. . . . . "[BBZ2012]A1703-zD6"@en . . . . ""@en . "A1703 zD6"@en . "A1703 zD6 is a strongly lensed Lyman-alpha emitter. It is located behind a foreground galaxy cluster known as , hence its name. It has a spectroscopically determined redshift of over 7, corresponding to a light travel time of 12.9 billion years. It is located in the Canes Venatici constellation. It was discovered in 2012, by a group led by L. D. Bradley, published in The Astrophysical Journal. The C IV emission line (with a wavelength of 1548 \u00C5) was detected from this galaxy, signifying triply ionized carbon. Because it takes high amounts of energy to triply ionize carbon, it may suggest that A1703 zD6 has an active galactic nucleus (AGN), or a population of very young, hot, and metal-poor stars. Subsequent investigations found that the ionization source is likely to be the latter: a cluster of stars (abbreviated SF, for star-forming region)."@en . . . . . . . "A1703-zD6"@it . . . "3611"^^ . . "A1703-zD6 \u00E8 una galassia remota con redshift di z = 7,045 che corrisponde ad una distanza percorsa dalla luce per giungere fino alla Terra di 12,89 miliardi di anni luce. Fa parte di un gruppo di sette galassie con z>7 identificate per mezzo dell'ammasso di galassie con il metodo del lensing gravitazionale."@it . . . "A1703 zD6"@en . "A1703 zD6 \u0647\u0648 \u0628\u0627\u0639\u062B \u0644\u064A\u0645\u0627\u0646 \u0623\u0644\u0641\u0627 \u0634\u062F\u064A\u062F \u064A\u0642\u0639 \u062E\u0644\u0641 \u0639\u062F\u0633\u0629 \u0627\u0644\u062C\u0627\u0630\u0628\u064A\u0629. \u062A\u0642\u0639 \u062E\u0644\u0641 \u0645\u062C\u0645\u0648\u0639\u0629 \u0645\u062C\u0631\u0627\u062A \u0641\u064A \u0627\u0644\u0645\u0642\u062F\u0645\u0629 \u062A\u064F\u0639\u0631\u0641 \u0628\u0627\u0633\u0645 Abell 1703 \u060C \u0648\u0645\u0646 \u0647\u0646\u0627 \u062C\u0627\u0621\u062A \u062A\u0633\u0645\u064A\u062A\u0647\u0627. \u0644\u0647\u0627 \u0627\u0646\u0632\u064A\u0627\u062D \u0623\u062D\u0645\u0631 \u0645\u062D\u062F\u062F \u0637\u064A\u0641\u064A\u064B\u0627 \u064A\u0632\u064A\u062F \u0639\u0646 7 \u060C \u064A\u062A\u0648\u0627\u0641\u0642 \u0645\u0639 \u0632\u0645\u0646 \u0627\u0646\u062A\u0642\u0627\u0644 \u0627\u0644\u0636\u0648\u0621 \u064A\u0628\u0644\u063A 12.9 \u0645\u0644\u064A\u0627\u0631 \u0633\u0646\u0629. \u064A\u0642\u0639 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0633\u0644\u0648\u0642\u064A\u0627\u0646 . \u062A\u0645 \u0627\u0643\u062A\u0634\u0627\u0641\u0647 \u0641\u064A \u0639\u0627\u0645 2012 \u060C \u0645\u0646 \u0642\u0628\u0644 \u0645\u062C\u0645\u0648\u0639\u0629 \u0628\u0642\u064A\u0627\u062F\u0629 LD Bradley \u060C \u0648\u0646\u064F\u0634\u0631 \u0641\u064A The Astrophysical Journal ."@ar . "A1703-zD6 \u00E8 una galassia remota con redshift di z = 7,045 che corrisponde ad una distanza percorsa dalla luce per giungere fino alla Terra di 12,89 miliardi di anni luce. Fa parte di un gruppo di sette galassie con z>7 identificate per mezzo dell'ammasso di galassie con il metodo del lensing gravitazionale."@it . . "J2000"@en . "A1703 zD6"@ar . . "A1703 zD6"@en . . . . . "A1703 zD6"@en . . . . "25.8"^^ . "A1703 zD6 \u0647\u0648 \u0628\u0627\u0639\u062B \u0644\u064A\u0645\u0627\u0646 \u0623\u0644\u0641\u0627 \u0634\u062F\u064A\u062F \u064A\u0642\u0639 \u062E\u0644\u0641 \u0639\u062F\u0633\u0629 \u0627\u0644\u062C\u0627\u0630\u0628\u064A\u0629. \u062A\u0642\u0639 \u062E\u0644\u0641 \u0645\u062C\u0645\u0648\u0639\u0629 \u0645\u062C\u0631\u0627\u062A \u0641\u064A \u0627\u0644\u0645\u0642\u062F\u0645\u0629 \u062A\u064F\u0639\u0631\u0641 \u0628\u0627\u0633\u0645 Abell 1703 \u060C \u0648\u0645\u0646 \u0647\u0646\u0627 \u062C\u0627\u0621\u062A \u062A\u0633\u0645\u064A\u062A\u0647\u0627. \u0644\u0647\u0627 \u0627\u0646\u0632\u064A\u0627\u062D \u0623\u062D\u0645\u0631 \u0645\u062D\u062F\u062F \u0637\u064A\u0641\u064A\u064B\u0627 \u064A\u0632\u064A\u062F \u0639\u0646 7 \u060C \u064A\u062A\u0648\u0627\u0641\u0642 \u0645\u0639 \u0632\u0645\u0646 \u0627\u0646\u062A\u0642\u0627\u0644 \u0627\u0644\u0636\u0648\u0621 \u064A\u0628\u0644\u063A 12.9 \u0645\u0644\u064A\u0627\u0631 \u0633\u0646\u0629. \u064A\u0642\u0639 \u0641\u064A \u0643\u0648\u0643\u0628\u0629 \u0627\u0644\u0633\u0644\u0648\u0642\u064A\u0627\u0646 . \u062A\u0645 \u0627\u0643\u062A\u0634\u0627\u0641\u0647 \u0641\u064A \u0639\u0627\u0645 2012 \u060C \u0645\u0646 \u0642\u0628\u0644 \u0645\u062C\u0645\u0648\u0639\u0629 \u0628\u0642\u064A\u0627\u062F\u0629 LD Bradley \u060C \u0648\u0646\u064F\u0634\u0631 \u0641\u064A The Astrophysical Journal . \u062A\u0645 \u0627\u0643\u062A\u0634\u0627\u0641 \u062E\u0637 \u0627\u0646\u0628\u0639\u0627\u062B C IV (\u0628\u0637\u0648\u0644 \u0645\u0648\u062C\u0629 1548 \u00C5 ) \u0645\u0646 \u0647\u0630\u0647 \u0627\u0644\u0645\u062C\u0631\u0629 \u060C \u0645\u0645\u0627 \u064A\u062F\u0644 \u0639\u0644\u0649 \u0627\u0644\u0643\u0631\u0628\u0648\u0646 \u0627\u0644\u0645\u062A\u0623\u064A\u0646 \u062B\u0644\u0627\u062B\u064A\u064B\u0627. \u0648\u0646\u0638\u0631\u064B\u0627 \u0644\u0623\u0646\u0647 \u064A\u062A\u0637\u0644\u0628 \u0643\u0645\u064A\u0627\u062A \u0643\u0628\u064A\u0631\u0629 \u0645\u0646 \u0627\u0644\u0637\u0627\u0642\u0629 \u0644\u062A\u0623\u064A\u0646 \u0627\u0644\u0643\u0631\u0628\u0648\u0646 \u062B\u0644\u0627\u062B\u064B\u0627 \u060C \u0641\u0642\u062F \u064A\u0634\u064A\u0631 \u0630\u0644\u0643 \u0625\u0644\u0649 \u0623\u0646 A1703 zD6 \u064A\u062D\u062A\u0648\u064A \u0639\u0644\u0649 \u0646\u0648\u0627\u0629 \u0645\u062C\u0631\u0629 \u0646\u0634\u0637\u0629 \u0623\u0648 \u0645\u062C\u0645\u0648\u0639\u0629 \u0645\u0646 \u0627\u0644\u0646\u062C\u0648\u0645 \u0627\u0644\u0635\u063A\u064A\u0631\u0629 \u062C\u062F\u064B\u0627 \u0648\u0627\u0644\u0633\u0627\u062E\u0646\u0629 \u0648\u0627\u0644\u0641\u0642\u064A\u0631\u0629 \u0628\u0627\u0644\u0645\u0639\u0627\u062F\u0646 . \u0648\u062C\u062F\u062A \u0627\u0644\u062F\u0631\u0627\u0633\u0627\u062A \u0627\u0644\u0644\u0627\u062D\u0642\u0629 \u0623\u0646 \u0645\u0635\u062F\u0631 \u0627\u0644\u062A\u0623\u064A\u0646 \u0645\u0646 \u0627\u0644\u0645\u062D\u062A\u0645\u0644 \u0623\u0646 \u064A\u0643\u0648\u0646 \u0627\u0644\u0623\u062E\u064A\u0631: \u0645\u062C\u0645\u0648\u0639\u0629 \u0645\u0646 \u0627\u0644\u0646\u062C\u0648\u0645 \u0641\u064A \u0645\u0646\u0637\u0642\u0629 \u062A\u0634\u0643\u0644 \u0627\u0644\u0646\u062C\u0648\u0645."@ar . . "7.045"^^ . . "48436388"^^ . . . . "[BBZ2012] A1703-zD6"@en . . . . . "1086545673"^^ . "A1703 zD6 is a strongly lensed Lyman-alpha emitter. It is located behind a foreground galaxy cluster known as , hence its name. It has a spectroscopically determined redshift of over 7, corresponding to a light travel time of 12.9 billion years. It is located in the Canes Venatici constellation. It was discovered in 2012, by a group led by L. D. Bradley, published in The Astrophysical Journal."@en . . .