. . . . "Neuvedeno."@en . . . . "0"^^ . "N\u00EDzkoenergetick\u00E1 emise zdroj\u016F kosmick\u00FDch z\u00E1blesk\u016F z\u00E1\u0159en\u00ED gama" . . "http://www.isvav.cz/projectDetail.do?rowId=GA205/99/0145"^^ . "0"^^ . . "Projekt, kter\u00FD sv\u00FDm zam\u011B\u0159en\u00EDm spad\u00E1 do oblasti astrofyziky vysok\u00FDch energi\u00ED, se zab\u00FDval podrobn\u00FDm studiem optick\u00E9ho spektra kosmick\u00FDch z\u00E1blesk\u016F z\u00E1\u0159en\u00ED gama. Jde st\u00E1le o pom\u011Brn\u011B aktu\u00E1ln\u00ED a sv\u00FDm zp\u016Fsobem i modern\u00ED t\u00E9ma sou\u010Dasn\u00E9 astrofyziky. V projektu byly"@cs . "GA205/99/0145" . "2003-04-01+02:00"^^ . "1"^^ . . . . . "Low-energy emmision of gamma ray burst sources"@en . . "Kosmick\u00E9 zdroje z\u00E1blesk\u016F z\u00E1\u0159en\u00ED gama p\u0159edstavuj\u00ED nejenergeti\u010Dt\u011Bj\u0161\u00ED zn\u00E1m\u00E9 erupce ve vesm\u00EDru a jsou pokl\u00E1d\u00E1ny za jednu z nejv\u011Bt\u0161\u00EDch astrofyzik\u00E1ln\u00EDch z\u00E1had na\u0161eho stolet\u00ED. Jsou pozorov\u00E1ny p\u0159ibli\u017En\u011B jednou denn\u011B a jejich podstata je dosud nezn\u00E1m\u00E1 .\u0158ada teoretick\u00FDch model\u016F p\u0159edpokl\u00E1d\u00E1, \u017Ee tyto jevy mohou b\u00FDt doprov\u00E1zeny emis\u00ED ve viditeln\u00E9m sv\u011Btle. A\u010Dkoli existuje dru\u017Eicov\u00E1 p\u0159ehl\u00EDdka oblohy v oblasti gama z\u00E1\u0159en\u00ED, simult\u00E1nn\u00ED a kvasisimult\u00E1nn\u00ED data ve viditeln\u00E9m sv\u011Btle jsou pro tyto jevy st\u00E1le mimo\u0159\u00E1dn\u011B vz\u00E1cn\u00E1. C\u00EDlem n\u00E1vrhu je poskytnout kvalitn\u00ED optick\u00E1 observa\u010Dn\u00ED data vyhovuj\u00EDc\u00ED soudob\u00FDm po\u017Eadavk\u016Fm dru\u017Eicov\u00FDch experiment\u016F, zejm\u00E9na co se t\u00FD\u010De zorn\u00E9ho pole a rychlosti akce. N\u00E1vrh je \u00FAzce zapojen do dru\u017Eicov\u00FDch aktivit (CGRO, HETE). C\u00EDleje z\u00EDskat optick\u00E1 m\u011B\u0159en\u00ED pro z\u00E1blesky detekovan\u00E9 t\u011Bmito dru\u017Eicemi a vyhodnotit je spole\u010Dn\u011B s dru\u017Eicov\u00FDmi daty. V\u011Bdeck\u00FDm c\u00EDlem je studium m\u00EDsta, vzd\u00E1lenosti a fyzik\u00E1ln\u00EDch model\u016F z\u00E1bleskov\u00FDch zdroj\u016F z\u00E1\u0159en\u00ED gama. Projekt je zapojen do \u0161irok\u00E9 mezi" . . "41"^^ . . "41"^^ . "Celestial Gamma ray bursts (GRB) represent the most luminous eruptions known in the Universe and are considered as one of largest astrophysical puzzles of this century. They are observed at a rate of approximately one per day and their origin and nature are still not known. Many theoretical models indicate that these bursts may be accompanied by optical emissions. Although all sky monitoring in gamma rays is carried out by satellites, the real-time and/or quasisimultaneous optical data for gamma ray bursts still are extremely rare. The aim of this proposal is to provide optical observational data meeting the recent satellite project requirements (FOV and rapid response). These activities are closely connected to the US satellite projects CGRO and HETE. The goal is to provide high quality follow up optical data for GRB detected by these satellite experiments and to evaluate them together with high energy satellite data. The fina"@en .