activity
20162023
most citedThe Early Data Release of the Dark Energy Spectroscopic Instrument

343 citations · 906 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.GA2023★ 7 cited

A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Discovers an Overdensity around a Metal Absorption-selected Galaxy at

Yunjing Wu, Feige Wang, Zheng Cai +27

The launch of opens a new window for studying the connection between metal-line absorbers and galaxies at the end of the Epoch of Reionization (EoR). Previous studies…

astro-ph.SR2023

GTC Follow-up Observations of Very Metal-Poor Star Candidates from DESI

Carlos Allende Prieto, David S. Aguado, Jonay I. González Hernández +48

The observations from the Dark Energy Spectroscopic Instrument (DESI) will significantly increase the numbers of known extremely metal-poor stars by a factor of ~ 10, improving the…

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.GA2023★ 26 cited

Detecting and Characterizing Mg II absorption in DESI Survey Validation Quasar Spectra

Lucas Napolitano, Agnesh Pandey, Adam D. Myers +33

We present findings of the detection of Magnesium II (Mg II, λ = 2796, 2803 Å) absorbers from the early data release of the Dark Energy Spectroscopic Instrument (DESI). DESI is pro…

astro-ph.GA2023★ 91 cited

A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z=6.61 Quasar

Feige Wang, Jinyi Yang, Joseph F. Hennawi +56

We present the first results from the JWST ASPIRE program (A SPectroscopic survey of biased halos In the Reionization Era). This program represents an imaging and spectroscopic sur…

astro-ph.GA2023★ 77 cited

A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of Quasars Using JWST

Jinyi Yang, Feige Wang, Xiaohui Fan +53

Studies of rest-frame optical emission in quasars at have historically been limited by the wavelengths accessible by ground-based telescopes. The James Webb Space Telescope (…

astro-ph.GA2023

DESI survey validation data in the COSMOS/HSC field: Cool gas trace main sequence star-forming galaxies at the cosmic noon

Siwei Zou, Linhua Jiang, Zheng Cai +23

We present the first result in exploring the gaseous halo and galaxy correlation using the Dark Energy Spectroscopic Instrument (DESI) survey validation data in the Cosmic Evolutio…

astro-ph.GA2022★ 50 cited

The Mass-Metallicity Relation of Dwarf Galaxies at Cosmic Noon from JWST Observations

Mingyu Li, Zheng Cai, Fuyan Bian +13

We present a study of the mass-metallicity relation (MZR) of 51 dwarf galaxies () at from the Abell 2744 and SMACS J0723-3732…

astro-ph.GA2022★ 20 cited

Metal-Enriched Neutral Gas Reservoir around a Strongly-lensed, Low-mass Galaxy at Identified by JWST/NIRISS and VLT/MUSE

Xiaojing Lin, Zheng Cai, Siwei Zou +19

Direct observations of low-mass, low-metallicity galaxies at provide an indispensable opportunity for detailed inspection of the ionization radiation, gas flow, and met…

astro-ph.GA2022★ 91 cited

The DESI Survey Validation: Results from Visual Inspection of the Quasar Survey Spectra

David M. Alexander, Tamara M. Davis, E. Chaussidon +69

A key component of the Dark Energy Spectroscopic Instrument (DESI) survey validation (SV) is a detailed visual inspection (VI) of the optical spectroscopic data to quantify key sur…

astro-ph.GA2022★ 45 cited

The Identification of a Dusty Multiarm Spiral Galaxy at with JWST and ALMA

Yunjing Wu, Zheng Cai, Fengwu Sun +13

Spiral arms serve crucial purposes in star formation and galaxy evolution. In this paper, we report the identification of A2744-DSG-, a dusty, multiarm spiral galaxy at $z=3.05…

astro-ph.GA2021★ 39 cited

Metallicity in Quasar Broad Line Regions at Redshift 6

Shu Wang, Linhua Jiang, Yue Shen +10

Broad line regions (BLRs) in high-redshift quasars provide crucial information of chemical enrichment in the early universe. Here we present a study of BLR metallicities in 33 quas…

astro-ph.GA2020★ 3 cited

Discovery of a damped Ly galaxy at z 3 towards the quasar SDSS J011852+040644

Ravi Joshi, Michele Fumagalli, Raghunathan Srianand +11

We report the detection of the host galaxy of a damped Ly system (DLA) with log N(HI) = at towards the background quasar SDSS…

astro-ph.GA2020★ 21 cited

Strong Mg II and Fe II Absorbers at 2.2 < z < 6.0

Siwei Zou, Linhua Jiang, Yue Shen +13

We present a study of strong intervening absorption systems in the near-IR spectra of 31 luminous quasars at . The quasar spectra were obtained with {\it Gemini} GNIRS that…

astro-ph.GA2020★ 7 cited

A Carbon-enhanced Lyman Limit System: Signature of the First Generation of Stars?

Siwei Zou, Patrick Petitjean, Pasquier Noterdaeme +4

We present the study of a Lyman limit system (LLS) at = 1.5441 towards quasar J134122.50+185213.9 observed with VLT X-shooter. This is a very peculiar system with str…

astro-ph.GA2017★ 26 cited

Near Infrared spectroscopic observations of high redshift C~{\sc i} absorbers

Siwei Zou, Patrick Petitjean, Pasquier Noterdaeme +5

We study a sample of 17 z>1.5 absorbers selected based on the presence of strong CI absorption lines in SDSS spectra and observed with the ESO-VLT spectrograph X-shooter. We derive…

astro-ph.GA2016★ 24 cited

A ghostly damped Ly system revealed by metal absorption lines

Hassan Fathivavsari, Patrick Petitjean, Siwei Zou +4

We report the discovery of the first 'ghostly' damped Ly absorption system (DLA), which is identified by the presence of absorption from strong low-ion species at $z_{\rm abs}=1…

astro-ph.CO2016★ 30 cited

The X-ray luminosity-temperature relation of a complete sample of low-mass galaxy clusters

Siwei Zou, B. J. Maughan, P. A. Giles +4

We present \Chandra\ observations of 23 galaxy groups and low-mass galaxy clusters at with a median temperature of ~2keV. The sample is a statistically complete flux-…