activity
20092026
most citedFermi Large Area Telescope Second Source Catalog

1.3k citations · 38.8k across the 391 of their papers we have counts for

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Showing 2024Show all

30 papers · 1 filter

astro-ph.IM2024

DarkNESS: developing a skipper-CCD instrument to search for Dark Matter from Low Earth Orbit

Phoenix Alpine, Samriddhi Bhatia, Fernando Chierchie +8

The DarkNESS (Dark Matter Nano-satellite Equipped with Skipper Sensors) mission aims to deploy a skipper-CCD CubeSat Observatory to search for dark matter (DM) from Low Earth Orbit…

astro-ph.CO2024

Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak Lensing

S. Bocquet, S. Grandis, E. Krause +216

Cosmic shear, galaxy clustering, and the abundance of massive halos each probe the large-scale structure of the Universe in complementary ways. We present cosmological constraints…

astro-ph.CO2024★ 11 cited

Dark Energy Survey Year 3: Blue Shear

J. McCullough, A. Amon, E. Legnani +115

Modeling the intrinsic alignment (IA) of galaxies poses a challenge to weak lensing analyses. The Dark Energy Survey is expected to be less impacted by IA when limited to blue, sta…

astro-ph.CO2024★ 23 cited

SENSEI at SNOLAB: Single-Electron Event Rate and Implications for Dark Matter

Itay M. Bloch, Ana M. Botti, Mariano Cababie +27

We present results from data acquired by the SENSEI experiment at SNOLAB after a major upgrade in May 2023, which includes deploying 16 new sensors and replacing the copper trays t…

astro-ph.GA2024

Eridanus III and DELVE 1: Carbon-rich Primordial Star Clusters or the Smallest Dwarf Galaxies?

Joshua D. Simon, Ting S. Li, Alexander P. Ji +8

We present spectroscopy of the ultra-faint Milky Way satellites Eridanus III (Eri III) and DELVE 1. We identify eight member stars in each satellite and place non-constraining uppe…

astro-ph.IM2024★ 3 cited

Cherenkov Photon Background for Low-Noise Silicon Detectors in Space

Manuel E. Gaido, Javier Tiffenberg, Alex Drlica-Wagner +6

Future space observatories dedicated to direct imaging and spectroscopy of extra-solar planets will require ultra-low-noise detectors that are sensitive over a broad range of wavel…