S
Shunsuke Baba
Researcher at Japan Aerospace Exploration Agency
Publications - 37
Citations - 247
Shunsuke Baba is an academic researcher from Japan Aerospace Exploration Agency. The author has contributed to research in topics: Galaxy & Active galactic nucleus. The author has an hindex of 7, co-authored 28 publications receiving 122 citations. Previous affiliations of Shunsuke Baba include National Institutes of Natural Sciences, Japan & University of Tokyo.
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Journal ArticleDOI
ALMA Observations of Multiple CO and C Lines toward the Active Galactic Nucleus of NGC 7469: An X-Ray-dominated Region Caught in the Act
Takuma Izumi,Dieu D. Nguyen,Masatoshi Imanishi,Taiki Kawamuro,Shunsuke Baba,Suzuka Nakano,Kotaro Kohno,Satoki Matsushita,David S. Meier,Jean L. Turner,Tomonari Michiyama,Nanase Harada,Sergio Martín,Kouichiro Nakanishi,Shuro Takano,Tommy Wiklind,Naomasa Nakai,Pei-Ying Hsieh +17 more
TL;DR: Izumi et al. as discussed by the authors used the Atacama Large Millimeter/submillimeter Array (ALMA) to map CO emission lines around the type 1 active galactic nucleus (AGN) of NGC 7469.
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All the PAHs: An AKARI-Spitzer Cross-archival Spectroscopic Survey of Aromatic Emission in Galaxies
TL;DR: In this paper, the authors present a large sample of 2.5-38 µm$ galaxy spectra drawn from a cross-archival comparison in the AKARI-Spitzer Extragalactic Spectral Survey (ASESS), and investigate a subset of 113 star-forming galaxies with prominent polycyclic aromatic hydrocarbon (PAH) emission spanning a wide range of star formation properties.
Journal ArticleDOI
All the PAHs: an AKARI-Spitzer Cross Archival Spectroscopic Survey of Aromatic Emission in Galaxies
TL;DR: In this paper, the authors present a large sample of 2.5-38 µm$ galaxy spectra drawn from a cross-archival comparison in the AKARI-Spitzer Extragalactic Spectral Survey (ASESS), and investigate a subset of 113 star-forming galaxies with prominent polycyclic aromatic hydrocarbon (PAH) emission spanning a wide range of star formation properties.
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Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIII. Large-scale Feedback and Star Formation in a Low-Luminosity Quasar at z = 7.07 on the Local Black Hole to Host Mass Relation
Takuma Izumi,Takuma Izumi,Yoshiki Matsuoka,Seiji Fujimoto,Masafusa Onoue,Michael A. Strauss,Hideki Umehata,Masatoshi Imanishi,Masatoshi Imanishi,Kotaro Kohno,Toshihiro Kawaguchi,Taiki Kawamuro,Shunsuke Baba,Tohru Nagao,Yoshiki Toba,Yoshiki Toba,Yoshiki Toba,Kohei Inayoshi,John D. Silverman,Akio K. Inoue,Soh Ikarashi,Kazushi Iwasawa,Nobunari Kashikawa,Takuya Hashimoto,Kouichiro Nakanishi,Kouichiro Nakanishi,Yoshihiro Ueda,Malte Schramm,Chien-Hsiu Lee,Hyewon Suh +29 more
TL;DR: In this article, the ALMA [CII] 158 $\mu$m line and underlying far-infrared (FIR) emission observations were presented toward HSC J124353.5 (J1243$+$0100) at $z = 7.07.
Journal ArticleDOI
Revised wavelength and spectral response calibrations for AKARI near-infrared grism spectroscopy: Cryogenic phase
Shunsuke Baba,Shunsuke Baba,Takao Nakagawa,Mai Shirahata,Naoki Isobe,Fumihiko Usui,Youichi Ohyama,Takashi Onaka,Kenichi Yano,Kenichi Yano,Chihiro Kochi,Chihiro Kochi +11 more
TL;DR: In this paper, the authors performed spectral calibrations for the AKARI near-infrared grism to quantitatively correct for the effect of the wavelength-dependent refractive index.