標(biāo)題: Titlebook: Science with the VLT in the ELT Era; Alan Moorwood Conference proceedings 2009 Springer Science+Business Media B.V. 2009 ALMA.Astronomical [打印本頁] 作者: Opulent 時(shí)間: 2025-3-21 17:58
書目名稱Science with the VLT in the ELT Era影響因子(影響力)
書目名稱Science with the VLT in the ELT Era影響因子(影響力)學(xué)科排名
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書目名稱Science with the VLT in the ELT Era網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Science with the VLT in the ELT Era被引頻次
書目名稱Science with the VLT in the ELT Era被引頻次學(xué)科排名
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書目名稱Science with the VLT in the ELT Era讀者反饋
書目名稱Science with the VLT in the ELT Era讀者反饋學(xué)科排名
作者: parallelism 時(shí)間: 2025-3-21 22:26
Pushing FORS to the Limit—A New Population of Faint Extended Ly, Emitters at ,~3al long slit spectrograph. A major motivation for our deep spectroscopic search was thereby the prospect of reaching sufficiently low surface brightness levels to detect or place interesting upper limits on the the fluorescent Ly. emission from optically thick regions induced by the metagalactic ion作者: 連鎖 時(shí)間: 2025-3-22 00:56 作者: 緊張過度 時(shí)間: 2025-3-22 05:06
Conference proceedings 2009peci c ideas and proposals for new, second generation VLT/I instruments were also solicited following a tradition set by several earlier Workshops held since the start of the VLT development. The programme consisted of invited talks and reviews and contributed talks and posters. Almost all those giv作者: justify 時(shí)間: 2025-3-22 08:51
E. V. Held,M. Gullieuszik,I. Saviane,F. Sabbadin,Y. Momany,L. Rizzi,F. Bresolind herein is the multidisciplinary teamwork. Most of the enabling technologies have been established by putting in the “melting pot” expertise in fields that, at first glance, may appear very far apart. I hope that this collection of articles will make the readers aware that vaccinology is rapidly taking a 978-94-007-9793-2978-94-007-4543-8作者: MIRE 時(shí)間: 2025-3-22 13:48 作者: 食料 時(shí)間: 2025-3-22 19:15
P. Bonifacio,J. Andersen,S. M. Andrievsky,B. Barbuy,T. C. Beers,E. Caffau,R. Cayrel,E. Depagne,P. Fr作者: 虛弱 時(shí)間: 2025-3-22 23:32 作者: Hot-Flash 時(shí)間: 2025-3-23 02:04
Th. Ratzka,Ch. Leinert,R. van Boekel,A. A. Schegerer作者: 傾聽 時(shí)間: 2025-3-23 06:43 作者: 付出 時(shí)間: 2025-3-23 10:52 作者: GRATE 時(shí)間: 2025-3-23 14:21 作者: Resection 時(shí)間: 2025-3-23 21:55 作者: 使苦惱 時(shí)間: 2025-3-23 22:49 作者: Charade 時(shí)間: 2025-3-24 03:09 作者: 發(fā)誓放棄 時(shí)間: 2025-3-24 08:20
M. Puech,F. Hammer,H. Flores,Y. Yang,B. Neichelformatik auch an den methodologischen Prolehre an. Daneben tr?gt die Wirtschaftsinformatik auch an den methodologischen Problemen der Informatik.. Nicht zuletzt entstehen methodologische Fragestellungen durch Besonderheiten des Untersuchungsgegenstands der Wirtschaftsinformatik sowie durch ihre Ausr作者: 拱墻 時(shí)間: 2025-3-24 12:23 作者: nutrients 時(shí)間: 2025-3-24 18:20
N. Przybilla,A. Seifahrt,K. Butler,M. F. Nieva,H.-U. K?ufl,A. Kauferven System zuzurechnen sind oder als Dienstleistung charakterisiert werden k?nnen. Dazu sollen die drei genannten Bereiche und ihre Rationalit?ten n?her beleuchtet und kurz umrissen werden. Die Aufarbeitung des Forschungsstands verfolgt sodann das Ziel der weiteren theoretischen Sensibilisierung und作者: 放縱 時(shí)間: 2025-3-24 21:05 作者: 放縱 時(shí)間: 2025-3-25 00:00 作者: MAG 時(shí)間: 2025-3-25 06:17
Guy Perrinarch institutes, universities) perform, but on how they interact with each other as elements of a collective system of knowledge creation and use, and on their interplay with social institutions (such as value, norms and legal frameworks)” (Dodgson in Elgar companion to neo-Schumpeterian economics. 作者: Resistance 時(shí)間: 2025-3-25 08:32
W. Jaffe,D. Raban,K. Meisenheimer,K. Tristram,Ch. Leinert,H. R?ttgeringglobal context our study is focusing on “future preparedness” of a specific group of countries, the OECD countries. The origin of this group dates back to 1960, when 18 European countries and the United States as well as Canada created in Paris an organization dedicated to global development. Today 作者: 借喻 時(shí)間: 2025-3-25 13:53
Olivier Chesneau find that project performance is positively affected by the strictness of project monitoring and evaluation by the government, but negatively affected by interventions in application procedures. Finally, we find neither complementarity nor substitution between project leadership and government moni作者: 精密 時(shí)間: 2025-3-25 19:32 作者: amenity 時(shí)間: 2025-3-25 21:37 作者: cipher 時(shí)間: 2025-3-26 01:08 作者: Embolic-Stroke 時(shí)間: 2025-3-26 07:52 作者: 殺蟲劑 時(shí)間: 2025-3-26 12:10
Science with the VLT in the ELT Era978-1-4020-9190-2Series ISSN 1570-6591 Series E-ISSN 1570-6605 作者: 帶來的感覺 時(shí)間: 2025-3-26 16:40 作者: Override 時(shí)間: 2025-3-26 18:47 作者: 豐富 時(shí)間: 2025-3-26 22:45 作者: Lethargic 時(shí)間: 2025-3-27 03:15 作者: 爆米花 時(shí)間: 2025-3-27 06:43
MIDI Sees Active Galactic Nucleimited to relatively bright objects, there are a dozen or so Seyfert galaxies, and at least one quasar, that are bright enough to see. These are the only extragalactic targets so far observed with optical/infrared interferometers.作者: prolate 時(shí)間: 2025-3-27 12:25 作者: 碎石頭 時(shí)間: 2025-3-27 16:43 作者: Ligament 時(shí)間: 2025-3-27 19:32 作者: 威脅你 時(shí)間: 2025-3-28 00:48 作者: 過渡時(shí)期 時(shí)間: 2025-3-28 03:33
The ESO Large Programme “First Stars”re not the first generation of stars they must be very close descendants of the first generation. One may hope to gain insight on the nature of the progenitors from detailed information on the descendants.作者: iodides 時(shí)間: 2025-3-28 06:27
Near-IR Spectroscopy of Blue Supergiantse that has so far been neglected. We report first results from a pilot spectroscopic investigation of Galactic BA-SGs at high resolution using CRIRES on the VLT. This is in order to establish quantitative near-IR spectroscopy of BA-SGs in preparation for the extragalactic stellar science programme with the E-ELT.作者: peritonitis 時(shí)間: 2025-3-28 10:29 作者: Malaise 時(shí)間: 2025-3-28 16:28 作者: Corroborate 時(shí)間: 2025-3-28 22:48
VLTI Science Highlightss the interest for the technique from the astronomical community keeps growing more ambitious instrumental projects are contemplated which will definitely put optical/near-infrared interferometry into mainstream astrophysics. It is shown here how VTLI plays a leading role in all these aspects.作者: 小平面 時(shí)間: 2025-3-29 01:27
The Use of the VLTI for Studying the Asymmetric Mass Loss of Evolved Starsavorable location. These first results are promising for the second generation VLTI instruments, and an improved synergy with the new generation VLT instruments and ALMA is foreseen. The Paranal site would represent in this context a key facility for high spatial resolution studies of time-variable, spatially complex compact dusty sources.作者: 驕傲 時(shí)間: 2025-3-29 06:55 作者: DOTE 時(shí)間: 2025-3-29 11:05
Pushing FORS to the Limit—A New Population of Faint Extended Ly, Emitters at ,~3an limit systems (LLS) to fainter surface brightness limits with observations performed in service mode in periods of bad seeing. For this purpose we have initiated a program of long-slit spectroscopy with FORS2 at the VLT to search for extended Ly. emission in a mostly blank field (LP 173.A-0440). 作者: charisma 時(shí)間: 2025-3-29 14:09 作者: glisten 時(shí)間: 2025-3-29 18:53 作者: Classify 時(shí)間: 2025-3-29 22:03 作者: inventory 時(shí)間: 2025-3-30 01:03 作者: 減去 時(shí)間: 2025-3-30 05:56 作者: 山羊 時(shí)間: 2025-3-30 10:47 作者: Counteract 時(shí)間: 2025-3-30 14:42 作者: CON 時(shí)間: 2025-3-30 18:14 作者: 爆米花 時(shí)間: 2025-3-30 23:27 作者: 使殘廢 時(shí)間: 2025-3-31 04:16
VLTI Science Highlightsted science operation and have boosted the rate of astrophysics-oriented publications based on interferometric results. Also, the advent of long-baseline interferometers making use of large pupils has opened the way to faint science and first results on extragalactic objects has made it a reality. A作者: deficiency 時(shí)間: 2025-3-31 06:40
MIDI Sees Active Galactic Nucleimited to relatively bright objects, there are a dozen or so Seyfert galaxies, and at least one quasar, that are bright enough to see. These are the only extragalactic targets so far observed with optical/infrared interferometers.