派博傳思國(guó)際中心

標(biāo)題: Titlebook: Astronomical Time Series; Proceedings of The F Dan Maoz,Amiel Sternberg,Elia M. Leibowitz Conference proceedings 1997 Springer Science+Busi [打印本頁]

作者: hormone-therapy 時(shí)間: 2025-3-21 18:47
書目名稱Astronomical Time Series影響因子(影響力)

書目名稱Astronomical Time Series影響因子(影響力)學(xué)科排名

書目名稱Astronomical Time Series網(wǎng)絡(luò)公開度

書目名稱Astronomical Time Series網(wǎng)絡(luò)公開度學(xué)科排名

書目名稱Astronomical Time Series被引頻次

書目名稱Astronomical Time Series被引頻次學(xué)科排名

書目名稱Astronomical Time Series年度引用

書目名稱Astronomical Time Series年度引用學(xué)科排名

書目名稱Astronomical Time Series讀者反饋

書目名稱Astronomical Time Series讀者反饋學(xué)科排名

作者: Measured 時(shí)間: 2025-3-21 21:25

作者: frugal 時(shí)間: 2025-3-22 00:36
Observations of Millisecond Pulsars on Time Scales from 10 Nanoseconds to 10 Yearsthe discovery of pulsars, which produce arguably the most famous astronomical time series (Hewish .., 1968). The diversity and richness of science that has developed from observations of pulsars could never have been foreseen by their discoverers. Most of this science is deduced from detailed studie

作者: FER 時(shí)間: 2025-3-22 05:38
Microlensing: Current Results and Future Prospectsalf that required to explain the dark matter, but the estimated MACHO mass (~ 0.4 M.) is most consistent with stars that should have been seen. Toward the bulge, the total mass is consistent with that given by dynamical estimates of the bulge mass, but the observed timescales seem to require that a

作者: inundate 時(shí)間: 2025-3-22 09:44
Image Subtraction in Time Series Analysis: Application to Microlensing and Light Echoeserture photometry). Often the field containing the source is extremely crowded, or the source is extended. We describe techniques that we have developed in order to follow changes in such sources, utilizing the technique of image subtraction. In this way the stable flux in a field can be subtracted

作者: 舔食 時(shí)間: 2025-3-22 13:22
Desperately Seeking Non-Gaussianitynity, therefore, than in the light curve of 0957+561, the gravitational lens that, until recently, had yielded frustratingly inconsistent determinations of its lag. We discuss the difficulties in measuring deviations from Gaussianity in weakly nonstationary processes (such as 1/. noise or random wal

作者: 平息 時(shí)間: 2025-3-22 18:33

作者: Friction 時(shí)間: 2025-3-23 01:04
Reverberation Mapping and the Physics of Active Galactic Nuclei, enabled mapping of the gas distribution around the central black hole, and are starting to resolve the continuum source structure. This review describes the recent and successful campaigns of the International AGN Watch consortium, outlines the theoretical background of reverberation mapping and t

作者: liposuction 時(shí)間: 2025-3-23 02:50
Echo Mapping of X-Ray Binaries and Active Galactic Nuclei). In these systems radiation from a compact variable source drives responses in the surrounding medium. We outline maximum entropy techniques used to find smooth delay maps that fit incomplete and noisy measurements of the driving and responding lightcurves. In AGNs, erratically variable ionizing f

作者: Radiation 時(shí)間: 2025-3-23 07:01

作者: carotid-bruit 時(shí)間: 2025-3-23 12:40
Radial Velocity Detections of Extra-Solar Planetsar planets will improve dramatically our understanding of the formation of planets and planetary systems, which was based till the last decade on the sole example of the solar system. Nevertheless, no extra-solar planet was convincingly detected until recently. This is so because planets are very fa

作者: 旅行路線 時(shí)間: 2025-3-23 15:20

作者: Tailor 時(shí)間: 2025-3-23 21:01

作者: ERUPT 時(shí)間: 2025-3-24 01:08
Tests of Irregularly Sampled Stochastic Time Series for AGN collected by the AGN WATCH, using more data, to obtain reverberation results for more objects, one will have to rely on irregularly sampled lightcurves. Previous analyses of irregularly sampled observations suggest that it is possible to obtain results from such data sets. To evaluate the statistic

作者: 噱頭 時(shí)間: 2025-3-24 02:30
Wavelet Transforms of Flickering Light Curves in Cataclysmic Variabless up to more than an entire magnitude in others. This phenomenon is known as flickering. Phenomenologically, it appears as a continuous series of overlapping flares in the light curves. For a comprehensive review, see Bruch (1992). As an example, Fig. 1 shows a light curve of the novalike variable V

作者: 小故事 時(shí)間: 2025-3-24 09:54
Fast Computation of Trigonometric Sums with Applications to the Frequency Analysis of Astronomical D..., . and for the full grid .., ., . = 0,..., . ? 1 of frequencies. The similar approach is known from radio astronomy in the context of synthesis imaging. However, when the so-called “gridding” is method to obtain relatively crude interpolations from unequally spaced two dimensional measurements (

作者: Density 時(shí)間: 2025-3-24 11:14

作者: Collected 時(shí)間: 2025-3-24 15:12

作者: FECT 時(shí)間: 2025-3-24 19:44

作者: Coronation 時(shí)間: 2025-3-25 00:30

作者: scrutiny 時(shí)間: 2025-3-25 07:06

作者: 徹底檢查 時(shí)間: 2025-3-25 10:50

作者: 易彎曲 時(shí)間: 2025-3-25 15:25

作者: rectocele 時(shí)間: 2025-3-25 17:39
Klaus Backhaus,Bernd Erichson,Rolf Weibers up to more than an entire magnitude in others. This phenomenon is known as flickering. Phenomenologically, it appears as a continuous series of overlapping flares in the light curves. For a comprehensive review, see Bruch (1992). As an example, Fig. 1 shows a light curve of the novalike variable V422 Oph.

作者: Painstaking 時(shí)間: 2025-3-25 20:12

作者: ENNUI 時(shí)間: 2025-3-26 02:38

作者: Aqueous-Humor 時(shí)間: 2025-3-26 05:18

作者: 隱藏 時(shí)間: 2025-3-26 09:02

作者: Eulogy 時(shí)間: 2025-3-26 16:00
https://doi.org/10.1007/978-3-322-97546-1the discovery of pulsars, which produce arguably the most famous astronomical time series (Hewish .., 1968). The diversity and richness of science that has developed from observations of pulsars could never have been foreseen by their discoverers. Most of this science is deduced from detailed studie

作者: 注視 時(shí)間: 2025-3-26 18:01
https://doi.org/10.1007/978-3-642-69614-5alf that required to explain the dark matter, but the estimated MACHO mass (~ 0.4 M.) is most consistent with stars that should have been seen. Toward the bulge, the total mass is consistent with that given by dynamical estimates of the bulge mass, but the observed timescales seem to require that a

作者: 擔(dān)心 時(shí)間: 2025-3-26 21:58
https://doi.org/10.1007/978-3-642-69614-5erture photometry). Often the field containing the source is extremely crowded, or the source is extended. We describe techniques that we have developed in order to follow changes in such sources, utilizing the technique of image subtraction. In this way the stable flux in a field can be subtracted

作者: Hiatal-Hernia 時(shí)間: 2025-3-27 04:17
https://doi.org/10.1007/978-3-642-69614-5nity, therefore, than in the light curve of 0957+561, the gravitational lens that, until recently, had yielded frustratingly inconsistent determinations of its lag. We discuss the difficulties in measuring deviations from Gaussianity in weakly nonstationary processes (such as 1/. noise or random wal

作者: Freeze 時(shí)間: 2025-3-27 05:26
https://doi.org/10.1007/978-3-642-69614-5avelengths constitutes the best proof that the object is indeed a gravitational lens, because microlensing and other subtle effects cause the spectra, colors and other instantaneous properties of the multiple images of a lensed quasar to be not strictly identical. Observation of a random pattern of

作者: Pelvic-Floor 時(shí)間: 2025-3-27 10:43
https://doi.org/10.1007/978-3-642-69614-5, enabled mapping of the gas distribution around the central black hole, and are starting to resolve the continuum source structure. This review describes the recent and successful campaigns of the International AGN Watch consortium, outlines the theoretical background of reverberation mapping and t

作者: 指數(shù) 時(shí)間: 2025-3-27 17:19

作者: cylinder 時(shí)間: 2025-3-27 19:02

作者: obsession 時(shí)間: 2025-3-28 00:51
https://doi.org/10.1007/978-3-658-11380-3ar planets will improve dramatically our understanding of the formation of planets and planetary systems, which was based till the last decade on the sole example of the solar system. Nevertheless, no extra-solar planet was convincingly detected until recently. This is so because planets are very fa

作者: 枯燥 時(shí)間: 2025-3-28 03:24
Zusammenfassung und Diskussion,ding. This process is examined in the broad context of scientific measurement in general, in the context of quantum mechanics, along with the contruction of models to match the behavior observed. The relationship between classical and quantum phenomena is placed in a new framework where each is seen

作者: ADAGE 時(shí)間: 2025-3-28 08:34

作者: acrimony 時(shí)間: 2025-3-28 11:19
,Analyse bin?rer abh?ngiger Variablen, collected by the AGN WATCH, using more data, to obtain reverberation results for more objects, one will have to rely on irregularly sampled lightcurves. Previous analyses of irregularly sampled observations suggest that it is possible to obtain results from such data sets. To evaluate the statistic

作者: 否認(rèn) 時(shí)間: 2025-3-28 15:32
Klaus Backhaus,Bernd Erichson,Rolf Weibers up to more than an entire magnitude in others. This phenomenon is known as flickering. Phenomenologically, it appears as a continuous series of overlapping flares in the light curves. For a comprehensive review, see Bruch (1992). As an example, Fig. 1 shows a light curve of the novalike variable V

作者: Adjourn 時(shí)間: 2025-3-28 20:40
Klaus Backhaus,Bernd Erichson,Rolf Weiber..., . and for the full grid .., ., . = 0,..., . ? 1 of frequencies. The similar approach is known from radio astronomy in the context of synthesis imaging. However, when the so-called “gridding” is method to obtain relatively crude interpolations from unequally spaced two dimensional measurements (

作者: 撫育 時(shí)間: 2025-3-29 02:07

作者: 感染 時(shí)間: 2025-3-29 04:19

作者: 慟哭 時(shí)間: 2025-3-29 07:57

作者: Crayon 時(shí)間: 2025-3-29 11:44
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/b/image/163606.jpg

作者: Heresy 時(shí)間: 2025-3-29 16:36
0067-0057 t fundamental effect that impress a. human being, or, in fact, most living creatures on this planet. An echo of this idea. can be heard in the Biblical story of978-90-481-4895-0978-94-015-8941-3Series ISSN 0067-0057 Series E-ISSN 2214-7985

作者: 有抱負(fù)者 時(shí)間: 2025-3-29 23:27
https://doi.org/10.1007/978-3-642-69614-5bject as 0957+561, the detectability of any deviation from Gaussian is problematical at best. At present, one can rule out a wedge model only if the individual shots are as infrequent as one in 10–20 days.

作者: 一個(gè)姐姐 時(shí)間: 2025-3-30 03:28
https://doi.org/10.1007/978-3-658-42221-9r the orbital radius would equal the Schwarzschild-geometry general-relativistic marginally stable orbit (12.5 km for a 1.4M. object). So far all models that have been put forward for explaining the new phenomenon have encountered problems. In this paper I review the relatively simple and highly sug

作者: propose 時(shí)間: 2025-3-30 07:21
Klaus Backhaus,Bernd Erichson,Rolf Weiber/EquationSource>=δ. spans the .. dimensional model subspace in the n dimensional space of the

作者: 季雨 時(shí)間: 2025-3-30 08:57
Conference proceedings 1997y that astronomical time series preceeded astronomy itself, as the impression of the day /night cycle on Earth is probably the first and most fundamental effect that impress a. human being, or, in fact, most living creatures on this planet. An echo of this idea. can be heard in the Biblical story of

作者: Inclement 時(shí)間: 2025-3-30 13:28

作者: Lumbar-Stenosis 時(shí)間: 2025-3-30 17:34

作者: 合法 時(shí)間: 2025-3-30 21:12

作者: 忘川河 時(shí)間: 2025-3-31 04:13

作者: Communal 時(shí)間: 2025-3-31 06:56

作者: dagger 時(shí)間: 2025-3-31 10:32

作者: 波動(dòng) 時(shí)間: 2025-3-31 13:23
https://doi.org/10.1007/978-3-322-97546-1actic nuclei, and gamma-ray bursts. State space representations, or Kalman filtering, provide a powerful mathematical environment for study of nonstationary, nonlinear, quasi-periodic, unevenly spaced, and Poisson time series in astronomy.

作者: abnegate 時(shí)間: 2025-3-31 18:52

作者: 木質(zhì) 時(shí)間: 2025-3-31 21:51

作者: 隱語 時(shí)間: 2025-4-1 02:05
https://doi.org/10.1007/978-3-658-11380-3int relative to their parent stars, with brightness ratios that can get as low as 10.—the luminosity ratio for the case of Jupiter and the Sun. With present technology it is therefore next to impossible to image directly any extra-solar planet residing inside the overpowering glare of its parent star.

作者: 尖 時(shí)間: 2025-4-1 06:26

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