activity
20162024
most citedThe DESI Experiment Part I: Science,Targeting, and Survey Design

1.3k citations · 1.5k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2024

Asteroseismology of the Nearby K-Dwarf Draconis using the Keck Planet Finder and TESS

Marc Hon, Daniel Huber, Yaguang Li +76

Asteroseismology of dwarf stars cooler than the Sun is very challenging due to the low amplitudes and rapid timescales of oscillations. Here, we present the asteroseismic detection…

astro-ph.GA2024

VODKA-JWST: A 3.8 kpc dual quasar at cosmic noon in a powerful starburst galaxy with JWST/MIRI IFU

Yu-Ching Chen, Yuzo Ishikawa, Nadia L. Zakamska +12

Dual quasars, two active supermassive black holes at galactic scales, represent crucial objects for studying the impact of galaxy mergers and quasar activity on the star formation…

astro-ph.GA2023

First results from the JWST Early Release Science Program Q3D: Powerful quasar-driven galactic scale outflow at

Andrey Vayner, Nadia L. Zakamska, Yuzo Ishikawa +25

Quasar-driven galactic outflows are a major driver of the evolution of massive galaxies. We report observations of a powerful galactic-scale outflow in a extremely red, intri…

astro-ph.GA20236 cited

Infrared spectroscopic confirmation of z~2 photometrically-selected obscured quasars

Yuzo Ishikawa, Ben Wang, Nadia L. Zakamska +3

The census of obscured quasar populations is incomplete, and remains a major unsolved problem, especially at higher redshifts, where we expect a greater density of galaxy formation…

astro-ph.GA20227 cited

Unresolved z~8 point sources and their impact on the bright end of the galaxy luminosity function

Yuzo Ishikawa, Takahiro Morishita, Massimo Stiavelli +7

The distribution and properties of the first galaxies and quasars are critical pieces of the puzzle in understanding galaxy evolution and cosmic reionization. Previous studies have…

astro-ph.IM2016236 cited

The DESI Experiment Part II: Instrument Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift…