activity
20142022
most citedThe DESI Experiment Part I: Science,Targeting, and Survey Design

1.3k citations · 1.7k across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2024

The DESI Early Data Release White Dwarf Catalogue

Christopher J. Manser, Paula Izquierdo, Boris T. Gänsicke +51

The Early Data Release (EDR) of the Dark Energy Spectroscopic Instrument (DESI) comprises spectroscopy obtained from 2020 December 14 to 2021 June 10. White dwarfs were targeted by…

astro-ph.SR202323 cited

DAHe white dwarfs from the DESI survey

Christopher J. Manser, Boris T. Gänsicke, Keith Inight +16

A new class of white dwarfs, dubbed DAHe, that present Zeeman-split Balmer lines in emission has recently emerged. However, the physical origin of these emission lines remains uncl…

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…

astro-ph.IM20161.3k cited

The DESI Experiment Part I: Science,Targeting, and Survey Design

DESI Collaboration, Amir Aghamousa, Jessica Aguilar +290

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

astro-ph.GA2016112 cited

Incidence of WISE-Selected Obscured AGNs in Major Mergers and Interactions from the SDSS

Madalyn E. Weston, Daniel H. McIntosh, Mark Brodwin +4

We use the Wide-field Infrared Survey Explorer (WISE) and the Sloan Digital Sky Survey (SDSS) to confirm a connection between dust-obscured active galactic nuclei (AGNs) and galaxy…

astro-ph.GA201411 cited

The Size Evolution of Elliptical Galaxies

Lizhi Xie, Qi Guo, Andrew P. Cooper +3

Recent work has suggested that the amplitude of the size mass relation of massive early type galaxies evolves with redshift. Here we use a semi-analytical galaxy formation model to…