Identifiers
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name variant
Jingwen Wu
0.60 · backfill
Papers (41)
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Rethinking Visual Neglect: Steering via Context-Preference for MLLM Hallucination Mitigation
cs.CL · 2026 · author #1
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Compact, AGN-hosting Dwarf Galaxies with "Little Red Dots"-like SEDs in the Local Universe
astro-ph.GA · 2026 · author #3
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Hessian-based photometric substructure as an evolutionary tracer of OB cluster candidates in M31
astro-ph.GA · 2026 · author #3
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An inverted infall profile for the collapse of the massive star-forming IRDC SDC335.579-0.292
astro-ph.GA · 2026 · author #6
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Status and perspectives of the CRAFTS extra-galactic HI survey
astro-ph.GA · 2019 · author #2
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Super-Eddington Accretion in the WISE-Selected Extremely Luminous Infrared Galaxy W2246-0526
astro-ph.GA · 2018 · author #4
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Inflow Motions associated with High-mass Protostellar Objects
astro-ph.GA · 2018 · author #5
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Re-visiting the extended Schmidt law: the important role of existing stars in regulating star formation
astro-ph.GA · 2018 · author #12
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Overdensities of SMGs around WISE-selected, ultra-luminous, high-redshift AGN
astro-ph.GA · 2017 · author #10
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The role of the most luminous, obscured AGN in galaxy assembly at z~2
astro-ph.GA · 2017 · author #16
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Eddington-Limited Accretion in z~2 WISE-selected Hot, Dust-Obscured Galaxies
astro-ph.GA · 2017 · author #1
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A Catalog of Low-Mass Star-Forming Cores Observed with SHARC-II at 350 microns
astro-ph.GA · 2016 · author #7
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SMA observations of the W3(OH) complex: Dynamical differentiation between W3(H$_2$O) and W3(OH)
astro-ph.SR · 2015 · author #3
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Results from the Wide-field Infrared Survey Explorer (WISE) Future Uses Session at the WISE at 5 Meeting
astro-ph.IM · 2015 · author #52
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Submillimetre observations of WISE/radio-selected AGN and their environments
astro-ph.GA · 2015 · author #13
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SMA Observations of W3(OH) Complex: Physical and Chemical Differentiation between W3(H$_2$O) and W3(OH)
astro-ph.SR · 2015 · author #3
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The Most Luminous Galaxies Discovered by WISE
astro-ph.GA · 2014 · author #3
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Half of the Most Luminous Quasars May Be Obscured: Investigating the Nature of WISE-Selected Hot, Dust-Obscured Galaxies
astro-ph.GA · 2014 · author #5
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Submillimetre observations of WISE-selected high-redshift, luminous, dusty galaxies
astro-ph.GA · 2014 · author #8
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Interferometric Follow-Up of WISE Hyper-Luminous Hot, Dust-Obscured Galaxies
astro-ph.GA · 2014 · author #1
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WISE Discovery of Hyper Luminous Galaxies at z=2-4 and Their Implications for Galaxy and AGN Evolution
astro-ph.CO · 2013 · author #3
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WISE detections of known QSOs at redshifts greater than six
astro-ph.CO · 2013 · author #11
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WISE J233237.05-505643.5: a Double-Peaked Broad-Lined AGN with Spiral-Shaped Radio Morphology
astro-ph.CO · 2013 · author #12
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Competitive accretion in the protocluster G10.6-0.4?
astro-ph.SR · 2012 · author #3
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Mid-Infrared Selection of Active Galactic Nuclei with the Wide-Field Infrared Survey Explorer. II. Properties of WISE-Selected Active Galactic Nuclei in the NDWFS Bo\"otes Field
astro-ph.CO · 2012 · author #13
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Spitzer Photometry of WISE-Selected Brown Dwarf and Hyper-Luminous Infrared Galaxy Candidates
astro-ph.SR · 2012 · author #25
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Submillimeter Follow-up of WISE-Selected Hyperluminous Galaxies
astro-ph.CO · 2012 · author #1
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The First Hyper-Luminous Infrared Galaxy Discovered by WISE
astro-ph.CO · 2012 · author #2
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A New Population of High Redshift, Dusty Lyman-Alpha Emitters and Blobs Discovered by WISE
astro-ph.CO · 2012 · author #14
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The Infrared Properties of Sources Matched in the WISE all-sky and Herschel-ATLAS Surveys
astro-ph.CO · 2012 · author #36
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Evidence for Inflow in High-Mass Star-Forming Clumps
astro-ph.SR · 2011 · author #3
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The Physical Properties of High-Mass Star-Forming Clumps: A Systematic Comparison of Molecular Tracers
astro-ph.GA · 2011 · author #3
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The Decrease of Specific Angular Momentum and the Hot Toroid Formation: The Massive Clump G10.6-0.4
astro-ph.SR · 2010 · author #5
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The Properties of Massive, Dense, Clumps: Mapping Surveys of HCN and CS
astro-ph.GA · 2010 · author #1
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Millimetre observations of a sample of high-redshift obscured quasars
astro-ph.GA · 2009 · author #6
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Submillimeter Array Observations of the Molecular Outflow in High-mass Star-forming Region G240.31+0.07
astro-ph.GA · 2009 · author #3
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The Spitzer c2d Survey of Nearby Dense Cores. V. Discovery of a VeLLO in the "Starless" Dense Core L328
astro-ph · 2008 · author #8
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Molecular Line Observations of the Small Protostellar Group L1251B
astro-ph · 2007 · author #5
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SHARC-II Mapping of Spitzer c2d Small Clouds and Cores
astro-ph · 2006 · author #1
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Connecting Dense Gas Tracers of Star Formation in our Galaxy to High-z Star Formation
astro-ph · 2005 · author #1
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Indications of Inflow Motions in Regions Forming Massive Stars
astro-ph · 2003 · author #1
Mentions
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1511.08325
#3 · backfill · confidence 0.70
Jingwen Wu
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1505.01923
#52 · backfill · confidence 0.70
Jingwen Wu
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1503.02561
#13 · backfill · confidence 0.70
Jingwen Wu
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1502.04467
#3 · backfill · confidence 0.70
Jingwen Wu
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1410.1751
#3 · backfill · confidence 0.70
Jingwen Wu
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1408.1092
#5 · backfill · confidence 0.70
Jingwen Wu
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1406.2506
#8 · backfill · confidence 0.70
Jingwen Wu
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1405.1147
#1 · backfill · confidence 0.70
Jingwen Wu
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1311.0120
#3 · backfill · confidence 0.70
Jingwen Wu
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1310.2301
#11 · backfill · confidence 0.70
Jingwen Wu
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1310.2257
#12 · backfill · confidence 0.70
Jingwen Wu
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2605.27993
#1 · arxiv_oai · confidence 0.70
Jingwen Wu
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1211.5206
#3 · backfill · confidence 0.70
Jingwen Wu
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1209.6055
#13 · backfill · confidence 0.70
Jingwen Wu
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1209.1855
#25 · backfill · confidence 0.70
Jingwen Wu
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1208.5518
#1 · backfill · confidence 0.70
Jingwen Wu
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1208.5517
#2 · backfill · confidence 0.70
Jingwen Wu
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1205.4030
#14 · backfill · confidence 0.70
Jingwen Wu
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1204.2020
#36 · backfill · confidence 0.70
Jingwen Wu
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1107.5343
#3 · backfill · confidence 0.70
Jingwen Wu
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1104.3899
#3 · backfill · confidence 0.70
Jingwen Wu
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1010.2255
#5 · backfill · confidence 0.70
Jingwen Wu
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1004.0398
#1 · backfill · confidence 0.70
Jingwen Wu
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0910.1099
#6 · backfill · confidence 0.70
Jingwen Wu
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0901.4179
#3 · backfill · confidence 0.70
Jingwen Wu
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0812.2012
#8 · backfill · confidence 0.70
Jingwen Wu
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0708.2959
#5 · backfill · confidence 0.70
Jingwen Wu