32 papers found
Refreshing results…
SMM J04135+10277: a distant QSO–starburst system caught by ALMA
ALMA Reveals a Gas-rich, Maximum Starburst in the Hyperluminous, Dust-obscured Quasar W0533–3401 at z ∼ 2.9
Color Dependence of Clustering of Massive Galaxies at 0.5 ≤z ≤2.5: Similar Spatial Distributions between Green Valley Galaxies and AGNs
SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). II. Structural Properties and Near-infrared Morphologies of Faint Submillimeter Galaxies
Non-legalistic activism from the social margin: Informal workers with pneumoconiosis in Shenzhen
‘Classes of Labour’ at the Margins of Global Commodity Chains in India and China: ‘Classes of Labour’ at the Margins of Global Commodity Chains
ALMA Detections of CO Emission in the Most Luminous, Heavily Dust-obscured Quasars atz> 3
The Spectral Energy Distribution of the Hyperluminous, Hot Dust-obscured Galaxy W2246–0526
Corrigendum to ‘Metapristone suppresses non-small cell lung cancer proliferation and metastasis via modulating RAS/RAF/MEK/MAPK signaling pathway’ [Biomed. Pharmacother. 90 (2017) 437-445]
The SCUBA-2 850μm Follow-up ofWISE-selected, Luminous Dust-obscured Quasars
Compact star forming galaxies as the progenitors of compact quiescent galaxies: Clustering result
Infrared Spectral Energy Distribution Decomposition Ofwise-Selected, Hyperluminous Hot Dust-Obscured Galaxies
The Most Luminous Heavily Obscured Quasars Have a High Merger Fraction: Morphological Study Ofwise-Selected Hot Dust-Obscured Galaxies
The SPATIALLY RESOLVED NUV–rCOLOR OF LOCAL STAR-FORMING GALAXIES AND CLUES FOR QUENCHING
miR-663 overexpression induced by endoplasmic reticulum stress modulates hepatocellular carcinoma cell apoptosis via transforming growth factor beta 1
Clustering of massive compact galaxies at 1 ≤ z ≤ 3 in CANDELS/3D-HST
Physical properties of distant red galaxies in the COSMOS/UltraVISTA field
PHYSICAL PROPERTIES OF COMPACT STAR-FORMING GALAXIES ATz∼ 2–3
From Outside-In to Inside-Out: Galaxy Assembly Mode Depends on Stellar Mass
What drives the M*-SFR relation turning over at high masses? The role of bulges
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