標(biāo)題: Titlebook: ISO Surveys of a Dusty Universe; Proceedings of a Rin D. Lemke,M. Stickel,K. Wilke Conference proceedings 2000 Springer-Verlag Berlin Heide [打印本頁] 作者: Forestall 時(shí)間: 2025-3-21 19:10
書目名稱ISO Surveys of a Dusty Universe影響因子(影響力)
書目名稱ISO Surveys of a Dusty Universe影響因子(影響力)學(xué)科排名
書目名稱ISO Surveys of a Dusty Universe網(wǎng)絡(luò)公開度
書目名稱ISO Surveys of a Dusty Universe網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱ISO Surveys of a Dusty Universe被引頻次
書目名稱ISO Surveys of a Dusty Universe被引頻次學(xué)科排名
書目名稱ISO Surveys of a Dusty Universe年度引用
書目名稱ISO Surveys of a Dusty Universe年度引用學(xué)科排名
書目名稱ISO Surveys of a Dusty Universe讀者反饋
書目名稱ISO Surveys of a Dusty Universe讀者反饋學(xué)科排名
作者: DAFT 時(shí)間: 2025-3-21 20:38
Conference proceedings 20001989 and 1990 surveys were only a minor topic. At that time we were excited by the discoveries of the IRAS survey mission and wanted to follow it up with pointed observations using an observatory telescope equipped with versatile instruments. With the rapid development of detector arrays and stimula作者: Anecdote 時(shí)間: 2025-3-22 03:18
ISO Deep Far-Infrared Survey in the Lockman Hole al. by a factor of 10–50. The slopes of the number densities are similar at the both wavelengths, implying far-infrared sources are at low redshift. Comparisons with radio and X-ray sources indicate most of far-infared sources are star-forming galaxies.作者: 表臉 時(shí)間: 2025-3-22 06:38
FIRBACK Source Counts and Cosmological Implications at other wavelengths, we have developped a phenomenological model, which constrains in a simple way the luminosity function evolution with the redshift, and fits all the existing deep source counts from the mid-infrared to the submillimetre range.作者: induct 時(shí)間: 2025-3-22 08:50
The Extragalactic Background and Its Fluctuations in the Far-Infrared Wavelengthsations, we have used the FIRBACK observations. FIRBACK is a deep cosmological survey conducted at 170μm with ISOPHOT [.]. We show that the emission of unresolved extra-galactic sources clearly dominates, at arc-minute scales, the background fluctuations in the lowest galactic emission regions. This is the first detection of the CFIRB fluctuations.作者: 懸掛 時(shí)間: 2025-3-22 14:04 作者: 大方一點(diǎn) 時(shí)間: 2025-3-22 20:07
Near Infrared Extragalactic Backgroundn foreground emission components. 2- point correlation analysis indicates that the fluctuation has a characteristic spatial frequencyat 1 ～ 2 × 10. arcmin. These results indicate that the detected isotropic emission is cosmological in origin, and is new observational evidence for the study of the formation and evolution of galaxies.作者: 翅膀拍動(dòng) 時(shí)間: 2025-3-23 01:00
The European Large Area ISO Survey (ELAIS): Latest Results A comprehensive identification programme is underway and a number of extremely luminous objects have already been discovered. This survey provides an exciting legacy from the ISO mission and (amongst many goals) will allow us to provide important constraints on the obscured star-formation history of the Universe.作者: –LOUS 時(shí)間: 2025-3-23 04:26
A Local Infrared Perspective to Deeper ISO Surveyssing longer wavelength IRAS colour criteria and produce complete 12 μm samples of galaxies and stars. This new technique allows us to estimate the contribution of non-dusty galaxies to the IRAS 12 μm counts and produce a true local mid-infrared extragalactic sample compatible with ISO surveys. We present our initial analysis and results.作者: ELUC 時(shí)間: 2025-3-23 07:32
The Star Formation History of the Universeound in an Ω. = 1 universe, but this model fails to account for even the lowest estimates of the 140–350 μm background by a factor of 2. Either the observed values are overestimated or we need a new population of submm sources. The problem is eased in a . = 0, Ωo = 0.3 or . = 0.7, Ωo = 0.3 universe.作者: 聲明 時(shí)間: 2025-3-23 23:43 作者: JOG 時(shí)間: 2025-3-24 03:50 作者: Cirrhosis 時(shí)間: 2025-3-24 07:21
ures to study the physiology and biochemistry of carbohydrate metabolism in plants but at the level of the cell. The second relates to the utilization of carbohydrates as a primary carbon source and their influence upon biomass and secondary metabolite productivity in cell cultures. Such a division 作者: 錯(cuò)事 時(shí)間: 2025-3-24 13:04 作者: 一再遛 時(shí)間: 2025-3-24 17:23 作者: opportune 時(shí)間: 2025-3-24 21:53
Dario Fadda,David Elbaz,Pierre-Alain Duc,Hector Flores,Catherine Cesarskyticists. To paraphrase Oscar Wilde, to have one disease is permissible, to have two looks like immunological unruliness. As polyendocrinopathy is immunological in origin, the varieties of multiple endocrine adenomatosis will not be considered here. The overlap of organ-specific autoimmune diseases h作者: thrombosis 時(shí)間: 2025-3-24 23:53 作者: helper-T-cells 時(shí)間: 2025-3-25 07:20
Christian Surace,Andreas Efstathiou,Philippe Héraudeau,Dietrich Lemke,Seb Oliver,Michael Rowan-Robinhydrate Metabolism in Pregnancy and the Newborn to be held in Aberdeen, and by now the form is set. How much its content has changed is a matter of nice judgement and not under the control of the organizers. It is not within their power to bring news of revolution, if there has been no revolution. C作者: Circumscribe 時(shí)間: 2025-3-25 07:34
Haruyuki Okuda of carbohydrates/protein interactions can be probed in parallel. .Carbohydrate Microarrays: Methods and Protocols. aims to give the reader the theoretical and experimental clues necessary for the fabrication and implementation of carbohydrate microarrays. This requires three essential steps: 1) to 作者: AIL 時(shí)間: 2025-3-25 15:02 作者: Tdd526 時(shí)間: 2025-3-25 19:22 作者: 可互換 時(shí)間: 2025-3-25 22:59 作者: 無彈性 時(shí)間: 2025-3-26 02:10 作者: 帽子 時(shí)間: 2025-3-26 04:35
Guilaine Lagache,Jean-Loup Puget,Alain Abergel,Francois-Xavier Désert,Hervé Dole,Francois R. Bouchet of carbohydrates/protein interactions can be probed in parallel. .Carbohydrate Microarrays: Methods and Protocols. aims to give the reader the theoretical and experimental clues necessary for the fabrication and implementation of carbohydrate microarrays. This requires three essential steps: 1) to 作者: 纖細(xì) 時(shí)間: 2025-3-26 09:14
Mika Juvela,Kalevi Mattila,Dietrich Lemkeation advice from the experts.Includes supplementary materia.Carbohydrate microarrays emerged as a key technology for the deciphering of the glycospace by providing a multiplex technology where tens to hundreds of carbohydrates/protein interactions can be probed in parallel. .Carbohydrate Microarray作者: 含鐵 時(shí)間: 2025-3-26 14:56 作者: dearth 時(shí)間: 2025-3-26 20:05 作者: 無彈性 時(shí)間: 2025-3-26 22:23 作者: Aesthete 時(shí)間: 2025-3-27 04:26 作者: Intercept 時(shí)間: 2025-3-27 08:40
Michael Rowan-Robinson of carbohydrates/protein interactions can be probed in parallel. .Carbohydrate Microarrays: Methods and Protocols. aims to give the reader the theoretical and experimental clues necessary for the fabrication and implementation of carbohydrate microarrays. This requires three essential steps: 1) to 作者: Neolithic 時(shí)間: 2025-3-27 10:39 作者: FRET 時(shí)間: 2025-3-27 17:37 作者: 悶熱 時(shí)間: 2025-3-27 19:53
The ISO Mission and Its Surveysovided sensitive and flexible imaging, photometric, polarimetric and low-mediumhigh resolution spectroscopic capabilities over a wide wavelength range from 2.5–240 μm. During its highly-successful operational lifetime, it made some 30000 individual pointed observations. All data are now in the publi作者: 浮夸 時(shí)間: 2025-3-27 22:40
A New Population of Faint Starburst Galaxies Revealed by 15 μm ISOCAM Deep Surveysthe Lockman Hole and Marano Field, the HDF-North and South (plus flanking fields) and the lensing cluster A2390 at low fluxes and IRAS at high fluxes. We cover four decades in flux from 50 μJy to ～0.3 Jy. The roughly 1000 sources detected with ISOCAM, 600 of which have a flux above the 80 % complete作者: 谷物 時(shí)間: 2025-3-28 02:28
Mid-Infrared Properties of Distant Cluster Galaxies as Revealed by ISOCAMid-IR properties and optical follow-ups of ISOCAM sources detected in Abell 1689 and Abell 2390, two clusters at a redshift of . = 0.2, and of J1888 and 3C330, two clusters at high redshift (. = 0.6)..Galaxies detected at 6.75 μm, which correspond to the brightest optical sources, always exhibit a c作者: 頭盔 時(shí)間: 2025-3-28 08:17 作者: Disk199 時(shí)間: 2025-3-28 12:32 作者: genesis 時(shí)間: 2025-3-28 15:41
Japanese Deep Surveys with ISObservations were very successful and provided valuable data on star forming activity and galaxy evolution. Model calculations indicate that there was an intense star formation period that peaked at around . = 0.7.作者: organism 時(shí)間: 2025-3-28 22:47 作者: MUTE 時(shí)間: 2025-3-29 00:43 作者: persistence 時(shí)間: 2025-3-29 06:22
Deep Far Infrared ISOPHOT Survey in “Selected Area 57”Space Observatory (ISO.) at both 60 μm and 90 μm. We describe our data reduction and analysis scheme with special emphasis on source extraction and flux calibration. With a formal signal to noise ratio of 6.75 we have source detection limits of 90 mJy at 60 μm and 50 mJy at 90 μm. To these limits we作者: 神化怪物 時(shí)間: 2025-3-29 10:14 作者: 四溢 時(shí)間: 2025-3-29 12:51 作者: 亂砍 時(shí)間: 2025-3-29 17:26
Cosmic Infrared Background: ISOPHOT FIR Source Counts at 90, 150 and 180 μmin most cases no previously known sources can be associated with them. Based on the far-infrared spectral energy distributions it is likely that dust-enshrouded, distant galaxies form a significant fraction of the sources..We estimate the number densities of extragalactic sources at 90μm, 150μm and 作者: Phagocytes 時(shí)間: 2025-3-29 21:15
Near Infrared Extragalactic Backgroundope in Space (IRTS). After subtracting the contribution of faint stars and zodiacal component based on the model, significant isotropic emission is detected whose in-band flux amounts to ～ 30 nWm.sr.. This brightness is consistent with upper limits of COBE/DIRBE, but is much brighter than the integr作者: defenses 時(shí)間: 2025-3-30 03:04 作者: Estimable 時(shí)間: 2025-3-30 06:04
A Local Infrared Perspective to Deeper ISO Surveysd comparison with ISO surveys and review their problems. We provide a stellar infrared diagnostic diagram to distinguish galaxies from stars without using longer wavelength IRAS colour criteria and produce complete 12 μm samples of galaxies and stars. This new technique allows us to estimate the con作者: Fecundity 時(shí)間: 2025-3-30 11:43
The Role of Luminous Infrared Galaxies at z ～ 1 as Revealed by the 15 μm Extragalactic Background Lilose to . ～ 0.8. A preliminary study of a sample of optical counterparts with spectroscopic redshifts in the Hubble Deep Field North (HDFN) and in one of the Canada-France Redshift Survey (CFRS) fields, indicates that they are massive (. ～ 10..⊙) and bright (several 10..⊙) galaxies. The contribution作者: 迷住 時(shí)間: 2025-3-30 16:02 作者: 同位素 時(shí)間: 2025-3-30 16:51 作者: Definitive 時(shí)間: 2025-3-31 00:36 作者: sorbitol 時(shí)間: 2025-3-31 01:45 作者: 分貝 時(shí)間: 2025-3-31 05:41
Michael J. D. Linden-V?rnle,Hans Ulrik N?rgaard-Nielsen,Henning E. J?rgensen,Leif Hansen,Martin Haasf the necessary materials and reagents, step-by-step, readily reproducible protocols, and notes on troubleshooting and avoiding known pitfalls..?.Authoritative and easily accessible,. .Carbohydrate Microarrays:978-1-4939-5866-5978-1-61779-373-8Series ISSN 1064-3745 Series E-ISSN 1940-6029 作者: FANG 時(shí)間: 2025-3-31 11:26
David L. Clementsf the necessary materials and reagents, step-by-step, readily reproducible protocols, and notes on troubleshooting and avoiding known pitfalls..?.Authoritative and easily accessible,. .Carbohydrate Microarrays:978-1-4939-5866-5978-1-61779-373-8Series ISSN 1064-3745 Series E-ISSN 1940-6029 作者: TOM 時(shí)間: 2025-3-31 16:06 作者: SIT 時(shí)間: 2025-3-31 20:28
David Elbazf the necessary materials and reagents, step-by-step, readily reproducible protocols, and notes on troubleshooting and avoiding known pitfalls..?.Authoritative and easily accessible,. .Carbohydrate Microarrays:978-1-4939-5866-5978-1-61779-373-8Series ISSN 1064-3745 Series E-ISSN 1940-6029 作者: Maximize 時(shí)間: 2025-4-1 01:22
f the necessary materials and reagents, step-by-step, readily reproducible protocols, and notes on troubleshooting and avoiding known pitfalls..?.Authoritative and easily accessible,. .Carbohydrate Microarrays:978-1-4939-5866-5978-1-61779-373-8Series ISSN 1064-3745 Series E-ISSN 1940-6029 作者: 畫布 時(shí)間: 2025-4-1 01:57
0075-8450 on the sky and the maximum distance derived from the detection sensitivity. Clearly, with this ?gure of merit, ISO, as a pointed observatory, is rated low. Applying the classic978-3-540-45553-0Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: CHOP 時(shí)間: 2025-4-1 07:52
A New Population of Faint Starburst Galaxies Revealed by 15 μm ISOCAM Deep Surveysngth studies of a subsample of the ISOCAM sources indicate that they are intrinsically bright galaxies (Luminous Infrared Galaxies, LIRGs), with median redshift 0.7. These galaxies, despite their low surface density, are responsible for a large part of star formation at . < 1 and contribute substant作者: 使乳化 時(shí)間: 2025-4-1 11:02
The Role of Luminous Infrared Galaxies at z ～ 1 as Revealed by the 15 μm Extragalactic Background Lignitude higher at . ～ 0.8 than today. Depending on their spectral energy distribution, these galaxies must produce more than 30% of the 140 μm EBL, where the cosmic infrared background peaks. Hence, they produce a significant fraction of the overall energy radiated by galaxies during the hubble time作者: pancreas 時(shí)間: 2025-4-1 14:40
Models for the Infrared Emission from Starburst Galaxiesxy to its age and star formation history. We find that exponentially decaying 10. - 10. yrs old bursts can explain the IRAS colours of starburst galaxies. The models are also shown to account satisfactorily for the multiwavelength data on the prototypical starburst galaxy M82 and NGC6090, a starburs作者: B-cell 時(shí)間: 2025-4-1 20:14 作者: Counteract 時(shí)間: 2025-4-2 00:47
Martin F. Kesslerby a single intravenous injection of alloxan or streptozotocin: two drugs which act selectively on the beta-cells of the pancreatic islets (Rerup, 1970). Streptozotocin is now preferred to alloxan because it has fewer side effects (Rudas, 1969). Another advantage of rodents, worth emphasising becaus作者: 變白 時(shí)間: 2025-4-2 03:24
Catherine J. Cesarskytoimmune polyglandular syndrome (Winter and Maclaren 1987); it has a strong association with HLA DR3 or DR4. The form of diabetes is insulin dependent, type I, and indeed has been termed type IB (Bottazzo et al. 1974), the form with a female preponderance, later onset and persistence of islet cell a作者: 邊緣帶來墨水 時(shí)間: 2025-4-2 09:23 作者: DUCE 時(shí)間: 2025-4-2 11:22
