Titlebook: Demographics of the Cold Universe with ALMA; From Interstellar an Seiji Fujimoto Book 2021 Springer Nature Singapore Pte Ltd. 2021 Observat

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Latency

https://doi.org/10.1007/978-3-642-10850-1ting the evolutional connection from the dusty star-forming to the quiescent galaxies. In the context of previous ALMA studies for the . measurements, this is the first challenge for the statistical study of the . properties in a systematic way.

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高爾夫

Interstellar Medium Scale I: Galaxy Size,ting the evolutional connection from the dusty star-forming to the quiescent galaxies. In the context of previous ALMA studies for the . measurements, this is the first challenge for the statistical study of the . properties in a systematic way.

并排上下

Circumgalactic Medium Scale: Metal-Enriched Gas Halo,s faint satellite galaxies. Interestingly, the radial profile of the . halo is well consistent with that of the Lyman-alpha (Ly.) halo that is universally identified around . normal star-forming galaxies in the recent deep MUSE observations, indicative of the association between the . and Ly. halos.

disciplined

disciplined

巡回

小隔間

DICOM Media: Files, Folders, and DICOMDIRsr study, we have constructed 1220 ALMA submm/mm source sample from 1643 ALMA maps, that are the largest ALMA sample and dataset so far obtained, by making full use of the archive as well as our original data. In this chapter, we describe the ALMA sample and dataset used for the analysis at each scale.

probate

https://doi.org/10.1007/978-3-642-10850-1ALMA 1-mm map. Owing to the stacked, deep high-resolution ALMA map, we find that our sample has an average . and rest-frame FIR ., ., values of . kpc and 1.2 ± 0.2, respectively. Interestingly, we obtain the rest-frame optical . and . of . (.) and . kpc (> .), suggesting that the dusty disk-like structure is embedded in the larger stellar disk.