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Yutaro Tachibana

Researcher at Tokyo Institute of Technology

Publications -  111
Citations -  1391

Yutaro Tachibana is an academic researcher from Tokyo Institute of Technology. The author has contributed to research in topics: Gamma-ray burst & Neutron star. The author has an hindex of 18, co-authored 110 publications receiving 1094 citations. Previous affiliations of Yutaro Tachibana include California Institute of Technology.

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The Fourth Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope

Marco Ajello, +152 more
TL;DR: The 4LAC catalog of active galactic nuclei (AGNs) detected by the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) between 2008 August 4 and 2016 August 2 contains 2863 objects located at high Galactic latitudes (|b|>10°deg}).
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The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole?

Daniel A. Perley, +72 more
TL;DR: In this article, the spectrum remains extremely hot throughout its evolution, and the photospheric radius contracts with time (receding below R <10^14 cm after 1 month).
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Machine learning for the Zwicky transient facility

TL;DR: In this article, various machine learning (ML) implementations and plans to make the maximal use of the large data set by taking advantage of the temporal nature of the data, and further combining it with other data sets.
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A Morphological Classification Model to Identify Unresolved PanSTARRS1 Sources: Application in the ZTF Real-time Pipeline

TL;DR: In this article, the authors presented a method to construct a large, deep catalog of point sources utilizing Pan-STARRS1 (PS1) 3π survey data, which consists of ~3 × 10^9 sources with m ≾ 23.5 mag.
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The First Tidal Disruption Flare in ZTF: From Photometric Selection to Multi-wavelength Characterization

TL;DR: In this article, the Zwicky Transient Facility (ZTF) observations of the tidal disruption flare AT2018zr/PS18kh reported by Holoien et al. and detected during ZTF commissioning were used to assess the quality of the ZTF astrometry.