astro-ph.CO2023★ 7 cited

Diffuse Sources, Clustering and the Excess Anisotropy of the Radio Synchrotron Background

F. J. Cowie, A. R. Offringa, B. K. Gehlot +4

We present the largest low frequency (120~MHz) arcminute resolution image of the radio synchrotron background (RSB) to date, and its corresponding angular power spectrum of anisotr…

astro-ph.CO2022★ 31 cited

The Second Radio Synchrotron Background Workshop: Conference Summary and Report

J. Singal, N. Fornengo, M. Regis +24

We summarize the second radio synchrotron background workshop, which took place June 15-17, 2022 in Barolo, Italy. This meeting was convened because available measurements of the d…

astro-ph.CO2022★ 26 cited

Can the Distance-Redshift Relation Be Determined from Correlations Between Luminosities?

V. Petrosian, J. Singal, S. Mutchnick

We explore whether an independent determination of the distance-redshift relation, and hence cosmological model parameters, can be obtained from the apparent correlations between t…