Zheng Cai
sancerre.as.arizona.edu
0000-0001-8467-6478
University of California at Santa Cruz
44 papers found
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Cosmic Galaxy-IGM H i Relation at z~ 2--3 Probed in the COSMOS/UltraVISTA 1.6 Deg2 Field
A Ringed Dwarf LINER 1 Galaxy Hosting an Intermediate-mass Black Hole with Large-scale Rotation-like Emission
Mapping the Most Massive Overdensities through Hydrogen (MAMMOTH). II. Discovery of the Extremely Massive Overdensity BOSS1441 at z= 2.32
Constraining C iii] Emission in a Sample of Five Luminous z= 5.7 Galaxies
Deep Learning of Quasar Spectra to Discover and Characterize Damped Lya Systems
Discovery of an Enormous Ly$α$ Nebula in a Massive Galaxy Overdensity at z= 2.3
Scientific Performance Analysis of the SYZ Telescope Design versus the RC Telescope Design
Imaging the Most Massive Galaxy Overdensities at z= 2.2: The Morphology-Density Relation at High Redshift
Probing the Metal Enrichment of the Intergalactic Medium at z= 5--6 Using the Hubble Space Telescope
Mapping the Most Massive Overdensity Through Hydrogen (Mammoth). I. Methodology
Imaging a Massive Galaxy Overdensity at z= 2.3: The Morphology-Density Relation at High Redshift
Ly$α$ EMITTER GALAXIES AT Z~ 2.8 IN THE EXTENDED CHANDRA DEEP FIELD SOUTH. I. TRACING THE LARGE-SCALE STRUCTURE VIA Ly$α$ IMAGING
LBT/LUCI SPECTROSCOPIC OBSERVATIONS OFz≃7 Galaxies GALAXIES
DISCOVERY OF EIGHTz∼ 6 QUASARS IN THE SLOAN DIGITAL SKY SURVEY OVERLAP REGIONS
CONSTRAINING VERY HIGH MASS POPULATION III STARS THROUGH He II EMISSION IN GALAXY BDF-521 ATz= 7.01
LBT/LUCI SPECTROSCOPIC OBSERVATIONS OF Z≃ 7 Galaxies GALAXIES
Constraining very high mass population III stars through He II emission in galaxy BDF-521 at z= 7.01
Cosmic Structure Formation: From First Star to Large-scale Filamentary Structure
An ULTRA-LUMINOUS QUASAR AT Z= 5.363 WITH a TEN BILLION SOLAR MASS BLACK HOLE AND a METAL-RICH DLA AT Z~ 5
Discovery of eight z~ 6 quasars in the sloan digital sky survey overlap regions
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