標題: Titlebook: Data Analysis in Astronomy IV; V. Gesù,L. Scarsi,H. U. Zimmermann Book 1992 Springer Science+Business Media New York 1992 astronomy.astrop [打印本頁] 作者: 磨損 時間: 2025-3-21 19:51
書目名稱Data Analysis in Astronomy IV影響因子(影響力)
書目名稱Data Analysis in Astronomy IV影響因子(影響力)學(xué)科排名
書目名稱Data Analysis in Astronomy IV網(wǎng)絡(luò)公開度
書目名稱Data Analysis in Astronomy IV網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Data Analysis in Astronomy IV被引頻次
書目名稱Data Analysis in Astronomy IV被引頻次學(xué)科排名
書目名稱Data Analysis in Astronomy IV年度引用
書目名稱Data Analysis in Astronomy IV年度引用學(xué)科排名
書目名稱Data Analysis in Astronomy IV讀者反饋
書目名稱Data Analysis in Astronomy IV讀者反饋學(xué)科排名
作者: 座右銘 時間: 2025-3-21 22:01 作者: Aesthete 時間: 2025-3-22 03:12
https://doi.org/10.1007/978-1-4615-3388-7astronomy; astrophysics; cosmic ray; photometry; telescope作者: Traumatic-Grief 時間: 2025-3-22 07:58
978-1-4613-6496-2Springer Science+Business Media New York 1992作者: 一起 時間: 2025-3-22 10:46
Ettore Majorana International Science Serieshttp://image.papertrans.cn/d/image/262663.jpg作者: 針葉類的樹 時間: 2025-3-22 15:27
Dysfunctional Immune Regulatory System,A few thoughts are presented on astronomical databases and archives from a user point of view. Shortcomings and possible future trends are also mentioned, as well as some considerations on a future ideal environment for direct home applications on real and remotely located astronomical data.作者: 針葉類的樹 時間: 2025-3-22 20:32 作者: TAIN 時間: 2025-3-22 23:03 作者: IRS 時間: 2025-3-23 02:50 作者: 諂媚于人 時間: 2025-3-23 07:30 作者: refraction 時間: 2025-3-23 09:50 作者: Fluctuate 時間: 2025-3-23 14:11
Matthew Davenport,Laura E. Dickinson Ph.D.later the ROSAT telescope began its operation with an observation of the central parts of the Large Magellanic Cloud. This long awaited event marked the begin of a new phase in X-ray astronomy during that an extension of our present database on X-ray sources by an order of magnitude is expected.作者: colostrum 時間: 2025-3-23 18:25 作者: 截斷 時間: 2025-3-24 00:51 作者: 解脫 時間: 2025-3-24 04:25 作者: 偏狂癥 時間: 2025-3-24 08:19
https://doi.org/10.1007/978-1-4684-4826-9 soon replace the IHAP system at ESO’s New Technology Telescope (NTT) when the NTT will be used also under remote control from ESO Headquarters in Garching. Observers will then have all utilities of a modern astronomical data analysis system at their finger tips, at the telescope..This paper describ作者: intercede 時間: 2025-3-24 14:33
Chronic Venous Disorders of the Lower Limbse form of two-dimensional images of the physical world and consists of measurements which are dependent on factors such as the imaging geometry, illumination, and structures present in the world. The goal of any vision system is to recognize familiar structures in the system’s environment, and obtai作者: creatine-kinase 時間: 2025-3-24 15:26 作者: ORE 時間: 2025-3-24 22:29
Jeffrey M. Rhodes,Peter Gloviczkith-independent. It has been used to analyse data from the Einstein Observatory, EXOSAT and Ginga, as well as optical photometry and helioseismology data. In the currently available version (No. 2.0), XRONOS includes programs for: light curve(s), hardness ratio and colour-colour plotting, epoch foldi作者: Macronutrients 時間: 2025-3-25 01:32
Venous Anatomy of the Lower Limbdge about spacial and kinematical characteristics of stellar populations. The tasks and the present state of the MEGA program has been described recently by Malyuto, Einasto, Kharchenko and Schilbach (1990). The use of absolute proper motions of stars (with respect to galaxies), photoelectric UBVR a作者: 類型 時間: 2025-3-25 04:30
A. L. P. Caforio,N. G. Mahon,W. J. McKennahe primary mirror suffers from spherical aberration. The resulting image quality is considerably below the design specifications, and causes a loss of sensitivity of approximately 2.5 magnitudes. Fortunately, the HST point spread function retains a sharp core having almost the nominal diffraction-li作者: ONYM 時間: 2025-3-25 09:00 作者: 強行引入 時間: 2025-3-25 14:16
A. L. P. Caforio,N. G. Mahon,W. J. McKennahe Hubble Space Telescope. STSDAS achieves system independence by being fully layered on the Image Reduction and Analysis Facility (IRAF) developed at the National Optical Astronomy Observatories. STSDAS augments the general capabilities of IRAF, and along with other IRAF-based analysis packages suc作者: Diuretic 時間: 2025-3-25 17:27 作者: scrutiny 時間: 2025-3-25 21:10
Matthew Davenport,Laura E. Dickinson Ph.D.later the ROSAT telescope began its operation with an observation of the central parts of the Large Magellanic Cloud. This long awaited event marked the begin of a new phase in X-ray astronomy during that an extension of our present database on X-ray sources by an order of magnitude is expected.作者: 失敗主義者 時間: 2025-3-26 00:47
https://doi.org/10.1007/978-3-030-10698-0ute for Extraterrestrial Physics (MPE), which provides the scientific and calibration program input, and the German Space Operations Center (GSOC), whose responsibility it is to generate a mission timeline satisfying all operational constraints. An optimum solution for the mission timeline is achiev作者: 符合規(guī)定 時間: 2025-3-26 05:01 作者: 健談 時間: 2025-3-26 09:34
Chronically Evolving Viral Hepatitisax-Planck Institut für Extraterrestrische Physik (MPE, Garching). As has been elaborated in a previous contribution the Standard Processing performs two major tasks: in a first step data are normalized and calibrated and then a Standard Image and Source Analysis is performed. The Principal Investiga作者: Amplify 時間: 2025-3-26 16:01 作者: remission 時間: 2025-3-26 18:44
HST Image Restoration - Status and Prospectsds, hardly seen before in optical astronomy. The characteristics of the aberrated point-spread function together with the stochastic properties of quantum-limited data have lead to the recognition of statistical algorithms as the methods of choice for HST image restoration.作者: Asparagus 時間: 2025-3-26 23:32 作者: 擴大 時間: 2025-3-27 01:57 作者: 滴注 時間: 2025-3-27 07:16
The ROSAT Data Archive and other Project Applications of a DBMSdard processing (SASS) of ROSAT data. The DBMS got used for a number of ’normal’ applications like mission planning (J.Schmid/S.Snowden) and the ROSAT proposal utility MIPS (J.Behnke GSFC). This paper discusses three ’hybride’ applications which split the transaction into data retrieval, execution of VMS commands and update of the database:作者: 燒烤 時間: 2025-3-27 13:26 作者: Champion 時間: 2025-3-27 17:18
Jeffrey M. Rhodes,Peter Gloviczkita. In the currently available version (No. 2.0), XRONOS includes programs for: light curve(s), hardness ratio and colour-colour plotting, epoch folding, power spectrum, autocorrelation, crosscorrelation, time skewness and statistical analysis.作者: cajole 時間: 2025-3-27 19:11
A. L. P. Caforio,N. G. Mahon,W. J. McKenna the National Optical Astronomy Observatories. STSDAS augments the general capabilities of IRAF, and along with other IRAF-based analysis packages such as the PROS system for X-ray data analysis from the Harvard-Smithsonian Center for Astrophysics, provides a broad suite of astronomical software within a common environment.作者: 自負的人 時間: 2025-3-28 00:05
P. Liu,K. Fuse,G. Chu,Y. Liu,A. Opavskyservative, having a low detection rate combined with a low false alarm rate. The classical k-nearest neighbours method offers a versatile and broad-ranging alternative. With the rather homogeneous input data used, the various multilayer perceptron algorithms used did not appear to offer advantages over the variants of k-nearest neighbours.作者: invert 時間: 2025-3-28 06:03 作者: exquisite 時間: 2025-3-28 08:36
STSDAS: The Space Telescope Science Data Analysis System the National Optical Astronomy Observatories. STSDAS augments the general capabilities of IRAF, and along with other IRAF-based analysis packages such as the PROS system for X-ray data analysis from the Harvard-Smithsonian Center for Astrophysics, provides a broad suite of astronomical software within a common environment.作者: accrete 時間: 2025-3-28 13:47 作者: 衰老 時間: 2025-3-28 17:27
Venous Anatomy of the Lower Limbnd Vilnius photometry together with automated quantitative spectral classification for large stellar-statistical samples are among the most essential features of the programme. The data are gathered in 47 areaswithin 30. from the main meridional section of the Galaxy.作者: 表主動 時間: 2025-3-28 21:30 作者: 刻苦讀書 時間: 2025-3-29 00:02
https://doi.org/10.1007/978-1-4684-4826-9ew. An overview is given of the design goals for the functionality of the future, combined software environment at ESO telescopes: instrument control, data acquisition, ‘quick-look’ data analysis and full on-line data reduction. Possible implementations are discussed.作者: metropolitan 時間: 2025-3-29 06:08
A. L. P. Caforio,N. G. Mahon,W. J. McKennan can still be met. Following the installation of corrective optics on the first shuttle servicing mission, with the subsequent installation of second-generation scientific instruments with built-in corrective optics, the full scientific potential of HST should be realized.作者: 無法破譯 時間: 2025-3-29 09:43
Chronically Evolving Viral Hepatitis be fully satisfied with the findings of the Standard Analysis and therefore wish to proceed with a more detailed data evaluation on his own. It is for this kind of investigation that we have developed the Extended Scientific Analysis System (EXSAS).作者: neoplasm 時間: 2025-3-29 14:37 作者: institute 時間: 2025-3-29 17:38
MIDAS on-Line at the Telescopeew. An overview is given of the design goals for the functionality of the future, combined software environment at ESO telescopes: instrument control, data acquisition, ‘quick-look’ data analysis and full on-line data reduction. Possible implementations are discussed.作者: 按時間順序 時間: 2025-3-29 22:31 作者: Canyon 時間: 2025-3-30 02:05
Interactive Analysis with EXSAS be fully satisfied with the findings of the Standard Analysis and therefore wish to proceed with a more detailed data evaluation on his own. It is for this kind of investigation that we have developed the Extended Scientific Analysis System (EXSAS).作者: Jogging 時間: 2025-3-30 08:03
Chronic Venous Disorders of the Lower Limbsiant for certain changes in the physical world [3]. In many computer vision applications, invariance against the following factors is required [3]: (i) sensor noise; (ii) optical distortion; (iii) viewpoint; (iv) perspective distortion; and (v) variations in photometric conditions.作者: 結(jié)合 時間: 2025-3-30 09:04
Markov Random Field Applications in Image Analysisiant for certain changes in the physical world [3]. In many computer vision applications, invariance against the following factors is required [3]: (i) sensor noise; (ii) optical distortion; (iii) viewpoint; (iv) perspective distortion; and (v) variations in photometric conditions.作者: 虛情假意 時間: 2025-3-30 16:18 作者: 前兆 時間: 2025-3-30 20:08
Book 1992 Center for Scientific Culture, Erice, Sicily, Italy, on April 12-19, 1991. The Workshop was preceded by three workshops on the same subject held in Erice in 1984, 1986 and 1988. The frrst workshop (Erice 1984) was dominated by presentations of "Systems for Data Analysis"; the main systems proposed 作者: calorie 時間: 2025-3-30 22:09
Astrophysics Data Systemuction of large and highly sensitive detector arrays in the visible and infrared, the development of several 8-m ground based optical telescopes, and the completion of the Very Large Baseline Array (VLBA) radio telescopes will start this process. A large amount of astrophysical data has already been作者: NEEDY 時間: 2025-3-31 01:28 作者: Negligible 時間: 2025-3-31 05:45
Markov Random Field Applications in Image Analysise form of two-dimensional images of the physical world and consists of measurements which are dependent on factors such as the imaging geometry, illumination, and structures present in the world. The goal of any vision system is to recognize familiar structures in the system’s environment, and obtai
