Radio astronomy, Astrochemistry, Galaxy evolution
I’m a PhD student at the University of Tokyo.
My research field is (sub-)millimeter astronomy.
I’m interested in interstellar chemistry especially in external galaxies.
Telescopes: ALMA, Nobeyama 45m, JCMT, LMT
Apr. 2020 –
JSPS Research Fellowships for Young Scientists DC1
Oct. 2018 – Mar. 2020
The University of Tokyo Research Assistant (IGPEES)
Apr. 2020 –
Department of Astronomy, Graduate School of Science, The University of Tokyo
(PhD student)
Apr. 2018 – Mar. 2020
Department of Astronomy, Graduate School of Science, The University of Tokyo
(Master’s degree)
Apr. 2014 – Mar. 2018
Department of Astronomy, School of Science, The University of Tokyo
(Bachelor’s degree)
Apr. 2008 – Mar. 2014
Nagoya University Affiliated Upper and Lower Secondary School
B4R is a receiver system which consists of 2mm receiver and a dedicated digital spectrometer composed of 4 (-> 6) XFFTS boards, integrated on the Large Millimeter Telescope (LMT, 50m) at Mexico. I’m working on:
webpage: http://lmtgtm.org/b4r/
The 50m Large Submillimeter Telescope (LST) is a planned single-dish telescope, which is optimized for wide-area imaging and spectroscopic surveys in the 70-420 GHz frequency range. I’m working on:
webpage: https://www.lstobservatory.org