書目名稱Gravitational Wave Data Analysis影響因子(影響力)學(xué)科排名
書目名稱Gravitational Wave Data Analysis網(wǎng)絡(luò)公開度
書目名稱Gravitational Wave Data Analysis網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Gravitational Wave Data Analysis被引頻次
書目名稱Gravitational Wave Data Analysis被引頻次學(xué)科排名
書目名稱Gravitational Wave Data Analysis年度引用
書目名稱Gravitational Wave Data Analysis年度引用學(xué)科排名
書目名稱Gravitational Wave Data Analysis讀者反饋
書目名稱Gravitational Wave Data Analysis讀者反饋學(xué)科排名
作者: 不滿分子 時(shí)間: 2025-3-21 21:26
Narrating the Past through Theatree law to finite-difference calculations of gravitational waveforms, and to suggest new, more robust (but mathematically equivalent) means of extracting the gravitational waveforms from Newtonian finite-difference calculations.作者: 驚奇 時(shí)間: 2025-3-22 03:31 作者: 冷漠 時(shí)間: 2025-3-22 04:43 作者: 眨眼 時(shí)間: 2025-3-22 11:22 作者: jumble 時(shí)間: 2025-3-22 15:11 作者: jumble 時(shí)間: 2025-3-22 17:49 作者: 哎呦 時(shí)間: 2025-3-22 23:23
The Rate of Gravitational Collapse in the Milky Wayvents of interest to gravitational radiation astronomers. It is shown that the rate of historical supernovae has been under estimated, and is at least 1 per 10 years in our galaxy. The rate of supernovae in external galaxies is consistent with the historical rate, but the radio pulsar rate, of 1 per作者: Libido 時(shí)間: 2025-3-23 02:12
Gravitational Radiation from Rotating Stellar Core Collapseine accurately the gravitational waveform from the collapse and the efficiency of the collapse in converting binding energy into gravitational radiation, it is necessary that a simulation accurately model certain features of the collapse. One purpose of this paper is to examine the scenario for supe作者: uncertain 時(shí)間: 2025-3-23 05:40 作者: 出生 時(shí)間: 2025-3-23 10:31 作者: CHART 時(shí)間: 2025-3-23 17:17
A Review of the Statistical Theory of Signal Detectiond include the classical theory of hypothesis testing, detection of known signals in white noise, maximum likelihood estimation of unknown parameters, the application of nonlinear filtering in signal detection and the use of pre-whitening filters to handle correlated noise.作者: 平項(xiàng)山 時(shí)間: 2025-3-23 19:53 作者: Traumatic-Grief 時(shí)間: 2025-3-23 23:38
Sample Covariance Techniques in the Detection of Gravitational Wavesion of the Green’s or Impulse response function from the time delayed movement estimates using the Winer-Volterra expansion is discussed for linear and non linear systems. The effect of additive outliers on the power spectral density estimates is illustrated and recent reviews referred. Finally the 作者: 偽造 時(shí)間: 2025-3-24 06:06
Parametric Transducers and Quantum Nondemolition in Bar Detectorsre a quantum nondemolition observable and thus potentially exceed the “quantum limit” for bar detectors. A more immediate benefit of this type of transducer to the development of gravitational wave antennae is the reduction of the requirements on the electrical Q and the pump phase noise. We summari作者: 表皮 時(shí)間: 2025-3-24 08:20
Round Table Discussion — Gravitational Wave Detectorsss detectors using laser interferometry and the first concrete sign of a long baseline detector being funded has appeared in response to a proposal by the Orsay and Pisa groups to INFN in Italy. Bar detectors have continued to develop, with the possibility of having several bars operating in coincid作者: 繼而發(fā)生 時(shí)間: 2025-3-24 13:06
Spacecraft Gravitational Wave Experimentschnology involved is sophisticated, the “raw” sensitivity of current generation experiments has been insufficient to produce a detection. To extract the maximum information from the Doppler data requires careful consideration of noise statistics, of how the noises map into the Doppler frequency obse作者: impale 時(shí)間: 2025-3-24 18:14
Gravitational Wave Experiments with Resonant Antennase metric tensor perturbation h(t) at the antenna resonance. By means of proper optimum filters, like the Wiener filter, it is possible to reach a sensitivity which is basically limited by the noise of the electronic amplifier. For one cryogenic antenna with mass M=2300 kg and temperature T=20 mK the作者: tic-douloureux 時(shí)間: 2025-3-24 22:36
Gravitational Antenna Bandwidths and Cross Sectionstes. For monochromatic continuous signals, the new approach gives the same cross sections as derived in 1960..A new method for data recording and analysis is proposed. This gives bandwidths several orders larger than are available by recording the output of an optimal filter..Means are suggested for作者: CLAN 時(shí)間: 2025-3-25 00:00
Comparison of Bars and Interferometers: Detection of Transient Gravitational Radiationor the detection of gravitational-wave bursts (e.g., supernovas, particle- black hole interactions), the bar antenna shows its resonant nature with a sensitivity that is broadly peaked near the bar frequency, while the interferometer shows a smooth f. frequency response (for a fixed gravitational en作者: 高射炮 時(shí)間: 2025-3-25 05:32 作者: Crayon 時(shí)間: 2025-3-25 09:53
Present Pasts in Neo-Victorian Fictionvents of interest to gravitational radiation astronomers. It is shown that the rate of historical supernovae has been under estimated, and is at least 1 per 10 years in our galaxy. The rate of supernovae in external galaxies is consistent with the historical rate, but the radio pulsar rate, of 1 per作者: Judicious 時(shí)間: 2025-3-25 15:31
Narrating the Past through Theatreine accurately the gravitational waveform from the collapse and the efficiency of the collapse in converting binding energy into gravitational radiation, it is necessary that a simulation accurately model certain features of the collapse. One purpose of this paper is to examine the scenario for supe作者: pancreas 時(shí)間: 2025-3-25 18:51 作者: Entrancing 時(shí)間: 2025-3-25 21:47 作者: 吹氣 時(shí)間: 2025-3-26 01:08 作者: coagulate 時(shí)間: 2025-3-26 07:09 作者: paleolithic 時(shí)間: 2025-3-26 08:37 作者: 討厭 時(shí)間: 2025-3-26 13:40
Language, Knowledge and Reality,re a quantum nondemolition observable and thus potentially exceed the “quantum limit” for bar detectors. A more immediate benefit of this type of transducer to the development of gravitational wave antennae is the reduction of the requirements on the electrical Q and the pump phase noise. We summari作者: ANIM 時(shí)間: 2025-3-26 16:53 作者: 出血 時(shí)間: 2025-3-26 22:56 作者: overture 時(shí)間: 2025-3-27 04:14
,(Meta-)Fiktionalit?t und (Anti-)Illusion,e metric tensor perturbation h(t) at the antenna resonance. By means of proper optimum filters, like the Wiener filter, it is possible to reach a sensitivity which is basically limited by the noise of the electronic amplifier. For one cryogenic antenna with mass M=2300 kg and temperature T=20 mK the作者: 謊言 時(shí)間: 2025-3-27 09:09
Personale Identit?t als narrative Identit?ttes. For monochromatic continuous signals, the new approach gives the same cross sections as derived in 1960..A new method for data recording and analysis is proposed. This gives bandwidths several orders larger than are available by recording the output of an optimal filter..Means are suggested for作者: AVID 時(shí)間: 2025-3-27 10:20 作者: affluent 時(shí)間: 2025-3-27 16:50
https://doi.org/10.1057/9780230373235 in our Galaxy is fairly likely to occur before laser interferometric antennae reach the 10. sensitivity level; it would give a clearer neutrino signal and possibly a reliable detection by cryogenic bar detectors.作者: municipality 時(shí)間: 2025-3-27 18:54
,Einleitung: Marken sind Gespr?che,d include the classical theory of hypothesis testing, detection of known signals in white noise, maximum likelihood estimation of unknown parameters, the application of nonlinear filtering in signal detection and the use of pre-whitening filters to handle correlated noise.作者: Factual 時(shí)間: 2025-3-28 00:25 作者: 有組織 時(shí)間: 2025-3-28 05:59
A Review of the Statistical Theory of Signal Detectiond include the classical theory of hypothesis testing, detection of known signals in white noise, maximum likelihood estimation of unknown parameters, the application of nonlinear filtering in signal detection and the use of pre-whitening filters to handle correlated noise.作者: MILL 時(shí)間: 2025-3-28 10:16
Gravitational Wave Data Analysis978-94-009-1185-7Series ISSN 1389-2185 作者: 幼稚 時(shí)間: 2025-3-28 13:06 作者: Abnormal 時(shí)間: 2025-3-28 18:26 作者: Tartar 時(shí)間: 2025-3-28 22:19
,(Meta-)Fiktionalit?t und (Anti-)Illusion,nance curve; it can reach values up to 100 Hz if a low noise amplifier is available. Finally the Rome antenna is briefly described. This antenna has a sensitivity of the order of h. ? 10. and has operated for nine months.作者: OREX 時(shí)間: 2025-3-29 00:12
Gravitational Wave Experiments with Resonant Antennasnance curve; it can reach values up to 100 Hz if a low noise amplifier is available. Finally the Rome antenna is briefly described. This antenna has a sensitivity of the order of h. ? 10. and has operated for nine months.作者: Basilar-Artery 時(shí)間: 2025-3-29 03:06
Present Pasts in Neo-Victorian Fiction 1 per 10 years in our galaxy. The rate of supernovae in external galaxies is consistent with the historical rate, but the radio pulsar rate, of 1 per 4 years obtained from geometrical evolution, is an order of magnitude larger than expected from the supernova rate.作者: Anonymous 時(shí)間: 2025-3-29 10:39 作者: tenosynovitis 時(shí)間: 2025-3-29 14:03 作者: 死亡率 時(shí)間: 2025-3-29 18:17
The Rate of Gravitational Collapse in the Milky Way 1 per 10 years in our galaxy. The rate of supernovae in external galaxies is consistent with the historical rate, but the radio pulsar rate, of 1 per 4 years obtained from geometrical evolution, is an order of magnitude larger than expected from the supernova rate.作者: nullify 時(shí)間: 2025-3-29 23:47 作者: 天氣 時(shí)間: 2025-3-30 03:25 作者: 使苦惱 時(shí)間: 2025-3-30 06:43
Narrative Ans?tze in Beratung und Coachingpost-Newtonian amplitudes of the waves under the assumption that the detector is in the light-recycling configuration and that we use the matched filter technique to dig out the signal from the noise.作者: 能夠支付 時(shí)間: 2025-3-30 09:07
https://doi.org/10.1007/978-1-4039-7003-9epresentative antennas and are seen to be operating near sensitivities allowing Galactic observations. Finally, each detector technology holds promises for increased sensitivity which will allow for collaborative detection of sources as distant as the Virgo cluster.作者: inspiration 時(shí)間: 2025-3-30 14:47
Coalescing Binaries to Post-Newtonian Orderpost-Newtonian amplitudes of the waves under the assumption that the detector is in the light-recycling configuration and that we use the matched filter technique to dig out the signal from the noise.作者: Cocker 時(shí)間: 2025-3-30 18:14
Comparison of Bars and Interferometers: Detection of Transient Gravitational Radiationepresentative antennas and are seen to be operating near sensitivities allowing Galactic observations. Finally, each detector technology holds promises for increased sensitivity which will allow for collaborative detection of sources as distant as the Virgo cluster.作者: Brittle 時(shí)間: 2025-3-30 20:42
