Tracing star formation in galaxies with molecular line and continuum observations
K. Kohno, K. Muraoka, B. Hatsukade, K. Tanaka, D. Iono, K. Nakanishi,, T. Tosaki, T. Sawada, R. Kawabe, H. Ezawa, N. Yamaguchi, Y. Tamura, G., Wilson, M.S. Yun, D. Hughes, S. Matsushita, and P.-Y. Hsieh

TL;DR
This paper presents recent advances in extragalactic star formation studies through molecular line and continuum observations across local and high-redshift galaxies, enhancing understanding of galaxy evolution.
Contribution
It provides new observational data from multiple telescopes on molecular lines and continuum emissions in diverse galaxy types, improving insights into star formation processes.
Findings
Detection of molecular lines in local Seyfert and starburst galaxies.
High-J CO observations of distant starburst galaxies.
Continuum measurements of high-redshift galaxies.
Abstract
We report our recent progress on extragalactic spectroscopic and continuum observations, including HCN(J=1-0), HCO(J=1-0), and CN(N=1-0) imaging surveys of local Seyfert and starburst galaxies using the Nobeyama Millimeter Array, high-J CO observations (J=3-2 observations using the Atacama Submillimeter Telescope Experiment (ASTE) and J=2-1 observations with the Submillimeter Array) of galaxies, and 1.1 mm continuum observations of high-z violent starburst galaxies using the bolometer camera AzTEC mounted on ASTE.
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