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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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21#
發(fā)表于 2025-3-25 05:08:03 | 只看該作者
https://doi.org/10.1007/978-3-642-10850-1ming galaxies that are good probes for the metal-enrichment in the primordial CGM gas. We carry out the visibility-based . 158-.m line stacking as well as the rest-frame FIR continuum for deep ALMA data of 18 normal star-forming galaxies at . 5.15–7.14. Also performing the HST stacking for the same
22#
發(fā)表于 2025-3-25 07:32:48 | 只看該作者
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發(fā)表于 2025-3-25 13:01:58 | 只看該作者
24#
發(fā)表于 2025-3-25 18:07:26 | 只看該作者
https://doi.org/10.1007/978-981-16-4979-0Observations with ALMA; Galaxy Formation; Galaxy Evolution; High Redshift; Star-forming Galaxies in the
25#
發(fā)表于 2025-3-25 22:46:26 | 只看該作者
26#
發(fā)表于 2025-3-26 00:08:10 | 只看該作者
Introduction,rmation history is obscured by the cold dust. It is thus inevitably important to investigate the origin of the CIB and unveil the obscured side of the universe (i.e. Cold Universe) to fully understand the galaxy evolution and formation. In the frameworks of . cold dark matter structure formation, th
27#
發(fā)表于 2025-3-26 04:26:44 | 只看該作者
28#
發(fā)表于 2025-3-26 11:49:41 | 只看該作者
Interstellar Medium Scale I: Galaxy Size,eep 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
29#
發(fā)表于 2025-3-26 15:23:30 | 只看該作者
Insterstellar Medium Scale II: Galaxy Morphology,ion, 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
30#
發(fā)表于 2025-3-26 17:23:29 | 只看該作者
Circumgalactic Medium Scale: Metal-Enriched Gas Halo,ming galaxies that are good probes for the metal-enrichment in the primordial CGM gas. We carry out the visibility-based . 158-.m line stacking as well as the rest-frame FIR continuum for deep ALMA data of 18 normal star-forming galaxies at . 5.15–7.14. Also performing the HST stacking for the same
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