標(biāo)題: Titlebook: Demographics of the Cold Universe with ALMA; From Interstellar an Seiji Fujimoto Book 2021 Springer Nature Singapore Pte Ltd. 2021 Observat [打印本頁(yè)] 作者: 無(wú)法修復(fù) 時(shí)間: 2025-3-21 18:50
書(shū)目名稱Demographics of the Cold Universe with ALMA影響因子(影響力)
書(shū)目名稱Demographics of the Cold Universe with ALMA影響因子(影響力)學(xué)科排名
書(shū)目名稱Demographics of the Cold Universe with ALMA網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Demographics of the Cold Universe with ALMA網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Demographics of the Cold Universe with ALMA被引頻次
書(shū)目名稱Demographics of the Cold Universe with ALMA被引頻次學(xué)科排名
書(shū)目名稱Demographics of the Cold Universe with ALMA年度引用
書(shū)目名稱Demographics of the Cold Universe with ALMA年度引用學(xué)科排名
書(shū)目名稱Demographics of the Cold Universe with ALMA讀者反饋
書(shū)目名稱Demographics of the Cold Universe with ALMA讀者反饋學(xué)科排名
作者: Latency 時(shí)間: 2025-3-21 21:49
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.作者: 虛情假意 時(shí)間: 2025-3-22 00:39 作者: 高爾夫 時(shí)間: 2025-3-22 08:01
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.作者: 并排上下 時(shí)間: 2025-3-22 10:37
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.作者: disciplined 時(shí)間: 2025-3-22 15:26 作者: disciplined 時(shí)間: 2025-3-22 20:55 作者: 巡回 時(shí)間: 2025-3-23 00:29 作者: 小隔間 時(shí)間: 2025-3-23 01:33
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.作者: probate 時(shí)間: 2025-3-23 07:26
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.作者: GUILE 時(shí)間: 2025-3-23 11:22
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作者: 弓箭 時(shí)間: 2025-3-23 16:28
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作者: 聯(lián)合 時(shí)間: 2025-3-23 19:54 作者: Horizon 時(shí)間: 2025-3-24 01:09 作者: 潔凈 時(shí)間: 2025-3-24 05:47
Conclusion,In this chapter, we summarize our main results and discussions in the scales of the ISM, the CGM, and the cosmic structure.作者: harrow 時(shí)間: 2025-3-24 09:53
Demographics of the Cold Universe with ALMA978-981-16-4979-0Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: interpose 時(shí)間: 2025-3-24 14:19 作者: 爆米花 時(shí)間: 2025-3-24 18:26
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作者: amyloid 時(shí)間: 2025-3-24 21:57
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作者: myalgia 時(shí)間: 2025-3-25 00:00
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 作者: Opponent 時(shí)間: 2025-3-25 05:08
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 作者: Expurgate 時(shí)間: 2025-3-25 07:32 作者: 尋找 時(shí)間: 2025-3-25 13:01 作者: Osmosis 時(shí)間: 2025-3-25 18:07
https://doi.org/10.1007/978-981-16-4979-0Observations with ALMA; Galaxy Formation; Galaxy Evolution; High Redshift; Star-forming Galaxies in the 作者: 蒸發(fā) 時(shí)間: 2025-3-25 22:46 作者: 清楚 時(shí)間: 2025-3-26 00:08
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作者: FRAX-tool 時(shí)間: 2025-3-26 04:26 作者: 吼叫 時(shí)間: 2025-3-26 11:49
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作者: 洞察力 時(shí)間: 2025-3-26 15:23
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 作者: lambaste 時(shí)間: 2025-3-26 17:23
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 作者: 不吉祥的女人 時(shí)間: 2025-3-27 00:08 作者: 成績(jī)上升 時(shí)間: 2025-3-27 03:54 作者: glacial 時(shí)間: 2025-3-27 09:11
DICOM Media: Files, Folders, and DICOMDIRsr/submillimeter Array (ALMA). Although the previous observations show that about half of the CIB is explained by individual submm/mm emission identified in the ISM scale, the physical origin of these individual submm/mm emission is still unclear even with the recent ALMA observations. Moreover, no o作者: Flinch 時(shí)間: 2025-3-27 11:04 作者: 中國(guó)紀(jì)念碑 時(shí)間: 2025-3-27 14:06
Kim Osman,Amber Marshall,Michael Dezuannis of the 10-kpc scale [C?.] halo newly discovered in our deep ALMA stacking. However, it is important that that outflows are required in all cases to enrich the carbon abundance of the primordial CGM gas around the early galaxies, where the outflows may be dominated by cold-mode outflows expelling t作者: delegate 時(shí)間: 2025-3-27 21:43
2190-5053 e of the findings are unexpected and as such challenge the current galaxy formation models, the book provides exciting questions that should be addressed in the next decades..978-981-16-4981-3978-981-16-4979-0Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: 廚房里面 時(shí)間: 2025-3-28 01:08
Introduction,r/submillimeter Array (ALMA). Although the previous observations show that about half of the CIB is explained by individual submm/mm emission identified in the ISM scale, the physical origin of these individual submm/mm emission is still unclear even with the recent ALMA observations. Moreover, no o作者: Derogate 時(shí)間: 2025-3-28 04:20 作者: 營(yíng)養(yǎng) 時(shí)間: 2025-3-28 09:25 作者: 鞠躬 時(shí)間: 2025-3-28 14:04 作者: 基因組 時(shí)間: 2025-3-28 14:39
Reviewing the Research Landscape of Online Scarcity Messages,ns. While scarcity marketing has long existed in brick-and-mortar settings, its presence in the online setting has changed the dynamics of consumers’ online shopping experiences. However, the literature on online scarcity messages lacks a unified conceptual framework. Therefore, this paper reports a作者: 流行 時(shí)間: 2025-3-28 21:36 作者: Mutter 時(shí)間: 2025-3-29 02:48
