GUILE
发表于 2025-3-23 11:22:51
Book 2021ay (ALMA). The author constructed the largest-ever ALMA sample and dataset, which enables them to identify very faint, rest-frame, far-infrared dust continuums as well as the carbon fine-structure line emission from distant galaxies that have been missed in previous surveys. The observational findin
弓箭
发表于 2025-3-23 16:28:09
Seiji FujimotoNominated as an outstanding Ph.D. thesis by the University of Tokyo, Japan.Discusses the largest ALMA dataset ever constructed.Describes the wide landscape of the Universe, from galaxy to cosmic struc
联合
发表于 2025-3-23 19:54:35
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Horizon
发表于 2025-3-24 01:09:20
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洁净
发表于 2025-3-24 05:47:21
Conclusion,In this chapter, we summarize our main results and discussions in the scales of the ISM, the CGM, and the cosmic structure.
harrow
发表于 2025-3-24 09:53:26
Demographics of the Cold Universe with ALMA978-981-16-4979-0Series ISSN 2190-5053 Series E-ISSN 2190-5061
interpose
发表于 2025-3-24 14:19:59
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爆米花
发表于 2025-3-24 18:26:22
DICOM Media: Files, Folders, and DICOMDIRshe submm/mm emission from high-. galaxies in the scales of the ISM, the CGM, and the cosmic structure based on the intensive ALMA data analyses. In our 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 ma
amyloid
发表于 2025-3-24 21:57:00
https://doi.org/10.1007/978-3-642-10850-1eep ALMA maps in Band 6/7 are composed of 1614 maps from the independent fields and 13 maps from the 3 lensing clusters. We analyze this large dataset to investigate the rest-frame far-infrared (FIR) size, ., and luminosity, . relation and the . evolution by a systematic .-visibility based technique
myalgia
发表于 2025-3-25 00:00:19
https://doi.org/10.1007/978-3-642-10850-1ion, in addition to its size. we have performed .-visibility based stacking for 33 ALMA sources at . 1–3 identified in the high resolution (beam = .) ALMA 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