標(biāo)題: Titlebook: New Horizons from Multi-Wavelength Sky Surveys; Proceedings of the 1 Brian J. McLean,Daniel A. Golombek,Harry E. Payne Conference proceedin [打印本頁] 作者: 去是公開 時間: 2025-3-21 19:19
書目名稱New Horizons from Multi-Wavelength Sky Surveys影響因子(影響力)
書目名稱New Horizons from Multi-Wavelength Sky Surveys影響因子(影響力)學(xué)科排名
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書目名稱New Horizons from Multi-Wavelength Sky Surveys被引頻次
書目名稱New Horizons from Multi-Wavelength Sky Surveys被引頻次學(xué)科排名
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書目名稱New Horizons from Multi-Wavelength Sky Surveys讀者反饋
書目名稱New Horizons from Multi-Wavelength Sky Surveys讀者反饋學(xué)科排名
作者: 頭盔 時間: 2025-3-21 20:55 作者: FAR 時間: 2025-3-22 01:36
Prospects for Future Astrometric Missionsfor a mission within the next five years would be through a collaborative effort for a small, fast, cheap spacecraft which could be a precursor for future, larger, more accurate missions, which are under study.作者: negligence 時間: 2025-3-22 04:37 作者: 箴言 時間: 2025-3-22 12:36 作者: Incompetent 時間: 2025-3-22 14:57 作者: 別炫耀 時間: 2025-3-22 20:20
Denis: a Deep Near Infrared Southern Sky Surveyyear mainly dedicated to technical tests and pilot surveys of selected regions of high astronomical interest. In September 1996, approximately 3000 square degrees of the sky have been covered, and the survey should be completed in 1999.作者: Debate 時間: 2025-3-22 21:23
The Miyun 232 MHz General Catalogueatalogue, using a matching radius of 100 arcseconds. The remaining MGC objects were then matched with the B2/B3 (408 MHz), 4C (178 MHz), Texas (365 MHz, 1400 MHz) and 87GB (4.85 GHz) catalogues. 6850 MGC sources were found to lack any radio counterpart in these reference catalogues. It means 19.9% of sources listed in the MGC are probably new.作者: Endearing 時間: 2025-3-23 03:09 作者: GIDDY 時間: 2025-3-23 07:19
The Prospects of Large Surveys in Astronomyf the extent to which these two approaches—emphasis on instrumental capabilities, as contrasted to emphasis on sky coverage—also contribute to an increase in astrophysical understanding. Here, the distinction needs to be made between discovering a new phenomenon and understanding its underlying processes.作者: Crepitus 時間: 2025-3-23 12:00 作者: 清洗 時間: 2025-3-23 16:22
Radio Surveysects were recognized in early high-frequency surveys. The first gravitationally lensed quasar appeared in the extensive Jodrell Bank 960 MHz survey, and the first measurement of gravitational radiation came from the binary pulsar serendipidously found in a pulsar survey.作者: PACK 時間: 2025-3-23 21:35
The MPIfR Radio Continuum Surveys and Their WWW Distribution number of surveys of the Galactic plane have been made with the 100-m telescope at arc minute angular resolution. Surveys at 2695 MHz (|.| ≤ 5°) (Reich . 1990, Fürst . 1990) and at 1410 MHz (|.| ≤ 4°) (Reich . 1990) are public.作者: 植物群 時間: 2025-3-24 00:15 作者: 斜 時間: 2025-3-24 05:08
M. Harwitinal filtration process (Anchimbe .), those ways of speaking that they consider grotesque, foreign, and idiosyncratic. This pushes those speakers who may be interested in imitating foreign accents to adhere to local speech forms, i.e. Cameroon English accent. This contradiction in attitudes and ling作者: 黑豹 時間: 2025-3-24 07:44
M. Disney part of the mainstream norm of the variety, and should, when the time comes, be incorporated into its grammar during standardisation. This is because the forms are used by educated Cameroonians, the emergent native speakers of the variety (see Anchimbe .), and the accepted speakers of the variety (作者: 有說服力 時間: 2025-3-24 13:08 作者: heterodox 時間: 2025-3-24 16:37
C. A. Beichmaninal filtration process (Anchimbe .), those ways of speaking that they consider grotesque, foreign, and idiosyncratic. This pushes those speakers who may be interested in imitating foreign accents to adhere to local speech forms, i.e. Cameroon English accent. This contradiction in attitudes and ling作者: mitral-valve 時間: 2025-3-24 20:35 作者: Relinquish 時間: 2025-3-25 00:40 作者: 規(guī)章 時間: 2025-3-25 06:58
N. Broschusing a concrete damaged plasticity (CDP) model provided by the commercial finite element package ABAQUS, whose parameters are estimated by tension and compression tests. In addition, a systematic parametric study is performed to analyze the effects of ovality, thickness, and outer/inner radius rati作者: chiropractor 時間: 2025-3-25 08:02 作者: 不連貫 時間: 2025-3-25 14:52
P. K. Seidelmanndish dialect division, but shows that the phonological distinction between the two is best characterized in terms of tendencies rather than exact, regular correspondences. Beyond many other individual isoglosses in the data that cross-cut one another, there is a weak pattern of transition between th作者: Pruritus 時間: 2025-3-25 17:58 作者: 絕食 時間: 2025-3-25 23:17
B. Peng,W. Yuan,R. Nan,Y. Yann this case, the InAs dots were grown at 520?°C with a growth rate of 0.1?MLs.. Growth pauses of 0, 25 and 50?s were introduced for samples A, B and C, respectively. Finally, single-pixel photodetector devices were fabricated from as-grown A, B and C samples with standard fabrication procedures.作者: debunk 時間: 2025-3-26 00:08
B. Peng,R. Nanscusses sub-monolayer (SML) growth technique to grow QDs. This recent technique has been proven to improve the device performance significantly. The contents of this monograph will prove useful to researchers and professionals alike.?.978-981-13-5466-3978-981-10-5702-1作者: 課程 時間: 2025-3-26 07:40 作者: Osteoarthritis 時間: 2025-3-26 09:57 作者: Carbon-Monoxide 時間: 2025-3-26 14:28
K. P. Sokolov-uniformly weighted edges). The corresponding network energy is the cumulative distribution function for the node degree. This distribution reveals a phase transition for the temperature dependence. The Debye model thus provides a new way to describe the node degree distribution in both unweighted a作者: indemnify 時間: 2025-3-26 19:40
S. A. Trushkin-uniformly weighted edges). The corresponding network energy is the cumulative distribution function for the node degree. This distribution reveals a phase transition for the temperature dependence. The Debye model thus provides a new way to describe the node degree distribution in both unweighted a作者: 脾氣暴躁的人 時間: 2025-3-27 00:27 作者: 虛構(gòu)的東西 時間: 2025-3-27 01:28
(Kurmani-Bahdini and Sorani), with some consideration of Southern Kurdish. The book will be of interest to students and scholars in fields such as?linguistics, linguistic typology, Iranian linguistics and lingu978-3-030-78839-1978-3-030-78837-7作者: 作繭自縛 時間: 2025-3-27 07:34
Conference proceedings 1998s have formidable data acquisition,processing, archiving, and data distribution demands and this meetingprovided a forum for sharing experiences amongst workers specializingin different wavebands as well as discussing how multibandobservations can reveal fundamental relationships in our understandingof the Universe.作者: 共同時代 時間: 2025-3-27 09:33
Electronic Optical Sky Surveyses us telescopes on which we expect sub-arcsecond images a large fraction of the time. Finally, and perhaps most important, the performance of computer hardware continues to advance, to the point where analysis of multi-terabyte datasets, while still daunting, is at least conceivable.作者: 搬運(yùn)工 時間: 2025-3-27 13:58
1743-9213 nces amongst workers specializingin different wavebands as well as discussing how multibandobservations can reveal fundamental relationships in our understandingof the Universe.978-0-7923-4803-0978-94-009-1485-8Series ISSN 1743-9213 Series E-ISSN 2352-2186 作者: 不幸的人 時間: 2025-3-27 21:00 作者: Suppository 時間: 2025-3-27 22:03 作者: 是貪求 時間: 2025-3-28 03:17 作者: Kidney-Failure 時間: 2025-3-28 07:37
New Horizons from Multi-Wavelength Sky Surveys978-94-009-1485-8Series ISSN 1743-9213 Series E-ISSN 2352-2186 作者: Devastate 時間: 2025-3-28 11:50 作者: Conscientious 時間: 2025-3-28 16:42
https://doi.org/10.1007/978-94-009-1485-8astrometry; astronomy; data acquisition; databases; galaxies; photometry; solar system; star; star formation作者: 無關(guān)緊要 時間: 2025-3-28 20:44
Selection Effects and Biasesy referring to the narrow optical and 21-cm windows with which I am familiar, to argue that the he was quite wrong. We still haven’t covered the whole spectrum, and in any case prejudices, biases and selection effects could still veil much of the truth from sight.作者: figure 時間: 2025-3-29 02:16
Ultraviolet Sky Surveysion of faint objects does not compete against an enhanced background (O’Connell 1987) and the telescope construction techniques are very similar (at least longward of ~50 nm) to those of optical astronomy.作者: 解凍 時間: 2025-3-29 04:53 作者: 包庇 時間: 2025-3-29 07:45 作者: 輕信 時間: 2025-3-29 12:22 作者: A保存的 時間: 2025-3-29 18:53
Selection Effects and Biasesy referring to the narrow optical and 21-cm windows with which I am familiar, to argue that the he was quite wrong. We still haven’t covered the whole spectrum, and in any case prejudices, biases and selection effects could still veil much of the truth from sight.作者: 運(yùn)動吧 時間: 2025-3-29 22:14 作者: antipsychotic 時間: 2025-3-30 00:33 作者: Integrate 時間: 2025-3-30 07:41 作者: flammable 時間: 2025-3-30 11:02 作者: 慌張 時間: 2025-3-30 15:17 作者: CHOIR 時間: 2025-3-30 19:08
Gamma Ray Sky Surveysme surveys performed over limited energy bands and/or over portions of the sky. These include the HEAO-A4 hard X-ray survey and the COS-B and SAS-2 high-energy gamma-ray surveys. The early work forms a basis for understanding and appreciating the . results, and so is reviewed in Section 2.作者: Ischemia 時間: 2025-3-31 00:39 作者: obligation 時間: 2025-3-31 01:16 作者: Vsd168 時間: 2025-3-31 08:27
The Miyun 232 MHz General Cataloguee), has been conducted with the Miyun Synthesis Radio Telescope operating at 232 MHz. The reduced Miyun General Catalogue contains 34,426 radio sources in total. To distinguish which sources were not observed by other sky surveys, we first identify sources in the MGC with those in the 6C (151 MHz) c作者: 不可思議 時間: 2025-3-31 11:01
Kilometer-Square Area Radio Synthesis Telescope200 MHz and 2 GHz, is to construct a passive spherical reflector array of about 30 individual unit telescopes, each ~ 300 m diameter (Butcher 1995). Valleys amid the hills of southwest China would be ideal for such LT concept. We refer to this effort as the Kilometer-square Area Radio Synthesis Tele作者: overhaul 時間: 2025-3-31 17:08
Radio Continuum Surveys Above 2 GHzrt 1995, Jonas . 1996). This is the highest frequency and highest angular resolution (HPBW = 20’) all-sky radio continuum survey made using a ground-based telescope. The la noise level is better than 30 mK. A high-pass filtered image of the data is shown in Figure 1.作者: 石墨 時間: 2025-3-31 18:49 作者: 變化無常 時間: 2025-3-31 23:57 作者: 打算 時間: 2025-4-1 02:16 作者: 蘑菇 時間: 2025-4-1 09:33
Denis: a Deep Near Infrared Southern Sky Surveyd arcsecond resolution using the ESO 1 meter telescope at La Siila, Chile. The DENIS operations have started in December 1995 after a . period of one year mainly dedicated to technical tests and pilot surveys of selected regions of high astronomical interest. In September 1996, approximately 3000 sq作者: PANG 時間: 2025-4-1 12:49
tional scientists.Also available online: http://www.landolt-This volume provides structural data of selected proteins, physical and chemical properties of amino acids, peptides and proteins, and information on theoretical studies. The pace at which new data are being generated in the biological scie
