. . . . . . . . . . . . . . . . . . . "L'astronomie des ph\u00E9nom\u00E8nes transitoire (nomm\u00E9e en anglais time domain astronomy), ou \u00E9tude des ph\u00E9nom\u00E8nes transitoires, est la branche de l'astronomie qui s'int\u00E9resse au changement des objets astronomiques au cours du temps. Ce changement peut \u00EAtre d\u00FB \u00E0 un mouvement (rotation, r\u00E9volution, etc.) ou \u00E0 un changement intrins\u00E8que de l'objet. Les objets et ph\u00E9nom\u00E8nes \u00E9tudi\u00E9s incluent les supernovas, les \u00E9toiles \u00E9ruptives, les sursauts gamma, les blazars et les noyaux actifs de galaxies. Selon les ph\u00E9nom\u00E8nes \u00E9tudi\u00E9s, l'astronomie des ph\u00E9nom\u00E8nes transitoires se subdivise en plusieurs branches :"@fr . . . . "Astronomia w dziedzinie czasu"@pl . "L'astronomie des ph\u00E9nom\u00E8nes transitoire (nomm\u00E9e en anglais time domain astronomy), ou \u00E9tude des ph\u00E9nom\u00E8nes transitoires, est la branche de l'astronomie qui s'int\u00E9resse au changement des objets astronomiques au cours du temps. Ce changement peut \u00EAtre d\u00FB \u00E0 un mouvement (rotation, r\u00E9volution, etc.) ou \u00E0 un changement intrins\u00E8que de l'objet. Les objets et ph\u00E9nom\u00E8nes \u00E9tudi\u00E9s incluent les supernovas, les \u00E9toiles \u00E9ruptives, les sursauts gamma, les blazars et les noyaux actifs de galaxies. Selon les ph\u00E9nom\u00E8nes \u00E9tudi\u00E9s, l'astronomie des ph\u00E9nom\u00E8nes transitoires se subdivise en plusieurs branches : \n* l'astronomie des ph\u00E9nom\u00E8nes transitoires dans le domaine des t\u00E9rahertz \n* ..."@fr . . . . . . . . . . . . . "Time-domain astronomy is the study of how astronomical objects change with time. Though the study may be said to begin with Galileo's Letters on Sunspots, the term now refers especially to variable objects beyond the Solar System. This may be due to movement or changes in the object itself. Common targets included are supernovae, pulsating stars, novas, flare stars, blazars and active galactic nuclei. Visible light time domain studies include OGLE, HAT-South, PanSTARRS, SkyMapper, ASAS, WASP, CRTS, and in a near future the LSST at the Vera C. Rubin Observatory."@en . "12157"^^ . . . . . 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"\u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0627\u0644\u0632\u0645\u0646\u064A \u0623\u0648 \u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0641\u064A \u0627\u0644\u0646\u0637\u0627\u0642 \u0627\u0644\u0632\u0645\u0646\u064A (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: Time domain astronomy)\u200F \u0647\u0648 \u0641\u0631\u0639 \u0645\u0646 \u0641\u0631\u0648\u0639 \u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0627\u0644\u0631\u0635\u062F\u064A \u064A\u0647\u062A\u0645 \u0628\u062F\u0631\u0627\u0633\u0629 \u0627\u0644\u0638\u0648\u0627\u0647\u0631 \u0648\u0627\u0644\u0623\u062D\u062F\u0627\u062B \u0627\u0644\u0641\u0644\u0643\u064A\u0629 \u0627\u0644\u0639\u0627\u0628\u0631\u0629 \u0648\u062F\u0631\u0627\u0633\u0629 \u0643\u064A\u0641\u064A\u0629 \u062A\u063A\u064A\u0631 \u0627\u0644\u0623\u062C\u0633\u0627\u0645 \u0627\u0644\u0641\u0644\u0643\u064A\u0629 \u0645\u0639 \u0645\u0631\u0648\u0631 \u0627\u0644\u0648\u0642\u062A. \u0628\u0633\u0628\u0628 \u062D\u0631\u0643\u062A\u0647\u0627 \u0623\u0648 \u0627\u0644\u062A\u063A\u064A\u064A\u0631\u0627\u062A \u0627\u0644\u062A\u064A \u062A\u0637\u0631\u0623 \u0639\u0644\u0649 \u0627\u0644\u062C\u0631\u0645 \u0627\u0644\u0641\u0644\u0643\u064A \u0646\u0641\u0633\u0647. \u0648\u062E\u0627\u0635\u0629 \u062A\u0644\u0643 \u0627\u0644\u062A\u064A \u062A\u062A\u062C\u0627\u0648\u0632 \u0627\u0644\u0646\u0638\u0627\u0645 \u0627\u0644\u0634\u0645\u0633\u064A. \u0627\u0644\u0623\u0647\u062F\u0627\u0641 \u0627\u0644\u0634\u0627\u0626\u0639\u0629 \u0627\u0644\u062A\u064A \u064A\u0634\u0645\u0644\u0647\u0627 \u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0627\u0644\u0632\u0645\u0646\u064A \u0647\u064A \u0627\u0644\u0645\u0633\u062A\u0639\u0631\u0627\u062A \u060C \u0627\u0644\u0645\u0633\u062A\u0639\u0631\u0627\u062A \u0627\u0644\u0623\u0639\u0638\u0645\u064A\u0629 \u060C \u0627\u0644\u0646\u062C\u0648\u0645 \u0627\u0644\u0645\u062A\u0648\u0647\u062C\u0629\u060C \u0646\u0648\u0627\u0629 \u0627\u0644\u0645\u062C\u0631\u0627\u062A \u0627\u0644\u0646\u0634\u0637\u0629 \u0648\u0627\u0644\u0646\u062C\u0648\u0645 \u0627\u0644\u0632\u0627\u0626\u0641\u0629 \u0627\u0644\u0645\u062A\u0648\u0647\u062C\u0629.\u0648\u064A\u0634\u0645\u0644 \u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0627\u0644\u0632\u0645\u0646\u064A \u062D\u0627\u0644\u064A\u0627 \u0638\u0647\u0648\u0631 \u0627\u0644\u0645\u0630\u0646\u0628\u0627\u062A\u060C \u0648\u0627\u0644\u0645\u062A\u063A\u064A\u0631\u0627\u062A \u0627\u0644\u0642\u064A\u0641\u0627\u0648\u064A\u0629. \u0627\u0644\u0623\u062F\u0648\u0627\u062A \u0627\u0644\u0645\u0633\u062A\u062E\u062F\u0645\u0629 \u0647\u064A \u0627\u0644\u0645\u0631\u0627\u0635\u062F \u0627\u0644\u0622\u0644\u064A\u0629 \u0648\u0627\u0644\u062A\u0635\u0646\u064A\u0641 \u0627\u0644\u062A\u0644\u0642\u0627\u0626\u064A \u0644\u0644\u0623\u062D\u062F\u0627\u062B \u0627\u0644\u0639\u0627\u0628\u0631\u0629\u060C \u0648\u0627\u0644\u0625\u062E\u0637\u0627\u0631\u0627\u062A \u0627\u0644\u0633\u0631\u064A\u0639\u0629 \u0645\u0646 \u0627\u0644\u0645\u0647\u062A\u0645\u064A\u0646 . \u0648\u064A\u0648\u0627\u062C\u0629 \u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0627\u0644\u0632\u0645\u0646\u064A \u0639\u062F\u0629 \u062A\u062D\u062F\u064A\u0627\u062A \u0645\u0646\u0647\u0627 \u062A\u062E\u0632\u064A\u0646 \u0627\u0644\u0643\u0645\u064A\u0629 \u0627\u0644\u0647\u0627\u0626\u0644\u0629 \u0645\u0646 \u0627\u0644\u0628\u064A\u0627\u0646\u0627\u062A \u0648\u0646\u0642\u0644\u0647\u0627\u060C \u0648\u062A\u0642\u0646\u064A\u0627\u062A \u0627\u0633\u062A\u062E\u0631\u0627\u062C \u0627\u0644\u0628\u064A\u0627\u0646\u0627\u062A\u060C \u0648\u0627\u0644\u062A\u0635\u0646\u064A\u0641\u060C \u0648\u0627\u0644\u0628\u064A\u0627\u0646\u0627\u062A \u063A\u064A\u0631 \u0627\u0644\u0645\u062A\u062C\u0627\u0646\u0633\u0629. \u0627\u0644\u0644\u0648\u062D\u0627\u062A \u0627\u0644\u0641\u0644\u0643\u064A\u0629 \u0627\u0644\u0642\u062F\u064A\u0645\u0629 \u0627\u0644\u0645\u0639\u0631\u0636\u0629 \u0645\u0646 \u0622\u0648\u0627\u062E\u0631 \u0627\u0644\u062B\u0645\u0627\u0646\u064A\u0646\u0627\u062A \u0648\u062D\u062A\u0649 \u0645\u0637\u0644\u0639 \u0627\u0644\u062A\u0633\u0639\u064A\u0646\u064A\u0627\u062A \u0627\u0644\u062A\u064A \u064A\u062D\u062A\u0641\u0638 \u0628\u0647\u0627 \u0645\u0631\u0635\u062F \u0643\u0644\u064A\u0629 \u0647\u0627\u0631\u0641\u0627\u0631\u062F \u064A\u062A\u0645 \u0631\u0642\u0645\u0646\u062A\u0647\u0627 \u0645\u0646 \u0642\u0628\u0644 \u0645\u0634\u0631\u0648\u0639 \u0647\u0627\u0631\u0641\u0627\u0631\u062F \u0627\u0644\u0648\u0635\u0648\u0644 \u0627\u0644\u0631\u0642\u0645\u064A \u0625\u0644\u0649 \u0645\u0626\u0629 \u0639\u0627\u0645 \u0645\u0646 \u0627\u0644\u0633\u0645\u0627\u0621 (Digital Access to a Sky Century @ Harvard) ."@ar . . . . . . . . . . "Astronomia w dziedzinie czasu \u2013 dzia\u0142 astronomii, zajmuj\u0105cy si\u0119 badaniem zmienno\u015Bci cia\u0142 niebieskich w czasie. Termin ten odnosi si\u0119 obecnie zw\u0142aszcza do zmiennych obiekt\u00F3w spoza Uk\u0142adu S\u0142onecznego. Zmienno\u015B\u0107 mo\u017Ce by\u0107 spowodowana ruchem lub fizycznymi zmianami samego obiektu. Typowymi obiektami zainteresowania s\u0105 supernowe, gwiazdy pulsuj\u0105ce, gwiazdy nowe, rozb\u0142yskowe, blazary i aktywne j\u0105dra galaktyk. Optyczne przegl\u0105dy nieba w dziedzinie czasu obejmuj\u0105 projekty, jak OGLE, HAT-South, PanSTARRS, , ASAS, WASP, oraz w niedalekiej przysz\u0142o\u015Bci LSST w ."@pl . . . . "\u6642\u57DF\u5929\u6587\u5B78"@zh . "\u6642\u57DF\u5929\u6587\u5B78\u662F\u7814\u7A76\u5929\u9AD4\u5982\u4F55\u96A8\u8457\u6642\u9593\u8B8A\u5316\uFF0C\u800C\u9019\u53EF\u80FD\u662F\u7531\u65BC\u5929\u9AD4\u7684\u904B\u52D5\uFF0C\u4E5F\u53EF\u80FD\u662F\u5929\u9AD4\u672C\u8EAB\u5728\u6539\u8B8A\uFF1A\u5305\u62EC\u8D85\u65B0\u661F\u3001\u7130\u661F\u3001\u8000\u8B8A\u9AD4\u3001\u548C\u6D3B\u8E8D\u661F\u7CFB\u6838\u3002\u4EE5\u53EF\u898B\u5149\u7814\u7A76\u6642\u57DF\u5929\u6587\u5B78\u7684\u6709\u3001\u5927\u578B\u7D9C\u5408\u5DE1\u5929\u671B\u9060\u93E1\uFF08LSST\uFF09\u3001\u6CDB\u661F\u8A08\u756B\uFF08PanSTARRS\uFF09\u3001\u3001\u3001\u548C\uFF08Catalina Real-time Transient Survey\uFF09\uFF1B\u5728\u96FB\u6CE2\u5929\u6587\u5B78\u9818\u57DF\u6709LOFAR\u5728\u89C0\u5BDFs\u3002\u96FB\u6CE2\u7814\u7A76\u6642\u57DF\u5929\u6587\u5B78\u5DF2\u7D93\u6709\u5F88\u9577\u7684\u6642\u9593\uFF0C\u5305\u62EC\u8108\u885D\u661F\u548C\u9583\u720D\u73FE\u8C61\u3002\uFF08Cherenkov Telescope Array\uFF09\u3001\u3001\u8CBB\u7C73\u3001\u3001\u570B\u969B\u4F3D\u746A\u5C04\u7DDA\u5929\u9AD4\u7269\u7406\u5BE6\u9A57\u5BA4\uFF08INTEGRAL\uFF09\u3001\u3001\u548C\u96E8\u71D5\u885B\u661F\u90FD\u5728\u5C0B\u627EX\u5C04\u7DDA\u548C\u03B3\u5C04\u7DDA\u7684\u77AC\u8B8A\u73FE\u8C61\u3002\u4F3D\u746A\u5C04\u7DDA\u66B4\u662F\u773E\u6240\u5468\u77E5\u7684\u9AD8\u80FD\u96FB\u78C1\u77AC\u8B8A\u3002 \u4F7F\u7528\u7684\u5DE5\u5177\u662F\u6A5F\u5668\u4EBA\u671B\u9060\u93E1\u3001\u81EA\u52D5\u5206\u985E\u77AC\u8B8A\u4E8B\u4EF6\u3001\u8FC5\u901F\u901A\u77E5\u611F\u8208\u8DA3\u7684\u4EBA\u548C\u6A5F\u69CB\u3002\u9583\u720D\u6BD4\u5C0D\u5169\u5F35\u5F71\u50CF\u53EF\u4EE5\u8B93\u4EBA\u5FEB\u901F\u7BE9\u6AA2\u51FA\u4E0D\u540C\u4E4B\u8655\uFF0C\u5F71\u50CF\u76F8\u6E1B\u4E4B\u524D\u9700\u8981\u6B78\u4E00\u5316\u8655\u7406\u3002\u6311\u6230\u5305\u62EC\u5927\u91CF\u8CC7\u6599\u7684\u8655\u7406\u3001\u5132\u5B58\u548C\u50B3\u8F38\u3001\u6578\u64DA\u6316\u6398\u6280\u8853\u3001\u5206\u985E\u3001\u4EE5\u53CA\u7570\u69CB\u8CC7\u6599\u3002 \u5F9E\u6B77\u53F2\u4E0A\u770B\uFF0C\u6642\u57DF\u5929\u6587\u5B78\u6E90\u81EA\u5F57\u661F\u7684\u51FA\u73FE\u548C\u9020\u7236\u8B8A\u661F\u3002\u54C8\u4F5B\u5927\u5B78\u5929\u6587\u53F0\u901A\u904E\uFF08DASCH\uFF0CDigital Access to a Sky Century @ Harvard\uFF09\u7684\u5C08\u6848\uFF0C\u5C071800\u5E74\u4EE3\u672B\u671F\u81F31900\u5E74\u4EE3\u521D\u671F\u66DD\u5149\u7684\u4E7E\u7248\u5F71\u50CF\u6578\u4F4D\u5316\u3002 \u5176\u5B83\u56E0\u70BA\u6642\u9593\u9020\u6210\u8B8A\u7570\u7684\u6709\u5C0F\u884C\u661F\u3001\u98DF\u3001\u3001\u884C\u661F\u51CC\u3001\u8B8A\u661F\u7B49\u7B49\u3002"@zh . . . . . . . "39304988"^^ . . "1108425789"^^ . "\u0639\u0644\u0645 \u0627\u0644\u0641\u0644\u0643 \u0627\u0644\u0632\u0645\u0646\u064A"@ar . . . . . . "Time-domain astronomy is the study of how astronomical objects change with time. Though the study may be said to begin with Galileo's Letters on Sunspots, the term now refers especially to variable objects beyond the Solar System. This may be due to movement or changes in the object itself. Common targets included are supernovae, pulsating stars, novas, flare stars, blazars and active galactic nuclei. Visible light time domain studies include OGLE, HAT-South, PanSTARRS, SkyMapper, ASAS, WASP, CRTS, and in a near future the LSST at the Vera C. Rubin Observatory. Time-domain astronomy studies transient astronomical events, often shortened by astronomers to a transients as well as various types of variable stars, including periodic, quasi-periodic, and that of changing behavior or type.Other causes of time variability are asteroids, high proper motion stars, planetary transits and comets. Transients characterize astronomical objects or phenomena whose duration of presentation may be from milliseconds to days, weeks, or even several years. This is in contrast to the timescale of the millions or billions of years during which the galaxies and their component stars in our universe have evolved. Singularly, the term is used for violent deep-sky events, such as supernovae, novae, dwarf nova outbursts, gamma-ray bursts, and tidal disruption events, as well as gravitational microlensing. Time-domain astronomy also involves long-term studies of variable stars and their changes on the timescale of minutes to decades. Variability studied can be intrinsic, including periodic or semi-regular pulsating stars, young stellar objects, stars with outbursts, asteroseismology studies; or extrinsic, which results from eclipses (in binary stars, planetary transits), stellar rotation (in pulsars, spotted stars), or gravitational microlensing events. Modern time-domain astronomy surveys often uses robotic telescopes, automatic classification of transient events, and rapid notification of interested people. Blink comparators have long been used to detect differences between two photographic plates, and image subtraction became more used when digital photography eased the normalization of pairs of images. Due to large fields of view required, the time-domain work involves storing and transferring a huge amount of data. This includes data mining techniques, classification, and the handling of heterogeneous data. The importance of the time-domain astronomy was recognized in 2018 by German Astronomical Society by awarding a Karl Schwarzschild Medal to Prof. Andrzej Udalski for \"pioneering contribution to the growth of a new field of astrophysics research, time-domain astronomy, which studies the variability of brightness and other parameters of objects in the universe in different time scales.\"Also the 2017 Dan David Prize was awarded to the three leading researchers in the field of time-domain astronomy: Neil Gehrels (Swift Gamma-Ray Burst Mission), Shrinivas Kulkarni (Palomar Transient Factory), Andrzej Udalski (Optical Gravitational Lensing Experiment)."@en . . . . . "\u6642\u57DF\u5929\u6587\u5B78\u662F\u7814\u7A76\u5929\u9AD4\u5982\u4F55\u96A8\u8457\u6642\u9593\u8B8A\u5316\uFF0C\u800C\u9019\u53EF\u80FD\u662F\u7531\u65BC\u5929\u9AD4\u7684\u904B\u52D5\uFF0C\u4E5F\u53EF\u80FD\u662F\u5929\u9AD4\u672C\u8EAB\u5728\u6539\u8B8A\uFF1A\u5305\u62EC\u8D85\u65B0\u661F\u3001\u7130\u661F\u3001\u8000\u8B8A\u9AD4\u3001\u548C\u6D3B\u8E8D\u661F\u7CFB\u6838\u3002\u4EE5\u53EF\u898B\u5149\u7814\u7A76\u6642\u57DF\u5929\u6587\u5B78\u7684\u6709\u3001\u5927\u578B\u7D9C\u5408\u5DE1\u5929\u671B\u9060\u93E1\uFF08LSST\uFF09\u3001\u6CDB\u661F\u8A08\u756B\uFF08PanSTARRS\uFF09\u3001\u3001\u3001\u548C\uFF08Catalina Real-time Transient Survey\uFF09\uFF1B\u5728\u96FB\u6CE2\u5929\u6587\u5B78\u9818\u57DF\u6709LOFAR\u5728\u89C0\u5BDFs\u3002\u96FB\u6CE2\u7814\u7A76\u6642\u57DF\u5929\u6587\u5B78\u5DF2\u7D93\u6709\u5F88\u9577\u7684\u6642\u9593\uFF0C\u5305\u62EC\u8108\u885D\u661F\u548C\u9583\u720D\u73FE\u8C61\u3002\uFF08Cherenkov Telescope Array\uFF09\u3001\u3001\u8CBB\u7C73\u3001\u3001\u570B\u969B\u4F3D\u746A\u5C04\u7DDA\u5929\u9AD4\u7269\u7406\u5BE6\u9A57\u5BA4\uFF08INTEGRAL\uFF09\u3001\u3001\u548C\u96E8\u71D5\u885B\u661F\u90FD\u5728\u5C0B\u627EX\u5C04\u7DDA\u548C\u03B3\u5C04\u7DDA\u7684\u77AC\u8B8A\u73FE\u8C61\u3002\u4F3D\u746A\u5C04\u7DDA\u66B4\u662F\u773E\u6240\u5468\u77E5\u7684\u9AD8\u80FD\u96FB\u78C1\u77AC\u8B8A\u3002 \u4F7F\u7528\u7684\u5DE5\u5177\u662F\u6A5F\u5668\u4EBA\u671B\u9060\u93E1\u3001\u81EA\u52D5\u5206\u985E\u77AC\u8B8A\u4E8B\u4EF6\u3001\u8FC5\u901F\u901A\u77E5\u611F\u8208\u8DA3\u7684\u4EBA\u548C\u6A5F\u69CB\u3002\u9583\u720D\u6BD4\u5C0D\u5169\u5F35\u5F71\u50CF\u53EF\u4EE5\u8B93\u4EBA\u5FEB\u901F\u7BE9\u6AA2\u51FA\u4E0D\u540C\u4E4B\u8655\uFF0C\u5F71\u50CF\u76F8\u6E1B\u4E4B\u524D\u9700\u8981\u6B78\u4E00\u5316\u8655\u7406\u3002\u6311\u6230\u5305\u62EC\u5927\u91CF\u8CC7\u6599\u7684\u8655\u7406\u3001\u5132\u5B58\u548C\u50B3\u8F38\u3001\u6578\u64DA\u6316\u6398\u6280\u8853\u3001\u5206\u985E\u3001\u4EE5\u53CA\u7570\u69CB\u8CC7\u6599\u3002 \u5F9E\u6B77\u53F2\u4E0A\u770B\uFF0C\u6642\u57DF\u5929\u6587\u5B78\u6E90\u81EA\u5F57\u661F\u7684\u51FA\u73FE\u548C\u9020\u7236\u8B8A\u661F\u3002\u54C8\u4F5B\u5927\u5B78\u5929\u6587\u53F0\u901A\u904E\uFF08DASCH\uFF0CDigital Access to a Sky Century @ Harvard\uFF09\u7684\u5C08\u6848\uFF0C\u5C071800\u5E74\u4EE3\u672B\u671F\u81F31900\u5E74\u4EE3\u521D\u671F\u66DD\u5149\u7684\u4E7E\u7248\u5F71\u50CF\u6578\u4F4D\u5316\u3002 \u5176\u5B83\u56E0\u70BA\u6642\u9593\u9020\u6210\u8B8A\u7570\u7684\u6709\u5C0F\u884C\u661F\u3001\u98DF\u3001\u3001\u884C\u661F\u51CC\u3001\u8B8A\u661F\u7B49\u7B49\u3002"@zh . . . . . . . . . "Astronomie des ph\u00E9nom\u00E8nes transitoires"@fr . "Astronomia w dziedzinie czasu \u2013 dzia\u0142 astronomii, zajmuj\u0105cy si\u0119 badaniem zmienno\u015Bci cia\u0142 niebieskich w czasie. Termin ten odnosi si\u0119 obecnie zw\u0142aszcza do zmiennych obiekt\u00F3w spoza Uk\u0142adu S\u0142onecznego. Zmienno\u015B\u0107 mo\u017Ce by\u0107 spowodowana ruchem lub fizycznymi zmianami samego obiektu. Typowymi obiektami zainteresowania s\u0105 supernowe, gwiazdy pulsuj\u0105ce, gwiazdy nowe, rozb\u0142yskowe, blazary i aktywne j\u0105dra galaktyk. Optyczne przegl\u0105dy nieba w dziedzinie czasu obejmuj\u0105 projekty, jak OGLE, HAT-South, PanSTARRS, , ASAS, WASP, oraz w niedalekiej przysz\u0142o\u015Bci LSST w ."@pl . . . . . . . . . . . . . . . . . . . . . . . . . "Time-domain astronomy"@en . . . . . . . . . . .