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Lifan Wang

Researcher at Texas A&M University

Publications -  122
Citations -  5677

Lifan Wang is an academic researcher from Texas A&M University. The author has contributed to research in topics: Supernova & Light curve. The author has an hindex of 34, co-authored 119 publications receiving 5254 citations. Previous affiliations of Lifan Wang include University of Sussex & Netherlands Institute for Space Research.

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The Herschel Multi-tiered Extragalactic Survey: HerMES

Seb Oliver, +120 more
TL;DR: The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy program designed to map a set of nested fields totalling ∼380deg^2 as mentioned in this paper.
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The Herschel Multi-tiered Extragalactic Survey: HerMES

Seb Oliver, +118 more
TL;DR: The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy program designed to map a set of nested fields totalling ~380 deg^2 as mentioned in this paper.
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The Supernova Gamma-Ray Burst Connection

TL;DR: In this paper, it was shown that the light curve of SN 1998bw can be understood as the result of viewing an aspherical explosion roughly along the symmetry axis of an exploding, non-degenerate C/O core of a massive star with a kinetic energy of 2x10^51 erg, a total ejecta mass of 2 solar masses, and a nickel-56 mass of 0.2 solar masses.
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Herschel unveils a puzzling uniformity of distant dusty galaxies

D. Elbaz, +117 more
TL;DR: In this paper, the spectral energy distribution and dust temperature of galaxies have strongly evolved over the last 80% of the age of the Universe, and possible consequences for the determination of star-formation rates (SFR) and any evidence for a major change in their starformation properties.
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HerMES: Far infrared properties of known AGN in the HerMES fields

Evanthia Hatziminaoglou, +83 more
TL;DR: In this paper, the authors study large samples of spectroscopically confirmed type 1 and type 2 AGN lying within the Herschel Multi-tiered Extragalactic Survey (HerMES) fields observed during the science demonstration phase, aiming to understand their FIR colour distributions and constrain their starburst contributions.