activity
20182021
most citedLarge format imaging spectrograph for the Large Submillimeter Telescope (LST)

6 citations · 7 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.GA20211 cited

Capturing the inside-out quenching by black holes with far-infrared atomic line ratios

Shigeki Inoue, Hiroshi Matsuo, Naoki Yoshida +2

We propose to use relative strengths of far-infrared fine structure lines from galaxies to characterise early phases of the inside-out quenching by massive black holes (BHs). The B…

astro-ph.IM20216 cited

Large format imaging spectrograph for the Large Submillimeter Telescope (LST)

K. Kohno, R. Kawabe, Y. Tamura +19

We present a conceptual study of a large format imaging spectrograph for the Large Submillimeter Telescope (LST) and the Atacama Large Aperture Submillimeter Telescope (AtLAST). Re…

astro-ph.GA2020

Deep Learning for Line Intensity Mapping Observations: Information Extraction from Noisy Maps

Kana Moriwaki, Masato Shirasaki, Naoki Yoshida

Line intensity mapping (LIM) is a promising observational method to probe large-scale fluctuations of line emission from distant galaxies. Data from wide-field LIM observations all…

astro-ph.GA2020

Deep learning for intensity mapping observations: Component extraction

Kana Moriwaki, Nina Filippova, Masato Shirasaki +1

Line intensity mapping (LIM) is an emerging observational method to study the large-scale structure of the Universe and its evolution. LIM does not resolve individual sources but p…

astro-ph.GA2019

Large Population of ALMA Galaxies at z>6 with Very High [OIII]88um to [CII]158um Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?

Yuichi Harikane, Masami Ouchi, Akio K. Inoue +20

We present our new ALMA observations targeting [OIII]88um, [CII]158um, [NII]122um, and dust continuum emission for three Lyman break galaxies at z=6.0293-6.2037 identified in the S…

astro-ph.GA2019

Cross-correlation between the 21-cm signal and [OIII] emitters during early cosmic reionization

K. Moriwaki, N. Yoshida, M. B. Eide +1

We study statistics of the 21-cm signal from the epoch of reionization. We propose to use [OIII] line emitting galaxies to cross-correlate with the 21-cm signal from .…