Opponent 发表于 2025-3-25 05:08:03
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 sameExpurgate 发表于 2025-3-25 07:32:48
http://reply.papertrans.cn/27/2654/265301/265301_22.png寻找 发表于 2025-3-25 13:01:58
http://reply.papertrans.cn/27/2654/265301/265301_23.pngOsmosis 发表于 2025-3-25 18:07:26
https://doi.org/10.1007/978-981-16-4979-0Observations with ALMA; Galaxy Formation; Galaxy Evolution; High Redshift; Star-forming Galaxies in the蒸发 发表于 2025-3-25 22:46:26
http://reply.papertrans.cn/27/2654/265301/265301_25.png清楚 发表于 2025-3-26 00:08:10
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, thFRAX-tool 发表于 2025-3-26 04:26:44
http://reply.papertrans.cn/27/2654/265301/265301_27.png吼叫 发表于 2025-3-26 11:49:41
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洞察力 发表于 2025-3-26 15:23:30
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 . kpclambaste 发表于 2025-3-26 17:23:29
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