activity
19972023
most citedThe Early Data Release of the Dark Energy Spectroscopic Instrument

343 citations · 1.7k across the 40 of their papers we have counts for

collaborators

40 papers

astro-ph.CO2023★ 343 cited

The Early Data Release of the Dark Energy Spectroscopic Instrument

DESI Collaboration, A. G. Adame, J. Aguilar +266

The Dark Energy Spectroscopic Instrument (DESI) completed its five-month Survey Validation in May 2021. Spectra of stellar and extragalactic targets from Survey Validation constitu…

astro-ph.CO2023★ 6 cited

Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument

DESI Collaboration, A. G. Adame, J. Aguilar +261

The Dark Energy Spectroscopic Instrument (DESI) was designed to conduct a survey covering 14,000 deg over five years to constrain the cosmic expansion history through precise m…

astro-ph.GA2022★ 55 cited

DESI Observations of the Andromeda Galaxy: Revealing the Immigration History of our Nearest Neighbor

Arjun Dey, Joan R. Najita, S. E. Koposov +45

We present DESI observations of the inner halo of M31, which reveal the kinematics of a recent merger - a galactic immigration event - in exquisite detail. Of the 11,416 sources st…

astro-ph.GA2022★ 27 cited

The impact of very massive stars on the chemical evolution of extremely metal-poor galaxies

S. Goswami, L. Silva, A. Bressan +6

In recent observations of extremely metal-poor low-mass starburst galaxies, almost solar Fe/O ratios are reported, despite N/O ratios consistent with the low metallicity. We invest…

astro-ph.GA2021★ 19 cited

An ALMA view of 11 Dusty Star Forming Galaxies at the peak of Cosmic Star Formation History

L. Pantoni, M. Massardi, A. Lapi +10

We present the ALMA view of 11 main-sequence DSFGs, (sub-)millimeter selected in the GOODS-S field, and spectroscopically confirmed to be at the peak of Cosmic SFH (z = 2-3). Our s…

astro-ph.GA2021★ 25 cited

On the effects of the Initial Mass Function on Galactic chemical enrichment

S. Goswami, A. Slemer, P. Marigo +7

There is mounting evidence that the stellar initial mass function (IMF) could extend much beyond the canonical Mi ~100, Msun limit, but the impact of such hypothesis on the chemica…